Nonmonotonic External Field Dependence of the Magnetization in a Finite Ising Model Theory
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Experimental evidence for an angular dependent transition of magnetization reversal modes in magnetic nanotubesOle Albrecht, Robert Zierold, Sebastián Allende, Juan Escrig, Christian Patzig et al.Citation: J. Appl. Phys. 109, 093910 (2011); doi: 10.1063/1.3583666View online: /10.1063/1.3583666View Table of Contents: /resource/1/JAPIAU/v109/i9Published by the AIP Publishing LLC.Additional information on J. Appl. Phys.Journal Homepage: /Journal Information: /about/about_the_journalTop downloads: /features/most_downloadedInformation for Authors: /authorsDownloaded 27 Sep 2013 to 202.207.14.58. This article is copyrighted as indicated in the abstract. Reuse of AIP content is subject to the terms at: /about/rights_and_permissionsExperimental evidence for an angular dependent transition of magnetization reversal modes in magnetic nanotubesOle Albrecht,1Robert Zierold,1Sebastia´n Allende,2,3Juan Escrig,3,4Christian Patzig,5Bernd Rauschenbach,5Kornelius Nielsch,1and Detlef Go¨rlitz1,a)1Institute of Applied Physics,University of Hamburg,Jungiusstrasse11,D-20355Hamburg,Germany2Departamento de Fı´sica,FCFM Universidad de Chile,Casilla487-3,8370415Santiago,Chile3Center for the Development of Nanoscience and Nanotechnology(CEDENNA),Avda.Ecuador3493,9170124Santiago,Chile4Departamento de Fı´sica,Universidad de Santiago de Chile(USACH),Avda.Ecuador3493,9170124Santiago,Chile5Leibniz-Institute of Surface Modification,Permoserstrasse15,D-04318Leipzig,Germany(Received7February2011;accepted29March2011;published online9May2011)We report on the experimental and theoretical investigation of the magnetization reversal inmagnetic nanotubes that have been synthesized by a combination of glancing angle and atomiclayer ing superconducting quantum interference device magnetometry the angulardependence of the coercivefields is determined and reveals a nonmonotonic behavior.Analyticalcalculations predict the crossover between two magnetization reversal modes,namely,themovement of different types of domain boundaries(vortex wall and transverse wall).Thistransition,already known in the geometrical dependences of the magnetization reversal in variousnanotubes,is found within one type of tube in the angular dependence and is experimentallyconfirmed in this work.V C2011American Institute of Physics.[doi:10.1063/1.3583666]I.INTRODUCTIONHighly anisotropic magnetic nanostructures can be used to overcome the superparamagnetic limit found in spherical nanomagnets1,2such as magnetic nanowires and nanotubes. Several methods for the preparation3–6of wires and their magnetic properties7–11have been described in the last dec-ade.Whereas wirelike structures offer two geometric param-eters,namely length and radius,that can be independently adjusted to influence the magnetic properties,tubular struc-tures allow for the variation of an additional degree of free-dom:the wall thickness.To benefit from this fact a detailed understanding of the magnetization reversal processes in such structures is of great importance.A very convenient route for the fabrication of tubular nanostructures is the use of a porous alumina membrane12,13as a template for a subsequent covering with magnetic material.Atomic layer deposition14,15and electrodeposition16,17are among the most prominent techniques used for such template preparation. Recently,Albrecht et al.18synthesized arrays of magnetic nanotubes by using the combination of glancing angle depo-sition(GLAD)and atomic layer deposition(ALD).The magnetic measurements on nanotubes have mostly been performed by superconducting quantum interference device(SQUID)or vibrating sample magnetometry(VSM) parallel or perpendicular to the long axis of the tube.19–22 Bachmann et al.23investigated the influence of the magnetic layer thickness in arrays of nanotubes on the reversal mode. For an applied magneticfield parallel to the long axis of the tubes they discovered a transition between two reversal modes that depends on the material and the geometrical parameters.Allende et al.24theoretically predicted a nonmonotonic behavior of the angular dependent coercivefield in a mag-netic nanotube,and explained this feature by a transition between a domain wall of a vortex and a transverse domain wall at a specific angle between the long axis of the tube and the applied magneticfield.In this work we present a combined experimental and analytical investigation of the angle dependent magnetiza-tion reversal in Fe3O4nanotubes.Glancing angle deposition was used to deposit Si columns on a Si substrate.The tech-nique allows for a deposition of nearly arbitrarily shaped structures by using self-shadowing effects.Subsequently,a magnetic tubular layer of Fe3O4was deposited by atomic layer deposition.The deposited layer thickness is close to a reported thickness dependent transition of the magnetization reversal modes.23The ALD technique is capable of produc-ing layers with a high thickness accuracy.As a simple exam-ple for the combined GLAD-ALD synthesis,here we present straight columns inclined to the substrate as a mechanical support structure for the Fe3O4nanotubes that are aligned neither parallel nor perpendicular to the substrate to avoid in-cidental substrate effects.A detailed description of the syn-thesis of the sample investigated here and the structural characterization of those nanotubes including TEM images has been given in a recent publication.18The investigated sample,the experimental setup,and the main results of the angular dependent measurements are described in Sec.II.Models of different modes of magnet-ization reversal in nanotube modes are discussed in Sec.III. In Sec.IV the experimentally obtained values of the coercive field are compared to the theoretical predictions.a)Author to whom correspondence should be addressed.Electronic mail:goerlitz@physnet.uni-hamburg.de.0021-8979/2011/109(9)/093910/5/$30.00V C2011American Institute of Physics109,093910-1JOURNAL OF APPLIED PHYSICS109,093910(2011)II.EXPERIMENTALWe investigate a sample with a mechanical support struc-ture consisting of inclined Si columns of b¼ð5762Þ grown on a Si substrate.The cylindrically shaped Si columns with a length ofð14006190Þnm have a mean radius of r¼ð6066Þnm and are covered with a Fe3O4layer of a thickness,RÀr¼ð1061Þnm.Thus,nanotubes of length ð14006190Þnm are produced by the ALD-process and the ratio of inner and outer radius of the Fe3O4tubes is g¼r=R%0:86.The layer thickness has been measured by x-ray reflectometry(XRR)on aflatfilm produced under the same conditions.As verified by XPS,electron diffraction,and high-resolution transmission electron microscopy in recent publications19,25,26the ALD synthesis yields a complete layer of magnetite,Fe3O4.It should be noted that the support struc-ture is needed to ensure the stability of the nanotube array and is retained for all subsequent investigations.Figure1(a)dis-plays a SEM micrograph of the investigated structure,and Fig.1(b)depicts a schematic drawing of the relevant direc-tions and angles in a single inclined nanotube synthesized on a substrate.The plane of the substrate is defined by the axes,x and y.The inclination of the structure to the substrate is described by b,i.e.,the angle between the surface normal,z,and the direction of the long axis of the tube,z0.The rotation around the y axis is described by the angle,c.The rotation of the tube around this axis is characterized by two extreme con-figurations.At a certain angle the tube axis,i.e.,the easy axis, is parallel to the appliedfield,H,and,shifted further by90 , z0is perpendicular to H.To investigate the angle dependent magnetization reversal processes of the nanotube array at a temperature of300K. magnetization isotherms were recorded,using a commercial SQUID-magnetometer(MPMS-XL,Quantum Design)equipped with a rotatable sample holder that allowed for a rotation of the sample in the range of360 with an adjustable increment down to0:1 .As displayed in Fig.2,where the two promi-nent angles H k z0and H?z0are selected exemplary,the angular dependent coercivefields were extracted from these recordings.The full angular range of the coercivefields is displayed in Fig.3.Starting from point A,(c¼0 ),the coercivity slowly rises between c¼45 and c¼85 (Point B),fol-lowed by a sharp decrease with a prominent minimum at the angle,c¼125 (Point C).At this point,the tubes are perpen-dicular to the applied magneticfield,H,i.e.,the hard axis is aligned with H.By a further increase of the angle,c,the coercivity rises again until c¼153 (Point D),and decreases again.It should be noted that at points B and D the substrate is oriented in different angles with respect to theapplied FIG.1.(Color online)(a)Scanning electron micrographs of inclined Si col-umns with an inclination angle with respect to the substrate normalb¼ð5762Þ fabricated by glancing angle deposition.(b)Coordinatesystem which is used in the discussion:The inclination of the columns withrespect to the xy plane of the substrate is described by the angle,b.Theangle,c,defines the rotation axis of the sample in respect of the appliedfield,H.The inset in(b)displays a schematic top drawing of a tube withboth radii,namely the inner(r)and the outer(R)one.FIG.2.(Color online)Magnified part of magnetization isotherms of twoselected angles H k z0(~)and H?z0( ).From this recording the angulardependent coercivity,H c,and squareness SQ¼l r=l s were extracted.For amagneticfield applied parallel to the tube the isotherm reveals a squarenessof approximately73%.The squareness in the case of a perpendicular appliedfield reaches a value of22%.Inset:Two magnetization isotherms for anapplied magneticfield parallel(!)or perpendicular(^)to the substrateplane.FIG.3.(Color online)(a)Angular dependence of the coercivefield ofinclined columns(b¼5762) for aðH k x!z!ÀxÞrotation by theangle.c.Point A defines the starting angle of the measurement(c¼0 ).AtPoint B the appliedfield is perpendicular to the substrate plane.At the mini-mum of the coercivefield at c%125 (Point C),the columns are perpendic-ular to the appliedfield.At Point D the magnitude of the magnetizationcomponent parallel to the appliedfield is the same as at Point B.field.The nonmonotonic behavior between A and C or C and D,respectively,cannot originate from a magnetization rever-sal due to the movement of a single domain wall type,as will be shown shortly.III.MAGNETIZATION REVERSAL MODELSIn magnetic nanotubes the magnetization reversal can occur by a coherent rotation of all moments or by the nuclea-tion and movement of the domain walls.For tubes with a negligible impact of defects,three different reversal modes are possible.21,27These reversal modes are illustrated in Fig.4and correspond to the coherent rotation (left panel),where all magnetic moments simultaneously rotate;the vortex wall (center panel),where magnetic moments rotate progressively via propagation of a vortex domain wall (this mode is fre-quently called the curling reversal mode);and transverse wall (right scenario),where magnetic moments rotate pro-gressively via propagation of a transverse domain wall.As was pointed by Landeros et al.27the coherent reversal mode is only favorable for very short magnetic tubes where the length of the tube is in the same range as the wall width.21,27Since we are interested in high aspect ratio tubes we will focus our attention on the vortex and transverse reversal modes.Recently,Allende et al.24calculated the angular de-pendence of the transverse and vortex modes in magnetic nanotubes.We shortly review their approach and adapt it as a first model to describe the nonmonotonic angular behavior of the coercivity in our samples.The nucleation theory with its analytic solutions allows the determination of the wall nucleation field,which describes for each reversal mode (transverse and vortex)the field and functional form at which the magnetization just starts to deviate from the saturated state.By using the correlation between the coercive field and the nucleation field mentioned later,it is possible to calculate the coerciv-ity.From the experimental point of view,it is easier to extract the coercive field from the recorded measurements to compare it to the theoretically predicted values than to use the wall nucleation field.A.Transverse reversal modeRecently,Landeros et al.27calculated the total energy for the transverse reversal mode considering the sum of the exchange and dipolar contributions.Then,they minimized the energy with regard to the domain wall width,w T .How-ever,they only calculated energies and they could not calcu-late the nucleation or coercive field.To solve this problem,Escrig et al.21assumed that the nucleation field of a system that reverses its magnetization by means of the nucleation and propagation of a transverse wall is equivalent to the nucleation field of an equivalent system with an effective volume that reverses its magnetization by coherent rotation.Fortunately,Stoner and Wohlfarth 28discussed the angular dependence of a coherent magnetization reversal.Then,this model can be adapted 21,29to describe the angular depend-ence of a transverse reversal mode by replacing the length of the whole structure,in which the coherent rotation takes place,by the reduced length of the involved domain wall with width,w T .Thus we have introduced the effective vol-ume proposed by Escrig et al.21The geometry of the effec-tive volume is described by a demagnetization factor,N z ðw T Þ.27Using this value for the real nanotube in a first simple model leads to the following equation for the angular dependent nucleation fieldH Tnðh Þ¼À2K ðw T ÞþK a ½ l 0M 0ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi1Àt 2þt 4p 1þt M 0;(1)where t ¼tan 1=3h ðÞwith h being the angle between the longaxis of the tube and the applied field.Besides,K ðw T Þ¼14l 0M 201À3N z ðw T Þ½ is the shape anisotropy con-stant.In the original work of Escrig et al.,21K a denotes the magneto-crystalline anisotropy (MCA)constant.Since we have polycrystalline nanotubes in our case,the MCA is aver-aged out and we generalize K a to be a universal anisotropy constant K a .Stoner and Wohlfarth have shown 28that the coercivity expression can be written as a function of the nucleation field asj H T cðh Þj ¼j H T n ðh Þj 0 h p 42H T n p 4 Àj H T nðh Þj p 4 h p 28><>::(2)Figure 5(black dashed curve)displays the angular depend-ence of the coercive field,using Eqs.(1)and (2),for a trans-verse reversal mode.The parameters used for the analyticalcalculation are the geometric parameters described in Sec.II ;the saturation magnetization,M 0¼4:8Â105Am À1,at room temperature and a constant for the uniaxial anisotropy,K a ¼1:9Á104Jm À3,along the tube axis presumably caused by internal stress due to the production process.It should be noted that the used value corresponds to a stress induced uniaxial anisotropy in thin magnetite films on MgOofFIG.4.(Color online)Possible magnetization reversal modes in magnetic nanotubes of length,‘.The orientations of the local magnetic moments are displayed by the arrows.Left:coherent reversal mode.Center:vortex rever-sal mode,with a domain wall of thickness,w V .Right:transverse reversal mode,with a domain wall of thickness,w T .approximately 104J =m 3found by Margulies et al.30Fol-lowing Landeros et al.27the domain wall width can be esti-mated to be w T %65nm.The obtained curve shows a monotonic decrease of the coercive field from an applied field aligned along the tube axis to a perpendicularly applied field.B.Vortex mode magnetic reversalThe angular dependence of the curling nucleation field in a prolate spheroid has been calculated first by Aharoni 31in 1997.Escrig et al.29adapted the approach to calculate the switching field for finite nanotubes with demagnetization factors,N x ;y ;z ,describing the magnetic behavior in an applied field parallel to the tube axis.The authors used the exact geometry of hollow cylinders for the demagnetization and took into account the internal and external radii of the tubes.Their result,Eq.(5)in Ref.29,yields an angular de-pendence of the coercive field,which,however,does not include any other anisotropy term than the shape anisotropy.The effect of adding an anisotropy is essentially the same as that of changing the shape anisotropy by changing the aspect ratio.The effect is far from being negligible,and the anisot-ropy,along with the finite size,must be taken into account.In order to include the same uniaxial anisotropy along the tube axis as in the case of the transverse reversal mode,we adapted the calculations by Aharoni 31for the vortex nuclea-tion field in nanotubes with uniaxial anisotropy along the tube axisH Vnðh Þcos ðh Àx Þ¼N x ð‘Þsin 2ðx ÞþN z ð‘Þcos 2ðx ÞÀÀc Àd 3cos 2ðx ÞÀ1ÂÃÁM 0;(3a)H Vn ðh Þsin ðh Àx Þ¼N x ð‘ÞÀN z ð‘Þþd ½sin ð2x Þ2M 0;(3b)where c ¼q 2L 2ex =R 2;d ¼K a =l 0M 20;and q satisfies32qJ 0q ðÞÀJ 1q ðÞ01Àg qJ 0g q ðÞÀJ 1g q ðÞ01¼0:(4)Here,J p z ðÞand Y p z ðÞare Bessel functions of the first andsecond kind,respectively,L ex ¼ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi2A =l 0M 20p is the exchange length,‘is the tube length,R is the external radius of the tube,g is the ratio of the inner and outer tube radius,and the angle,x ,is the angle 31where the nucleation starts with respect to the tube axis.Equation (4)has an infinite number of solutions,where only the one with the smallest nucleation field has to be considered.33To obtain the nucleation field,H Vnðh Þ,we simultaneously numerically solved Eqs.(3a)and (3b)for each applied field angle,h .As pointed out by Aharoni,31a jump of the magnetization for an isolated system occurs at or near the vortex nucleation field.Therefore,the coercivity is quite close to the absolute value of the nucleation field and we assume here,as in other studies,19,31,34that in theV mode ÀH V nis a good approximation to the coercivity,H V c .This assumption is supported by the high squareness value (73%)of the magnetization isotherm obtained for the H k z (vortex regime),displayed in Fig.2.The angular dependence of the coercive field in the vor-tex regime was calculated with the same parameters as in the transverse one including the anisotropy term mentioned before and the exchange constant,A ¼1Â10À11Jm À1taken from Ref.35.Unlike the transverse reversal mode,it exhibits a monotonic increase of the coercive field up to 90 as shown in Fig.5(red solid curve).For symmetry reasons a mono-tonic decrease is obtained between 90 and 180 .Neither the sole consideration of the movement of a transverse or a vortex wall,respectively,can explain the non-monotonic behavior of the experimentally obtained depend-ence of the coercive field.IV.TRANSITION BETWEEN TRANSVERSE AND VORTEX REVERSAL MODEBy a combination of the angular dependences for the transverse and the vortex reversal modes considered above (the system will reverse its magnetization by whichever mode opens an energetically accessible route first,that is,by the mode that offers the lowest coercivity)we obtain a non-monotonic behavior of the angular dependence of the coer-cive field with distinct maxima and minima.As displayed in Fig.6,the calculation (solid lines)for the dominant majority of tubes with R ¼70nm and r ¼60nm exhibit crossing points at the same angles as the experimentally obtained maxima,which allows us to attribute them to a transition from a vortex to a transverse mode of magnetization rever-sal.21The prominent minimum is recovered by the calcula-tion for the transverse mode.It should be noted that for direct comparison with the theoretical results the experimen-tally derived curve is shifted in Fig.6with respect to Fig.3by the inclination angle,90 Àb ¼33 .We observe that the theoretical curves match the experimental data very well.The small shift of the experimental data points to higher val-ues,compared to the calculated curves at small angles,can possibly be explained by the deviation of the tubes’cross-FIG.5.(Color online)Angular dependence of the coercive field determined by analytical calculations for the vortex and transverse reversal mode between two prominent configurations.The applied field is parallel to the long axis of the tube at c ¼0 and perpendicular to the long axis of the tube at c ¼90 .The vortex mode (red solid line)exhibits a monotonic increase of the coercive field between the parallel and perpendicular configuration.In stark contrast to this,the coercive fields in the transverse mode (black dashed line)monotonically decrease.section from perfect circularity (see the inset to Fig.6).We at-tribute the deviations for larger angles as stemming from the magnetic (dipolar)interaction in the tube ensemble.It has been pointed out by Escrig et al.21that the dipolar interaction of neighboring tubes results in a lowering of the coercive fields.V.CONCLUSIONWe have presented a combined experimental and theo-retical investigation of a novel type of magnetic nanostruc-tures obtained by a preparative approach in which ALD is used to coat a template obtained by GLAD.By the angular dependent magnetization measurements,namely the extrac-tion of the coercive field from the magnetization isotherms,for these tubular structures we find experimental evidence for an angular dependent transition of magnetization reversal modes which have been theoretically predicted.Analytical calculations allow us to identify the transition between the vortex and the transverse reversal mode.Shamaila et al.36also observed a nonmonotonic angular dependent coercive field in thick-walled nanotubes,but in contrast to our results,they explained it by a transition between the vortex and the coherent reversal mode.Despite the fact that they explained the nonmonotonic behavior for the angular dependence of the coercivity,it is just a qualitative explanation and not a quantitative understanding such as the one we propose in this paper.However,the coherent rotation should only apply to extremely small (monodomain)particles.For somewhat larger particles,such as magnetic nanotubes,we have to con-sider transverse and vortex reversal modes.ACKNOWLEDGMENTSThe authors appreciate constructive discussions with J.Bachmann (Hamburg),and thank A.Zolotaryov (Hamburg)for the supporting XRR measurements.S.A.and J.E.acknowledge the support from Fondecyt under Grant Nos.3090047and 1110784,the Millennium Science Nucleus“Basic and Applied Magnetism”(Project No.P06-022-F),and Financiamiento Basal para Centros Cientı´ficos y Tecnolo ´-gicos de Excelencia.Financial support by the Deutsche For-schunsgemeinschaft under Grant Nos.FOR 522(C.P.,B.R.,and K.N.),SPP 1165(R.Z.and K.N.),and SFB 668(K.N.,O.A.,and S.A.)as well as financial support from the Free and Hanseatic City of Hamburg in the context of the “Landesexzellenzinitiative Hamburg”(Project “NAME,”R.Z.and K.N.)is gratefully acknowledged.1J.A.Christodoulides,Y.Zhang,G.C.Hadjipanayis,and C.Fountzoulas,IEEE Trans.Magn.36,2333(2000).2S.Sun,C.B.Murray,D.Weller,L.Folks,and A.Moser,Science 287,1989(2000).3K.Nielsch,R.B.Wehrspohn,J.Barthel,J.Kirschner,U.Go ¨sele,S.F.Fischer,and H.Kronmu ¨ller,Appl.Phys.Lett.79,1360(2001).4B.E.Alaca,H.Sehitoglu,and T.Saif,Appl.Phys.Lett.84,4669(2004).5K.Nielsch,R.Hertel,R.Wehrspohn,J.Barthel,J.Kirschner,U.Go ¨sele,S.Fischer,and H.Kronmu ¨ller,IEEE Trans.Magn.38,2571(2002).6S.Pignard,G.Goglio,A.Radulescu,L.Piraux,S.Dubois,A.Declemy,and J.L.Duvail,J.Appl.Phys.87,824(2000).7R.Hertel and J.Kirschner,Physica B 343,206(2004).8R.Ferre ´,K.Ounadjela,J.M.George,L.Piraux,and S.Dubois,Phys.Rev.B 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自旋能斯特效应
自旋能斯特效应是指在核自旋磁偶极子与外磁场相互作用时,核自旋能级发生分裂的现象。
这个效应是由于核自旋与外磁场相互作用导致核磁矩在外磁场中定向,从而改变了核自旋态的能量。
根据量子力学的观点,核自旋在外磁场中的能量可以通过哈密顿算符来描述。
在外磁场的作用下,哈密顿算符可以写成:
H = -μ·B
其中,μ表示核磁矩,B表示外磁场。
这个哈密顿算符的本征值表示核自旋的能级。
根据量子力学的理论,在外磁场中,核自旋分为两个能级,具体数目取决于核自旋的量子数。
一般情况下,每个核自旋量子数对应一个能级,存在2I+1个能级,其中I表示核自旋量子数。
自旋能斯特效应的重要性在于它在核磁共振中的应用。
通过测量核磁共振信号,可以获取有关样品中核自旋的信息,进而了解样品的性质。
这种方法在医学影像、化学分析等领域有重要的应用。
第23卷 第1期物 理 学 进 展Vol.23,No.1 2003年3月PRO GRESS IN PHYSICS Mar.,2003文章编号:1000Ο0542(2003)01Ο0062Ο20铁磁/反铁磁双层膜中交换偏置周仕明1,李合印2,袁淑娟1,王磊1(11复旦大学应用表面国家实验室和复旦大学物理系,上海 20043321复旦大学信息学院,上海 200433)摘 要: 铁磁/反铁磁交换偏置在巨磁电阻器件中具有重要的应用,引起了物理学及材料学等领域内广大科学家的浓厚兴趣。
本文首先阐述了交换偏置的基本性质;然后简述了交换偏置的实验研究方法;最后,着重介绍了几种主要的理论模型。
关键词: 交换偏置;铁磁;反铁磁中图分类号: O48215;O482.52+3;O482.52+5 文献标识码: A0 引 言铁磁(FM)/反铁磁(AFM)体系(如双层膜)在外磁场中从高于反铁磁奈尔温度冷却到低温后,铁磁层的磁滞回线将沿磁场方向偏离原点,其偏离量被称为交换偏置场,通常记作H E,同时伴随着矫顽力的增加,这一现象被称之为交换偏置,有时称体系存在单向各向异性。
Meikleijohn和Bean于1956年在CoO外壳覆盖的Co颗粒中首先发现了这一现象[1~2]。
图1给出了CoO/Co体系中交换偏置的基本特征。
CoO/Co颗粒的顺时针和逆时针转矩曲线之间有明显的磁滞效应,两个方向的转矩曲线并不相重合,如图1a的所示,而对于均匀的铁磁材料,高场下转动磁滞趋于零。
如图1b所示,当外场沿着冷却场的方向测量时,磁滞回线将向负磁场方向偏离,样品的磁滞回线出现不对称性。
交换偏置广泛存在于FeMn/FeNi和Cr2O3/FeNi等很多体系中[3]。
为了能够更好地了解交换偏置的基本特征,人们一般采用铁磁/反铁磁双层膜结构。
铁磁/反铁磁交换偏置展现出很多新的物理现象,其基本特性与铁磁层和反铁磁层材料、厚度以及结构取向、温度、生长顺序及工艺条件等密切相关,其机制涉及到界面相互作用,包含很多丰富的物理内涵,是凝聚态物理中的重要研究课题。
a r X i v :0908.3568v 4 [c o n d -m a t .d i s -n n ] 11 S e p 2009Typeset with jpsj2.cls <ver.1.2.2b >LetterObservation of Magnetic Monopoles in Spin IceHiroaki Kadowaki 1,Naohiro Doi 1,Yuji Aoki 1,Yoshikazu Tabata 2,Taku J.Sato 3,Jeffrey W.Lynn 4,Kazuyuki Matsuhira 5,and Zenji Hiroi 61Department of Physics,Tokyo Metropolitan University,Hachioji-shi,Tokyo 192-03972Department of Materials Science and Engineering,Kyoto University,Kyoto 606-85013NSL,Institute for Solid State Physics,University of Tokyo,Tokai,Ibaraki 319-11064NCNR,National Institute of Standards and Technology,Gaithersburg,Maryland 20899-6102,USA 5Department of Electronics,Faculty of Engineering,Kyushu Institute of Technology,Kitakyushu 804-85506Institute for Solid State Physics,University of Tokyo,Kashiwa 277-8581(Received August 11,2009;accepted September 8,2009;published October 13,2009)Excitations from a strongly frustrated system,the kagom´e ice state of the spin ice Dy 2Ti 2O 7under magnetic fields along a [111]direction,have been studied.They are theoretically proposed to be regarded as magnetic monopoles.Neutron scattering measurements of spin correlations show that close to the critical point the monopoles are fluctuating between high-and low-density states,supporting that the magnetic Coulomb force acts between them.Specific heat measurements show that monopole-pair creation obeys an Arrhenius law,indicating that the density of monopoles can be controlled by temperature and magnetic field.KEYWORDS:magnetic monopole,spin ice,kagom´e ice,neutron scattering,specific heatSince the quantum mechanical hypothesis of the ex-istence of magnetic monopoles proposed by Dirac,1,2)many experimental searches have been performed,rang-ing from a monopole search in rocks of the moon to experiments using high energy accelerators.3)But none of them was successful,and the monopole is an open question in high energy physics.Recently,theo-retical attention has turned to condensed matter sys-tems where tractable analogs of magnetic monopoles might be found,4–6)and one prediction 5)is for an emer-gent elementary excitation in the spin ice 7,8)compound Dy 2Ti 2O 7.In solid water,the protons are disordered even at ab-solute zero temperature and thus retain finite entropy,9)and spin ice exhibits the same type of disordered ground states.8,10)The Dy spins occupy a cubic pyrochlore lat-tice,which is a corner sharing network of tetrahedra (Fig.1(a)).Each spin is parallel to a local [111]easy axis,and interacts with neighboring spins via an effec-tive ferromagnetic coupling.This brings about a geomet-rical frustration where the lowest energy spin configura-tions on each tetrahedron follow the ice rule,“2-in,2-out”structure,and the ground states of the entire tetrahedral network are macroscopically degenerate in the same way as the disordered protons in water ice.9,10)In addition to this remarkable observation,there is the more intrigu-ing possibility 5)that the excitations from these highly degenerate ground states are topological in nature and mathematically equivalent to magnetic monopoles.The macroscopic degeneracy of the spin ice state can be partly lifted by applying a small magnetic field along a [111]direction.11)Along this direction the pyrochlore lattice consists of a stacking of triangular and kagom´e lattices (Fig.1(a)).In this field-induced ground state,the spins on the triangular lattices are parallel to the field and consequently drop out of the problem,while those on the kagom´e lattices retain disorder under the same ice rules,only with a smaller zero-point entropy.12)This is referred to as the kagom´e ice state 11,13–15)(Fig.1(b)).In Fig.1(c)we illustrate creation of a magnetic monopole and antimonopole pair in the kagom´e ice state.An excitation is generated by flipping a spin on the kagom´e lattice,which results in ice-rule-breaking “3-in,1-out”(magnetic monopole)and “1-in,3-out”(anti-monopole)tetrahedral neighbors.From the viewpoint of the dumbbell model,5)where a magnetic moment is replaced by a pair of magnetic charges,the ice-rule-breaking tetrahedra simulate magnetic monopoles,with net positive and negative charges sitting on the centers of tetrahedra.The monopoles should interact via the mag-netic Coulomb force,5)which is brought about by the dipolar interaction 16)between spins in Dy 2Ti 2O 7.They can move and separate by consecutively flipping spins,but are confined to the two-dimensional kagom´e layer (e.g.Fig.1(d)).This possibility of separating the local excitation into its constituent parts is a novel fraction-alization in a frustrated system in two or three dimen-sions,5,17)and enables many new aspects of these emer-gent excitations to be studied experimentally,such as pair creation and interaction,individual motion,currents of monopoles,correlations and cooperative phenomena.In the present study,inspired by the theoretical predic-tion of the monopoles,we have investigated two aspects of magnetic monopoles in spin ice using direct neutrona[111]H=0b cd eH//[111]H//[111]H//[111]H//[111]Fig.1.(Color)Magnetic moments of Dy2Ti2O7reside on the py-rochlore lattice.8)At low temperatures,four magnetic momentson each tetrahedron obey the ice rule(2-in,2-out).The resultingspin ice state is shown in(a).The pyrochlore lattice consists ofstacked triangular and kagom´e lattices,shown by green and bluelines,respectively,along a[111]direction.(b)Under small[111]magneticfields,spins on the kagom´e lattice remain in the dis-ordered kagom´e ice state.11)(c)An excited state is induced byflipping a spin from(b),enclosed by a dashed circle,where neigh-boring tetrahedra have3-in,1-out and1-in,3-out configurations.These ice-rule-breaking tetrahedra are represented by magneticmonopoles with opposite charges depicted by spheres.(d)Byconsecutivelyflipping two spins from(c),the monopoles are frac-tionalized.(e)As the magneticfield is increased,H≫H c,spinsrealize a fully ordered,staggered arrangement of monopoles.scattering techniques and thermodynamic specific heatmeasurements.Single crystals of Dy2Ti2O7were prepared by thefloating-zone method.11)Specific heat was measured by aquasi-adiabatic method.Neutron scattering experimentson a single crystal under a[111]field were performed onthe triple-axis spectrometers BT-9at the NIST Centerfor Neutron Research and the ISSP-GPTAS at the JapanAtomic Energy Agency.The sample was mounted in di-lution refrigerators so as to measure the scattering planeperpendicular to the[111]direction.A straightforward signature of monopole-pair cre-ation is an Arrhenius law in the temperature(T)depen-dence of the specific heat(C),C(T)∝exp(−∆E/k B T),where∆E is afield(H)dependent creation energy.Onecan simply expect∆E=E0−µH owing to the Zeemaneffect.Figure2shows the measured C(T)of Dy2Ti2O7under a[111]appliedfield as a function of1/T.TheArrhenius law is clearly seen at low temperatures,indi-C(J/Kmol-Dy)1/T (K-1)Fig.2.(Color)Specific heat under[111]fields is plotted as a func-tion of1/T.In the intermediate temperature range these dataare well represented by the Arrhenius law denoted by solid lines.The inset shows thefield dependence of the activation energy.cating that monopole–antimonopole pairs are thermallyactivated from the ground state.We remark that all themeasurements were performed underfield cooling condi-tions,which are important to avoid complications due tospin freezing8,10,18)among the ground state manifolds,whose degeneracy are slightly lifted.We think that thedeviation from the Arrhenius law at the lowest temper-atures is attributable to these perturbative effects.Theobserved activation energy∆E depends linearly on H(Fig.2inset)between0.2and0.9T,i.e.,in the kagom´eice state.The deviation from linearity below0.2T(spinice regime)suggests that the nearest-neighbor effectivebond energy J effslightly changes between the two states.The zero-field value∆E(H=0)=3.5K reasonablyagrees with an estimation∆E(H=0)=4J eff=4.5K using J effin ref.16.The observed Arrhenius law ofC(T),which is attributable to variation of density of themonopole pairs,implies that the number of monopolescan be tuned by changing T and H.A microscopic experimental method of observingmonopoles is magnetic neutron scattering.One challengeto the experiments is to distinguish the relatively weakscattering from the small number of monopoles from thevery strong magnetic scattering8,14)of the ground states.A theoretical idea5)which is helpful for identifying themonopole scattering is that the[111]field acts as chem-ical potential of the monopoles,enabling us to controltheir density as shown by the present specific heat mea-surements.As thefield is increased,the kagom´e ice statewith low monopole density changes continuously to themaximum density state,the staggered monopole state(Fig.1(e)),where all spin configurations become“3-in,1-out”or“1-in,3-out”to minimize the Zeeman energy.For the present neutron scattering experiments,theI n t e n s i t y (a r b . u n i t s )Density of monopole (per tetrahedron)H (T)Fig.3.(Color)The magnetic Bragg intensity at T =T c +0.05K is plotted as a function of the [111]field.The open squares and dashed curves represent the measurements at (2¯20)and corre-sponding MC simulations,respectively.The dot-dashed curve is the density of positively charged monopoles obtained by the sim-ulation.The inset shows the HT phase diagram under the [111]field.The solid line represents the first-order phase transition with the critical point shown by an open circle.13)The dashed lines are crossovers.15)The intensity maps shown in Fig.4were measured at the two points depicted by open squares.best temperature and field region to observe monopoles in Dy 2Ti 2O 7is close to the liquid-gas type critical point 13)(T c ,H c )(Fig.3inset).In the monopole pic-ture,5)where they are interacting via the magnetic Coulomb force,the first-order phase transition 13)is as-cribed to phase separation between high-and low-density states.We naturally anticipate that neutron scattering close to the critical point is a superposition of the scatter-ing pattern by the (low-density)kagom´e ice state 14)and that by high-density monopoles,which is diffuse scatter-ing around magnetic Bragg reflections,i.e.,ferromagnetic fluctuations.The neutron measurements were performed under a [111]field,and Monte Carlo (MC)simulations 14)were also carried out for the dipolar spin ice model 16,18)to quantify our observations.Figure 3shows the field de-pendence of the magnetic intensity of the (2¯20)Bragg reflection at T =T c +0.05=0.43K.The intensity plateau for H <0.8T corresponds to the kagom´e ice state with low density monopoles.The deviation from the plateau as H exceeds 0.8T indicates that monopoles are being created gradually,while the saturation of the intensity for H ≫H c denotes the staggered monopole state (Fig.1(e)).In Fig.3we also show the Bragg inten-sity and the density of the positively charged monopoles obtained by the simulation.The observation shows good agreement with the simulation for H <H c .On the other hand,above H c there are substantially less monopoles than expected from the simulation,which will be dis-cussed below.We selected T =T c +0.05K and H =H c (Fig.3inset)for observation of the fluctuating high-and low-density monopoles.At this H ,T point,we measured in-tensity maps in the scattering plane.An intensity map of the kagom´e ice state at T =T c +0.05K and H =0.5T was also measured for comparison.Figure 4compares the measured and simulated intensity maps.The observed scattering pattern of the kagom´e ice state (Fig.4(a))is in excellent agreement with the simulation (Fig.4(c)),showing the peaked structure 14)at (2/3,−2/3,0)and the pinch point 19)at (4/3,−2/3,−2/3).These structures re-flect the kagom´e ice state.The observed (Fig.4(b))and simulated (Fig.4(d))intensity maps close to the critical point show a weakened kagom´e -ice scattering pattern (by the low-density state)and diffuse scattering around (2¯20)(by the high-density state).The observation agrees fairly well with the simu-lation.However the diffuse scattering is less pronounced for the observation.We found that this discrepancy orig-inated from an instrumental condition of the GPTAS spectrometer,which has a large vertical resolution of ∆q =0.25˚A −1(full width at half maximum,FWHM).We carried out the same measurement on the BT-9spec-trometer.It has a smaller vertical resolution of ∆q =0.1˚A −1(FWHM),which does not affect the diffuse scat-tering.The resulting data are shown in Fig.4(f),which are in better agreement with the simulation (Fig.4(d))around (2¯20).An interesting point suggested by this resolution effect is that correlations of the high-density monopoles are three dimensional in space,although the monopoles can only move in the two dimensional layers (Fig.1(d)).The three dimensional correlations are con-sistent with the isotropic Coulomb interaction between monopoles.We note that the kagom´e -ice scattering pat-tern is two dimensional in nature,14)and thus is not af-fected by the vertical resolution.To illustrate the high-and low-density monopoles yielding the scattering patterns in Figs.4(b),4(d),and 4(f),two typical snapshots of the monopoles of the MC simulation are shown in Fig.4(e),where we depict mag-netic charges at centers of the tetrahedra.Lines connect-ing the centers of tetrahedra form a diamond lattice,and magnetic charges reside on its lattice points.Re-gions of the low-density monopoles (where black points dominate)produce the kagom´e -ice scattering pattern,while those of the high-density monopoles (where red and blue points dominate)produce the diffuse scatter-ing around the Bragg reflections.These critical fluctu-ations between high-and low-density phases reinforce the proposed explanation 5)of the puzzling liquid-gas type critical point 13)using the similarity argument to phase transitions of ionic particle systems on lattices.20)Consequently they strongly suggest existence of mag-netic monopoles interacting via the magnetic Coulomb force.Further investigations of critical phenomena,15)screening of the Coulomb interaction,and effects of the00.20.40.60.81013(h, -h, 0)(k , k , -2k )a cb df2(220)(220)(202)(202)(220)Fig.4.(Color)Intensity maps measured at T =T c +0.05K in the scattering plane are shown for two field values (Fig.3inset):the kagom´e ice state at 0.5T (a,c)and the fluctuating high-and low-density monopoles at H c (b,d,f).(a,b)and (f)were measured on the GPTAS and BT-9spectrometers,respectively.(c,d)are simulated intensities.(e)Two snapshots of the monopoles of the simulation corresponding to (b,d,f)are shown on the diamond lattice,in which blue,red,and black points represents +,−and 0magnetic charges,respectively.The light green circles in (b,d,f)show the high intensity regions caused by the high-density monopoles,i.e.,ferromagnetic fluctuations.anisotropic motion of the monopoles within the kagom´e lattices are of interest.A question,which is not pursued in the present study,is how monopoles unbound by the fractionaliza-tion move in the kagom´e paring the ob-served Arrhenius law with that of a study 21)of the dif-fusive motion of monopoles in spin ice state,it seems that the interesting temperature ranges where uncon-fined monopoles move diffusively are roughly T >1.5K (H =0.5T)and T >0.7K (H =0.9T).There may be another interesting issue in the discrepancy between ob-served Bragg intensity and the classical MC simulation shown in Fig.3(H >H c ).We speculate that it may indicate the existence of quantum mechanical effects ne-glected in the computation.Puzzling experimental facts at low T were also noticed by the slow saturation of mag-netization 13)and the non-zero specific heat 15)above H c down to very low temperatures,T <0.1K.For exam-ple,if the double spin flips shown in Fig.1(d)can occur by tunneling,22)monopoles (or holes in the staggered monopole state)might move more easily than classical 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㊀第40卷㊀第11期2021年11月中国材料进展MATERIALS CHINAVol.40㊀No.11Nov.2021收稿日期:2021-07-14㊀㊀修回日期:2021-09-28基金项目:国家自然科学基金资助项目(11804343)第一作者:汤㊀进,男,1989年生,副研究员通讯作者:杜海峰,男,1979年生,研究员,博士生导师,Email:duhf@DOI :10.7502/j.issn.1674-3962.202107019透射电镜差分相位分析技术磁畴研究汤㊀进1,吴耀东1,2,熊奕敏1,田明亮1,杜海峰1(1.中国科学院合肥物质科学研究院强磁场科学中心极端条件凝聚态物理安徽省重点实验室,安徽合肥230031)(2.合肥师范学院物理与材料工程学院,安徽合肥230061)摘㊀要:透射电子显微镜具有高空间磁分辨率和易集成的多场调控等特点,成为当下纳米尺度下先进磁结构观测的主要手段之一㊂首先介绍和比较了透射电镜磁表征的3种模式:洛伦茨模式㊁电子全息模式和差分相位分析模式,然后详细综述了差分相位分析技术表征一类中心对称晶体Fe 3Sn 2材料中新型磁畴结构的研究进展㊂在该研究中,首先结合差分相位分析技术和三维微磁学模拟,阐释了中心对称材料中复杂 多拓扑态 磁畴起源于磁结构的三维特性,随后基于该材料温度诱导自旋重取向内禀物性,在Fe 3Sn 2受限纳米盘中,利用差分相位分析技术发现了一类全新的涡旋状磁结构 靶磁泡 ,研究了其磁场演化行为,最后提出了斯格明子-磁泡基存储器的概念,并实现了磁场和电流高度可控斯格明子-磁泡拓扑磁转变㊂差分相位分析技术揭示的中心对称磁性材料纳米结构中的新颖磁畴及丰富的电流驱动动力学,有望促进未来基于新型磁畴结构的拓扑相关自旋电子学器件的开发㊂关键词:透射电子显微镜;差分相位分析;磁畴;斯格明子-磁泡;中心对称磁体中图分类号:TH742㊀㊀文献标识码:A㊀㊀文章编号:1674-3962(2021)11-0851-10Magnetic Domain Imaging by Differential PhaseContrast Technique of Transmission Electronic MicroscopyTANG Jin 1,WU Yaodong 1,2,XIONG Yimin 1,TIAN Mingliang 1,DU Haifeng 1(1.Anhui Province Key Laboratory of Condensed Matter Physics at Extreme Conditions,High Magnetic Field Laboratory,Hefei Institutes of Physical Science,Chinese Academy of Sciences,Hefei 230031,China)(2.School of Physics and Materials Engineering,Hefei Normal University,Hefei 230061,China)Abstract :Transmission electronic microscopy (TEM)has become one of the most advanced techniques to observe nano-metric-sized magnetic domains,owing to its high spatial magnetic resolution and easy accessibility in integrating multiple physic fields.Here,we compared three techniques of TEM observing magnetic domains:Lorentz-TEM,electronic hologra-phy and differential phase contrast scanning TEM (DPC-STEM).Then we reviewed recent advances in magnetic domains imaging of a centrosymmetric magnet Fe 3Sn 2by DPC-STEM.We demonstrated physical clarifications to multiple topological states ,which are attributed to three-dimensional (3D)depth-modulated spin configurations,using DPC-STEM and 3D mi-cromagnetic simulations.We then reported a new class of vortex-like spin configurations named target bubble and their field-driven magnetic evolutions in Fe 3Sn 2nanodisks.Finally,we proposed a new strategy to design memory named Skyrmi-on-bubble-based memory,which utilizes Skyrmions and bubbles as binary bits 1 and 0 ,respectively.Current-field-controlled topological Skyrmion-bubble transformations have been also achieved.The novel magnetic domains and their in-triguing electronic-magnetic properties shed by DPC-STEM are expected to facilitate advances in developing topology-related spintronic devices.Key words :transmission electronic microscopy;differential phase contrast;magnetic domain;Skyrmion-bubble;cen-trosymmetric uniaxial magnet1㊀前㊀言磁性材料已经被广泛应用于现代生活中,具有很大的市场价值,其中一个典型代表是自旋电子学磁功能器件[1]㊂自旋电子学是将电子的两个内禀属性电荷和自旋博看网 . All Rights Reserved.中国材料进展第40卷相结合的研究学科㊂以机械硬盘为代表的自旋电子学器件已经取得了较大的商业成功[2]㊂机械硬盘是利用磁化反平行排列的磁畴来表征双数据比特,通过读头的机械转动来实现读写㊂但是传统机械硬盘受到机械振动和热扰动的影响,其性能已趋于功能极限㊂为了突破功能极限,科学家们期望通过发现新型磁结构来构建新一代自旋电子学器件㊂磁斯格明子是新型磁结构的代表[3-5]㊂磁斯格明子是一类涡旋状新型磁结构,具有拓扑非平庸类粒子行为㊁可调的小尺寸和丰富的电磁相关动力学行为等特点[6]㊂磁斯格明子的关键稳定机制是材料体系中的Dzyaloshinskii-Moriya(DM)相互作用[7]㊂根据DM 相互作用类型,磁斯格明子主要分为3种:①具有体DM 相互作用的材料,如B 20型FeGe 和MnSi 材料中的布洛赫(Bloch)型磁斯格明子[3,4,8,9](图1a);②具有表面DM相互作用的材料,如铁磁/重金属异质结薄膜和C 3v 对称晶体GaV 4S 8中的奈尔(Néel)型磁斯格明子[10,11];③具有二维各向异性DM 相互作用的材料,如D 2d 晶体MnPdPtSn 中的反磁斯格明子[12]㊂此外,在传统中心对称单轴铁磁体中,偶极相互作用与单轴磁晶各向异性等的竞争也会产生出一类局域柱状畴磁结构 磁泡,其中类型I 磁泡的闭合畴壁贡献了与Bloch 型手性斯格明子相同的整数拓扑荷,因此其也被称为磁泡斯格明子(图1b)[13-22]㊂近年来,这些具有丰富磁学㊁电学性质的磁斯格明子可以作为信息载体,用来构建存储器㊁逻辑器件㊁神经网络器件和互联信息器件等[23-25],形成了一类新兴的自旋电子学亚类学科 拓扑自旋电子学[26-28]㊂图1㊀非中心对称螺磁体中布洛赫型磁斯格明子(a)[3,4,8,9];中心对称单轴铁磁体中的磁泡斯格明子(b)[13-22]Fig.1㊀Bloch-type Skyrmion in an noncentrosymmetric screw magnet (a)[3,4,8,9];Skyrmion bubble in a centrosymmetric uniaxialferromagnet (b)[13-22]拓扑自旋电子学研究领域关键的科学问题之一是磁斯格明子的电调控[23]㊂而未来自旋电子学器件高存储密度要求磁信息载体的尺寸为纳米尺度,因此需要探索纳米尺度下的磁斯格明子的相关性能,这要求磁表征技术的高空间分辨率㊂现代磁学的发展也得益于先进磁表征技术的发展㊂依据自旋与电流㊁电子㊁光等的相互作用,科学家们已经开发出了多种先进的磁表征技术[26],如表1所示[11,23,29-31]㊂其中,透射电镜不仅能够观测纳米尺度范围内的磁畴,也易于集成多物理场条件,对样品和外界环境要求相对较低[32]㊂因此,透射电镜成为了近年来高分辨率磁表征的重要技术手段,极大地推动了磁斯格明子相关的研究进展,例如磁斯格明子的首次实空间观测[4]㊁磁浮子的首次实空间观测[33]㊁反斯格明子的首次实空间观测等,都是利用透射电镜技术实现的[12]㊂本文将首先介绍基于透射电镜的3种基本磁表征手段,并随后着重综述透射电镜差分相位分析技术表征一类中心对称晶体中的新型磁畴结构的研究进展㊂表1㊀磁表征技术:洛伦茨透射电子显微镜㊁磁力显微镜㊁自旋极化扫描隧道显微镜㊁X 射线显微学㊁表面磁光克尔效应㊁X-射线磁圆二色仪-光发射电子显微镜[11,23,29-31]Table 1㊀Magnetic imaging techniques :Lorentz-transmission elec-tronic microscopy (Lorentz-TEM ),magnetic force mi-croscopy (MFM ),spin-polarized scanning tunneling mi-croscopy (spin-polarized STM ),X-ray holography (X-ray holography ),surfacemagneto-opticalKerreffect(SMOKE ),X-ray magnetic circular dichroism-photoe-mission electron microscopy (XMCD-PEEM )[11,23,29-31]Techniques ResolutionSpatial /nm Time Field /T Temperature/K Lorentz-TEM ~2ms -2~25~1300MFM~10s -16~162~400Spin-polarized STM~0.5s-9~9<10X-ray holography~20nsSMOKE~300ns -9~92~800XMCD-PEEM~25s02~3002㊀透射电镜磁表征技术透射电镜磁表征技术是基于电子在磁场运动过程中受到的洛伦茨力,因此磁表征的透射电镜也被称作洛伦茨透射电镜[4,32]㊂透射电镜电子束的传输方向为垂直于样品表面,由于电子的轨迹只受到与其运动方向垂直的磁场的影响,因此洛伦茨透射电镜只能表征面内磁矩㊂此外,透射模式也表明透射电镜探测到的是样品厚度方向积分的磁矩㊂依据电子受到洛伦茨力发生偏转的探测方式,透射电镜磁表征技术可以分成3种(图2):欠焦/过焦情况下的菲涅尔磁衬度,即传统洛伦茨技术[4];通过分辨样品和全息丝的干涉条纹宽度的变化来获得磁相位,即电子全息技术[34-37];扫描聚焦电子束通过样品后,4个分立探头探测的电子束强度的差异等价于磁相位衬度差分,即差分相位分析扫描透射电镜技术[13,15,16,38-40]㊂258博看网 . All Rights Reserved.㊀第11期汤㊀进等:透射电镜差分相位分析技术磁畴研究图2㊀透射电镜3种磁表征技术示意图:洛伦茨[4]㊁电子全息[34-37]和差分相位分析[13,15,16,38-40]Fig.2㊀Schematic designs of three magnetic imaging techniques of trans-mission electronic microscopy:Lorentz [4],electronic hologra-phy [34-37]and differential phase contrast scanning [13,15,16,38-40]根据不同透射电镜磁成像技术的特点,3种方式各具特色,但也存在着缺点㊂传统离焦下表征的洛伦茨模式是最早也是现在最流行的透射电镜磁成像表征方式[20],具有易于操作㊁比较直观反射磁结构和成像速度快等优点,但是这种方法也有以下缺点:①由于离焦状态下样品边缘具有菲涅尔强衍射,使得该方法不适用于太小受限结构的磁分辨[41];②作为一种间接获得磁相位的方法,传统输运强度分析(transport of intensity equation,TIE)技术解析磁结构的过程中可能会引入一些人为的磁信息,造成严重的偏差[42]㊂电子全息技术是一种正焦模式下直接表征磁相位的方法,能够非常准确和定量地解析磁结构[34-37],但是这种方法也有以下缺点:①电子全息模式观测到的是干涉条纹[34],不能直观反映磁结构,不适用于一些快速磁结构动力学响应的表征;②由于干涉所需的参考光束需要经过真空,因此电子全息只能表征靠近样品边缘的磁结构,有效观测尺寸大约为1μm [37]㊂差分相位分析扫描透射模式也是一种正焦状态下直接探测磁矩的方式(图3),具有磁成像精度高㊁范围广等优点,特别是能够精确表征样品缺陷处的磁结构信息[13,15,16,38-40],但是该方法也有以下缺点:①扫描聚焦模式成像较慢(数十秒以上),不适用于实时磁结构动力学表征;②扫描聚焦模式下会对样品造成损伤㊂从以上讨论可以得出,相比于传统洛伦茨模式,电子全息和差分相位分析都是更为精确的磁相位表征技术,但是电子全息只适用于一些小样品的表征,而差分相位分析技术并不受到样品尺寸的限制,可以表征任意尺寸磁样品的磁结构㊂本文将着重介绍差分相位分析方法在偶极磁斯格明子材料的新型磁结构表征中的近期科研进展㊂3㊀差分相位分析磁畴表征3.1㊀三维磁斯格明子与磁泡由于单轴磁晶各向异性㊁偶极-偶极相互作用㊁交换图3㊀差分相位分析方法分析磁畴的过程[13,15,16,38-40]:(a ~d)扫描透射模式下,4个分立的差分衬度探头A㊁B㊁C 和D 得到聚焦电子束穿过一个直径为1550nm 的Fe 3Sn 2纳米盘的衬度图像;(e)探头A 和C 的差分衬度,与样品中沿着y 轴的磁场强度成正比;(f)探头B 与D 的差分衬度,与样品中沿着x 轴的磁场强度成正比;(g)通过(A -C)2+(B -D)2计算出的整个面内磁场强度分布图;(h)最终重构的面内场强分布图Fig.3㊀Analysis procedure for determining the magnetic structure in a1550nm Fe 3Sn 2disc by using differential phase contrast scan-ning TEM [13,15,16,38-40]:(a ~d)differential phase contrastcomponent images from the four segments of the detectors A,B,C and D,respectively;(e)differential phase contrast compo-nent obtained by subtracting C from A (A -C),which is propor-tional to the field component along the y axis;(f)differential phase contrast component obtained by subtractingD from B (B -D),which is proportional to the field component along the x axis;(g )totalin-planefieldstrengthobtainedfrom(A -C)2+(B -D)2;(h)in-plane magnetization mapping相互作用和外磁场赛曼能的竞争,中心对称单轴磁性材料能够形成局域的柱状磁畴结构,该结构被称为磁泡(图1b)[20,43,44]㊂虽然磁泡在20世纪70~90年代得到了大量的研究,并构建了磁泡存储器等功能性器件[45],但由于该器件的大尺寸(微米尺度)不适用于紧凑的器件设计而逐渐被淘汰[43]㊂最近,新型涡旋局域磁结构斯格明子的发现也重新引起了研究人员对传统磁泡的广泛兴趣[21,22,31,42,46-54]㊂依据柱状磁畴的畴壁磁化分布,磁泡可分为类型I 拓扑非平庸磁泡和类型II 拓扑平庸磁泡[21]㊂其中具有闭合畴壁的类型I 磁泡具有与磁斯格明子相同的拓扑性,也被称为斯格明子磁泡[31,51-54]㊂特别地,最近的研究发现了直径小于50nm 的斯格明子磁泡和自旋转移力矩驱动磁泡动力学行为[17,31,54]㊂这些研究成果也预示着传统磁泡可以被用来构建新型高性能自旋电子学器件[18]㊂为简便表述,后文将中心对称晶体中的类型I 斯格明子磁泡和类型II 磁泡分别称为磁斯格明子和磁泡㊂358博看网 . All Rights Reserved.中国材料进展第40卷虽然中心对称晶体中的磁斯格明子和磁泡结构已经得到了很好的理论解析[55],但在近期采用透射电镜研究磁泡材料磁畴工作中发现了复杂的 多拓扑态 磁结构[22,47]㊂这些复杂磁结构与传统磁斯格明子和磁泡结构有很大差异,同时一直没有得到很好的物理解释,限制了磁泡材料的未来应用性㊂分析可知,这些复杂 多拓扑态 磁结构均是通过透射电镜洛伦茨模式得到,且解析的磁结构被认为是二维的㊂传统洛伦茨模式表征磁结构是通过TIE 技术解析过焦㊁正焦和欠焦菲涅尔磁衬度得到的㊂而为了得到更清晰的磁结构,TIE 技术通常需要设定滤波参数来过滤噪音和非磁背景,但滤波也可能会得到偏离真实情况的磁结构[42];同时TIE 技术也不适用于解析传统均匀铁磁磁畴[14,16]㊂透射电镜技术得到的是沿着样品厚度方向的积分磁化分布,但以往的研究认为磁结构在厚度方向为磁化均匀的[22,47]㊂作者团队[16]采用透射电镜差分相位分析-扫描透射模式和三维微磁学计算模拟相结合的方式,系统地研究了Kagome 中心对称晶体材料Fe 3Sn 2中的复杂 多拓扑态 多环和Φ形-圆弧形磁涡旋结构,如图4所示㊂Fe 3Sn 2是一类室温单轴铁磁体[56-61],单轴磁化易轴在室温下沿着c 轴㊂同时,Fe 3Sn 2为低品质因子材料,即单轴磁晶各向异性K u 小于12μ0M 2s ,μ0和M s 分别为真空磁导率和饱和磁化率㊂通过三维微磁学计算模拟发现[62],对于低品质因子的Fe 3Sn 2薄片样品,强的偶极-偶极相互作用会导致磁斯格明子和磁泡沿着厚度方向发生连续自旋扭转,形成界面涡旋状磁结构㊂因此,上述模拟结果表明,Fe 3Sn 2纳米薄片样品的磁斯格明子和磁泡沿着厚度方向不是均匀磁化的(图4e 和4f),因此在透射电镜解析的磁结构中必须考虑厚度方向的积分磁化分布㊂同时,利用差分相位分析进一步得到了Fe 3Sn 2纳米薄片样品的多环状和圆弧形涡旋磁结构(图4a 和4b),发现其与传统洛伦茨模式解析磁结构有很大差异,但与三维微磁模拟的磁斯格明子和磁泡的积分磁化分布高度一致(图4c 和4d)㊂这些研究结果表明, 多拓扑态 起源于传统中心对称材料中的三维磁斯格明子和磁泡结构,磁结构的复杂性是由于非均匀三维磁结构投射到二维平面后的积分相加所导致的㊂3.2㊀靶磁泡的发现及其磁场驱动演化过程Fe 3Sn 2的磁晶各向异性具有强温度依赖性,单轴磁各向异性常数K u 随着温度降低而减小,因此易磁化方向会由高温时的c 轴转变到低温时的ab 易磁化面,即温度诱导自旋重取向[61]㊂本课题组[13]制备了不同尺寸受限Fe 3Sn 2纳米盘,利用差分相位分析研究了其零磁场下的图4㊀Fe 3Sn 2纳米结构中类型I 斯格明子磁泡和类型II 拓扑平庸磁泡的三维磁结构[16]:(a,b)差分相位分析方法得到的面内自旋分布;(c,d)三维微磁模拟得到的平均面内磁化分布;(e,f)三维微磁模拟得到的厚度调制磁结构Fig.4㊀3D spin texture of type-I Skyrmion bubble and type-II topologi-cally trivial bubble in the Fe 3Sn 2nanostructure [16]:(a,b)in-plane magnetization mappings of two types of bubbles obtainedfrom differential phase contrast technique;(c,d)average in-plane magnetization mappings of two types by 3D micromagnetic simulation;(e,f)depth-modulated 3D magnetic bubbles by 3Dmicromagnetic simulation磁畴演化行为,如图5所示㊂由于在传统洛伦茨模式离焦磁表征模式下,受限小尺寸样品边缘强的菲涅尔衍射条纹给磁结构解析带来极大的干扰,因此正焦模式下工作的差分相位分析技术更适用于精确研究受限体系下的磁畴结构㊂不同于在高温300K 的条纹畴磁基态(图5a),在低温100K 的易面磁化Fe 3Sn 2(001)纳米盘中,偶极-偶极相互作用会诱导面内磁矩沿着圆盘边缘排列,形成经典的软磁磁涡旋结构(图5b)㊂以软磁磁涡旋为种子磁结构,当升高温度到室温,易面磁纳米盘转变为垂直磁纳米盘,Fe 3Sn 2(001)纳米盘中会形成多环靶态磁结构,命名其为 靶磁泡 (图5c)㊂通过分析靶磁泡的中间层磁化分布,发现其自旋从中心到最外边缘旋转了π的整数(k )倍(图5d),因此中心对称晶体中的靶磁泡也可以被看作k π-磁斯格明子㊂这种自旋重取向导致的软磁磁涡旋到靶磁泡的转变可被微磁模拟重复出来(图5e ~5h)㊂458博看网 . All Rights Reserved.㊀第11期汤㊀进等:透射电镜差分相位分析技术磁畴研究图5㊀在Fe 3Sn 2纳米盘中通过在零磁场下加热到室温的方式,利用差分相位分析技术观测到的室温下的条纹畴到低温下的软磁磁涡旋到室温下的靶磁泡(k π-磁斯格明子)的转变[13]:(a)300K 室温条纹畴;(b)100K 磁涡旋;(c)300K 室温靶磁泡;(d)沿着图5c 中A 到B 位置连线相关面内磁化强度;(e)模拟的室温条纹畴;(f)模拟的100K 磁涡旋;(g)模拟的室温靶磁泡;(h)模拟的沿着图5g 中C 到D 位置连线相关面内磁化强度Fig.5㊀Transformation from a soft magnetic vortex at 100K to a target bubble (k π-Skyrmion)at 300K through zero-field warming in an Fe 3Sn 2nanodisk obtained by differential phase contrast [13]:(a)experimental stripes at 300K;(b)soft vortex at 100K;(c)target bubble at300K;(d)position dependent in-plane magnetization amplitude along the line A to B in Fig.5c;(e~g)simulated stripes with uniaxi-al magnetic anisotropy K u =53.0kJ /m 3,soft vortex with K u =2.3kJ /m 3and target bubbles with K u =53.0kJ /m 3;(h)simulated posi-tion dependent in-plane magnetization amplitude along the line C to D in Fig.5g㊀㊀k π-磁斯格明子的拓扑荷为0(k 为奇数)或1(k 为偶数)㊂前期研究表明,k π-磁斯格明子具有k 相关可调自旋波激发和多场调控磁性等特点,其中2π-磁斯格明子(也叫做类斯格明子Skyrmionium)被提出可以用来构建无垂直漂移赛道存储器和斯格明子互联器件等[63,64]㊂但k π-磁斯格明子的研究多为理论模拟研究,仅仅在极少数的磁系统中被观察到[65,66],k π-磁斯格明子(k >2)的实验发现尤其充满挑战㊂通过以软磁磁涡旋为种子磁结构以及调节Fe 3Sn 2(001)纳米盘的直径,得到了丰富的零磁场稳定的k π-磁斯格明子(k =2,3,4和5)㊂与手性磁体中零磁场下两种简并的k π-磁斯格明子相比较,理论上中心对称材料中的零磁场k π-磁斯格明子有2k +1种㊂此外,之前的理论研究也预言了磁场诱导的k π-磁斯格明子的新颖磁性[67-70],但相关的实验研究还很少㊂因此,本课题组[15]进一步利用差分相位分析研究了Fe 3Sn 2(001)纳米盘中的磁场演化行为,如图6所示㊂磁场驱动下,Fe 3Sn 2(001)纳米盘k π-磁斯格明子主要呈现出3个特点:①零磁场下的不规则形状转变为高磁场下的轴对称形状(图6a);②磁场诱导k 系数的减小;③k π-磁斯格明子直径随磁场增强而连续减小(图6b)㊂中心对称Fe 3Sn 2纳米盘中的k π-磁斯格明子具有室温和零磁场稳定性㊁丰富多重简并态以及利用外磁场和图6㊀Fe 3Sn 2纳米结构中采用差分相位分析技术观测到的磁场诱导的k π-磁斯格明子(靶磁泡)的磁演化行为[15]:(a)实验观测的高磁场下稳定的圆形k π-磁斯格明子;(b)k π-磁斯格明子的直径随着磁场强度的变化关系,图中正方形点㊁三角形点和圆形点分别代表4π㊁3π和2π磁斯格明子Fig.6㊀Field-driven magnetic evolutions of k π-Skyrmion in Fe 3Sn 2nan-odisks obtained by differential phase contrast [15]:(a)roundk π-Skyrmions stabilized at high fields;(b)field B dependent diameter of k π-Skyrmions,the square,triangle,and circle sym-bols in Fig.6b denote the parameter k with values of 4,3,and2,respectively558博看网 . All Rights Reserved.中国材料进展第40卷纳米盘直径可实现可调k参数等特点,有望进一步被应用于新型磁电子学器件的设计中㊂3.3㊀可逆电流调控磁斯格明子-磁泡拓扑磁转换中心对称Fe3Sn2材料中有两种局域磁结构:磁斯格明子和磁泡㊂传统的磁斯格明子基存储器是将磁斯格明子和铁磁态看作数据比特的 1 和 0 [29]㊂但是由于热扰动和斯格明子间的相互作用[33,71],斯格明子的非定向运动会造成数据链的混乱㊂而为了抑制斯格明子的无序运动,需要在传统斯格明子基存储器中的每个数据比特位构建人工缺陷,这无疑会增加器件构建的成本㊂我们提出采用磁泡替代传统铁磁空隙当作数据比特 0 来构建磁斯格明子-磁泡存储器,如图7a~7d所示[18]㊂当磁场完全垂直于Fe3Sn2(001)纳米结构时,为了使偶极-偶极相互作用能最小化,柱状畴形成具有闭合磁畴的磁斯格明子稳定相㊂当磁场不是完全垂直于Fe3Sn2 (001)纳米结构而具有大的面内磁场时,为了使赛曼能最小化,柱状畴形成具有朝向面内磁场方向磁畴的磁泡稳定相㊂当磁场的倾斜角度适中时,磁斯格明子和磁泡是稳定共存,也是磁斯格明子-磁泡存储器实现的前提㊂在强受限Fe3Sn2(001)纳米条带中,通过施加一个5ʎ倾斜的磁场,成功实现了磁斯格明子-磁泡单链(图7e),这种磁斯格明子-磁泡单链被当作一串数据比特㊂图7㊀一种基于磁斯格明子和磁泡的存储器原型的提出[18]:(a)斯格明子-磁泡存储器概念设计图;(b)代表数据比特 1 的斯格明子磁结构;(c)用磁泡替代铁磁来代表数据比特 0 ;(d)磁泡的菲涅尔磁衬度;(e)Fe3Sn2纳米条带中实现的磁斯格明子-磁泡单链,可以用来代表磁斯格明子-磁泡存储器中的一串 11011000001 数据链Fig.7㊀Propose of a magnetic memory based on Skyrmions and bubbles[18]:(a)schematic design of Skyrmion-bubble-based magnetic memory;(b)a Skyrmion representing the data bit 1 ;(c)a bubble replacing ferromagnet to represent the data bit 0 ;(d)Fresnel contrast of the bubble;(e)experimental realization of a single Skyrmion-bubble chain to represent the data bit11011000001 in a Fe3Sn2nanostripe㊀㊀磁斯格明子和磁泡的拓扑荷分别为1和0,具有截然不同的拓扑相关物性,如斯格明子霍尔效应和拓扑霍尔效应[72-75]㊂可控的磁斯格明子和磁泡的产生及其相互转换能够促进拓扑相关的磁电子学器件的开发㊂依据磁斯格明子和磁泡的产生机制,通过倾转外磁场能够有效调控磁斯格明子和磁泡的产生和转换[21,50]㊂本课题组[19]研究了Fe3Sn2纳米盘中磁斯格明子和磁泡的稳定性以及他们之间磁场诱导的拓扑磁转换,发现磁盘中磁斯格明子和磁泡的数量不仅与纳米盘直径有关,还与磁场角度相关㊂当纳米盘直径减小到~540nm时,该受限结构中最多只能稳定一个磁斯格明子或磁泡㊂通过固定外磁场强度同时调节其相对于磁盘法向的角度,成功实现了单斯格明子-单磁泡间可控的拓扑磁转换,如图8所示㊂两类磁状态间的拓扑磁转变可以用于器件的写入和删除等功能,但磁场方法不兼容于当代和未来的电子学器件设计和应用,而电学调控磁斯格明子-磁泡的拓扑转变的研究仍有待发掘㊂因此,本课题组进一步探索了电流可控磁斯格明子-磁泡相互转变的可能性[17]㊂在Fe3Sn2(001)纳米薄片中,磁场小角度倾斜于薄片法向时,磁斯格明子和磁泡都是稳定的磁状态㊂当设置磁斯格明子晶格为初始磁状态,施加高密度纳秒电流脉冲后,会发生磁斯格明子到磁泡的转变;当设置磁斯格658博看网 . All Rights Reserved.㊀第11期汤㊀进等:透射电镜差分相位分析技术磁畴研究图8㊀Fe 3Sn 2纳米结构中磁场诱导的斯格明子-磁泡转换[19]:(a~e)洛伦茨模式观测的斯格明子-磁泡转换,(f ~j)对应的微磁模拟的斯格明子-磁泡转变,(k)斯格明子-磁泡转变过程中的拓扑数的变化,(l)斯格明子-磁泡转变过程中的总自由能密度随磁场角度的变化Fig.8㊀Field-induced topological Skyrmion-bubble transformations in Fe 3Sn 2nanodisks [19]:(a ~e)Skyrmion-bubble transformationsobtained by Lorentz-TEM,(f ~j)corresponding Skyrmion-bubble transformations obtained by micromagnetic simulation,(k)winding number as a function of tilted field angle,(l)total free energy density as a function of tilted field angle明子晶格为初始磁状态,施加低密度纳秒电流脉冲后,会发生磁泡到磁斯格明子的转变㊂重要的是,通过调控电流幅度,这种磁斯格明子-磁泡相互转变是完全可逆的,如图9所示[17]㊂利用微磁学计算模拟发现,电流可控磁斯格明子-磁泡相互转变可被归因于自旋转移力矩和焦耳热效应的综合作用㊂当施加高密度电流脉冲时,电流的焦耳热会导致样品升温而发生热退磁,而在两个电流脉冲的间隙,样品又会降温而发生磁恢复过程㊂在热退磁的过程中,样品的饱和磁场强度会降低,而外加磁场强度固定不变,因此会发生磁斯格明子到铁磁态的转变㊂由于磁场是倾斜于样品垂直方向的,因此铁磁态是具有一定面内分量的倾斜铁磁态,面内磁化分量平行于面内磁场分量㊂而在降温的磁化恢复过程中,由于磁泡的畴壁磁化是与倾斜磁化背景一致,因此磁泡更优先于磁斯格明子从倾斜磁化背景中产生㊂特别地,即使磁泡的总自由能能量高于磁斯格明子,这种磁斯格明子到倾斜铁磁到磁泡转变的过程也能够发生㊂而低密度脉冲电流诱导的磁泡到磁斯格明子的产生归因于自旋转移力矩效应㊂磁泡的能量要高于磁斯格明子,自旋转移力矩相当于一个外界激发,能够使高能亚稳磁泡产生变形而处于一个非稳定状态,从而能够越过能量势垒转变到低能磁斯格明子稳定态㊂此外,在Fe 3Sn 2(001)纳米薄片中,在较低外磁场下,磁泡会转变为条纹磁畴㊂之前的研究中已经能够实现电流控制条纹磁畴到磁斯格明子的转变,但其逆过程磁斯格明子到条纹磁畴的转变还比较少见[31,76-82]㊂通过高低纳秒脉冲电流切换,同样能够实现磁斯格明子-条纹磁畴的可逆和可重复的拓扑磁转换㊂4㊀结㊀语本文阐述了将差分相位分析技术应用到偶极磁斯格明子/磁泡材料Fe 3Sn 2中的新型磁结构观测和电驱动拓扑磁转变动力学研究中的进展,研究结果表明,差分相位技术推动了三维磁结构㊁靶磁泡/k π-磁斯格明子等新型磁结构的精确表征,澄清了中心对称晶体中复杂磁结构的起源,并为后续的新型磁结构相关自旋电子学的应用奠定了重要基础㊂本课题组也提出了磁斯格明子-磁泡存储器的概念设计,并在实验室实现了单链磁斯格明子-758博看网 . 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Recently,topological insulator has attracted great interests due to its peculiar band structures and electronic properties.The two-dimensional quantum spin Hall systems and three-dimensional TIs including Bi2Se3,Bi2Te3,and Bi1-xSbx have theoretically proposed and experimentally observed.They have a bulk excitation gap and gapless edge states for 2D TIs and 2D surface at boundaries:1D edge states for 2D TIs and 2D surface states for 3DTIs.The surface states of 3D TIs with an odd number of Dirac cones are robust against(weak and nonmagnetic)disorder scattering and many-body interactions.The Bi2Se3 material has been predicted and verified to have a bulk gap of 0.3 eV and a single Dirac come of surface states.The 3D TIs are expected to show several unique properties when the time reversal symmetry is broken.The latter can be realizes directly by a ferromagnetic insulating(FI) layer attached to the 3D TI surface.The motion of the Dirac electrons is influenced mainly by the magnetization of the FI layer rather than its stray field.This is in contrast to the Schodinger electrons in conventional semiconductor heterostructures modulates by nanomagnets.Some features of Dirac fermions on the surface of a TI have been revealed in the presence of proximate FIfilms,which have no analog in either graphene or 2D Schrodinger electrons.However,the effect of a magnetic superlattice on such kind of 2D carriers has not been examined so far.In this work,we study the band structures and ballistic transport of Dirac electrons on the TI surface under the modulation of a periodic magnetic superiattice.For a finite superlattice,when half of the FI stripes switch their magnetization directions a tunneliing magnetoresistance (MR) witha tunable sign is obtained. The system under consideration is a 2D electron gas on a given surface of a 3D TI like Bi2Sw3,as sketched in Fig.1.The surface is taken to be the(x,y) plane.Two kinds of FI materials with different coercive fields are deposited alternatively on top of the surface to form a magnetic superlattice along the x axis.For simplicity,we assume that all FI stripes have the same width a/2 and magnetization strength mo.The smallest distance between them is a/2.The magnetization of a FI stripe induces an exchange field for the Dirac fermions due to the proximity of TI and ferromagnetism.The easy axis of a FI stripe is usually along its length direction and thus either in parallel(p)or antiparallel (AP) with the +y axis.The initial magnetic superlattice with such a magnetization configuration is shown in Fig.1(a),which has a lattice constant a.For the soft FI material,a small in-plane magnetic field can switch its magnetization orientation.Accordingly,the magnetizations of adjacent FI stripes are changes fron the P to the AP alignment while the lattice constant of the magnetic superlattice turns to be 2a.In the presence of the periodic exchange field generated by N FI stripes,the motion of eletrons on the TI surface can be described by the 2D Dirac Hamiltonianwhere vF is the Fermi velocity,P=(px,py) is the electron momentum,7x and *y are Pauli matrices in spin space,M is the effective exchange field,and my(x) takes a constant value mo in the stripe regions with magnetization aligned to the y axis and zero otherwise.For convenience we express all quantities in dimensionless units by means of the length of the basic unit a and the enegy &*.For a typical value of a=50 nm and the Bi2Se3 material,one has Eoowing to the translational invariance of the system along the y direction,the total wave function of Dirac electrons can be expressed as &&,where ky is the transverse wave vector.At each region with a constant exchange field my,the reduced one-dimensional wave function & for a givenincident energy E can be written aswhere & and & together with the wave amplitudes c(x) and d(x) are piecewise constant.From the requirement of wave function continuity and the scattering boundary conditions,the transmission amplitude t can be calculated by means of the scattering matrix method.Note that t depens strongly not only on the incident energy Eand the transverse wave vector k,but also on the magnetization configuration.The ballistic conductance at zero temperature can be expressed in terms of the transmission amplitudewhere & is the incident angle relative to the x direction.Ef is the Fermi energy ,& is taken as the conductance unit,and & is the length of the device in the y direction.In order to understand the effect of the periodic exchange field on the transport properties of Dirac electrons,it isinstructive to investigate the band structures of a perfect magnetic superiattice on the surface of a 3D TI.For a given Bloch wave vector k ,the band energy E(k) can be derived analytically from the continuity requirement of the wave function and the periodic boundary condition of the superlattice.For the P magnetization configuration shown in Fig.1(a),the transcendental equation is given byNote that the exchange field in this configuration is equivalent to a periodic array of fictitions & magnetic fields with the same height but alternative sign.The result is thus the same as that in Ref.18.It should be emphasized that the physical origin of the magnetic superlattice in Ref.18 is distinct from that considered here.For the AP magnetization configuration shown in Fig.1(b),the analytical expression of the dispersive relation reads Fig.2 (Color online) Dispersion relations of Dirac electrons modulated by the magnetic superlattic witha P and AP configuration.In&and * the band energy Eat two k,values,ky=0(solid line) and ky=-1(dashed line),is plotted as a function of the Bloch wave vector k under the magnetization strenths mo=2 and m0=3.In c and f the variation in E with k,is plotted under two magnetization strengths mo=2 (circle marks) and mo=3(triangular marks)It is clearly seen from Eqs.4and5 that for a given mo and ky the Bloch wave vector k is only relevant to E.Thus the energy spectrum is symmetric with respect to E=0.Hereafter we consider only the nonnegative energy regime.The condition for the analytical expressions.For the Pmagnetization alignment & and the zero-energy solution requires k=0 and & .As for the AP configuration,the system has a symmetry related with the operator T,where T is the time reversal and R is the reflection X (x is a central point of the superlattice).The energy spectrum is thus symmetric about ky =0.The zero-energy solution appears only when k=0 and ky=0.Note that for both cases the zero-energy solution is unique and the transverse velocity & should vanish at &.For a general ky and mo a band gap including the point E=0 will be opened by the periodic magnetic modulation.The size of the band gap depends on the values of ky and mo.The general band features discussed above are reflected in the numerical solutions of Eqs.4and5,which are shown in Fig.2.It canbe observes that around the zero-energy solutions the energy spectrum is linear.Thus the Diac point is shifted by the magnetic superlattice with the P configuration but is unchanged in the AP configuration.In both cases,the velocity of the linear spectrum depends on mo.For E>k,the ky-dependent term in Eq.1 can be viewed as a perturbation,resulting in a slow variation in E with ky.For the same ky and mo the band gap of the P configuration overlaps only partly with that of the AP alignment.This may lead to a tunneling MR with a tunable sign.Figure 3 presents the trandmission probability as a function of the Fermi energy and the incident angle & for mo=2.The number of FI stripes is chose to be N=50.The transmission spectrum demonstrate an obvious angular anisotropy for both the P and AP alignment.For the P alignment t is blocked for all incident angles when the incident energy E locates in the full transmission gap.This can be understood from two aspects.One is that in the superlattice region there exists a band gap including E=0 for a large .The transmission is usually rather small as the incident energy falls into a band gap.The other aspect is that for & although the band gap of the incident region requires &.Outside the full transmission gap a large transmission is usually allowable for a negative angle &.The reason is that in the superlattice region the Dirac point is shifted to the k-point.Resonant features under positive incident angles can be seen due to the presence of quasibound states.For the AP alignment the transmission shown in Fig.3b is symmetric with respect to the angle&,as a result of the symmetry mentioned above.The reflection is almost complete in the whole & region for E=&,which is a common part of the band gaps for all available ky.As demonstrated above,the transmission features for the P and AP confifurations are quite distinct.Such a difference is also exhibited in the measurable quantity, the conductance G and G.In Fig.4 the conductance is plotted as a function of the Fermi energy for several values of the exchange field.For a amall mo,there exist several conductance valleys for both the P and AP alignment.With the increasing of mo the valleys move toward the high-energy region and become wider and lower.Finally,the valleys will turn to a conductance-forbidden region.When E lies in the full transmission gap of the P(AP) alianment,the conductance & is rather small while the conductance & can be large.The MR ratio is defined as 7 .The conductance spectrum in Fig.4 indicate a large ME amplitude in the full transmission gaps of both the P and AP alignmeng\t.Since the two kinds of full transmission gaps may have no overlap,the sign of the MR is alternated as the Fermi energy increases.In summary, we have studied the band structures and transport features of Dirac electrons on the surface of a 3D TI subject to a periodic exchange field.The superlattice modulation is provided by a series of equally spaced FI stripes which sre attached to the TI surface.The magnetizations of adjacent FI stripes can be switched between the parallel and antiparallel configurations.The Dirac point is shifted by the magnetic superlattice,we have shown a full transmission gap for both the parallel and antiparallel configurations.For a suitable range of the magnetization strength,the two kinds of trnsmission gaps are nonoverlapped and thus a large MR with a tunable sign can be achieved.。
CROSSOVER BETWEEN MAGNETIC REVERSAL MODES IN ORDERED Ni AND Co NANOTUBEARRAYSMARIANA P.PROENCAIFIMUP and IN ÀInstitute of Nanoscience and Nanotechnologyand Departamento de F {sica eAstronomia,Universidade do Porto,Rua do Campo Alegre 6874169-007Porto,PortugalInstituto de Ciencia de Materiales de MadridCSIC,28049Madrid,SpainCELIA T.SOUSA,JOAO VENTURA and JOAO P.ARAUJO IFIMUP and IN ÀInstitute of Nanoscience and Nanotechnologyand Departamento de F {sica e Astronomia Universidade do Porto,Rua do Campo Alegre 6874169-007Porto,PortugalJUAN ESCRIG Departamento de F {sicaUniversidad de Santiago de Chile (USACH ),andCenter for the Development of Nanoscience and Nanotechnology (CEDENNA )Avneda Ecuador 3493,Santiago,ChileMANUEL VAZQUEZInstituto de Ciencia de Materiales de MadridCSIC,28049Madrid,Spain mvazquez@icmm.csic.esReceived 16July 2012Accepted 6October 2012Published 28January 2013Ordered arrays of Ni and Co nanowires and nanotubes,with diameters between 30nm and 60nm,were prepared by electrodeposition into nanoporous alumina templates.The study of the corre-sponding magnetization reversal processes was performed by analyzing the angular dependence of coercivity (H c )and using a simple analytical model.The agreement between experimental and theoretical data shows that magnetization in nanowire arrays reverses by means of nucleation and propagation of a transverse domain wall,independently of the diameter.However,a critical di-ameter of $50nm was found in the case of nanotubes,above which a nonmonotonic angular dependent H c was observed,evidencing a transition between vortex and transverse reversal modes.Keywords :Nanotubes;nanowires;magnetization reversal;domain wall;alumina templates.SPINVol.2,No.4(2012)1250014(7pages)©World Scienti¯c Publishing Company DOI:10.1142/S2010324712500142S P I N D o w n l o a d e d f r o m w w w .w o r l d s c i e n t i f i c .c o m b y 94.132.87.244 o n 02/05/13. F o r p e r s o n a l u s e o n l y .1.IntroductionWith the growing interest in nanotechnology,nanomaterials are becoming increasingly important.Spherical nanoparticles have been produced,o®er-ing potential applications in a diversi¯ed set of ¯elds,ranging from biomedicine 1to energy storage.2However,nanowires (NWs;high aspect ratio nano-particles)and nanotubes (NTs)exhibit aniso-tropic (shape-dependent)collective properties (e.g.photoluminescence,conductivity,magnetization),3,4increasing the number of degrees of freedom that can be manipulated.For magnetic applications such as sensors or media,it is important to study both the domain structure and magnetic con¯guration within the NW/NT arrays,and their dependence on geometry,element size (and shape)and inter-element distance.5À8As the size is reduced,the balance between di®erent energies (magnetostatic,magnetocrystalline,exchange,thermal)can be criti-cally altered,drastically a®ecting domain con¯g-uration.9À12The detailed physical study of such assemblies can give us the ability to tune competing interactions,searching for novel phenomena induced by nanoscopic con¯nement or proximity e®ects.The major applications of magnetic nanomater-ials require a thorough understanding of the mag-netization reversal mechanisms.These are in turn directly related to the coercivity,13À15and depend on geometric parameters such as shape,length,diameter,wall thickness or spatial ordering.16À18The accurate control of such parameters,combined with a detail study of the nanomaterial's magnetic properties,provides new information on the appli-cation of each nanomagnet array.Additionally,it eases the tuning of the magnetization reversal mode by external parameters,such as the direction of the applied magnetic ¯eld.A limited number of studies have been reported on the angular dependent magnetic properties of NW and NT arrays fabricated inside nanopore templates (polycarbonate track etched mem-branes,19,20inclined Si columns.21)Even scarcer experimental results on the angular dependence of the coercivity in highly ordered NW/NT arrays have been obtained.16,21À25Additionally,the prep-aration of NTs with small diameters (d <60nm)is a di±cult and complex task,so that most of the reports on the magnetic properties of NT arrays correspond to outer diameters of d $200nm.26À30Interesting changes in the magnetic behavior whenreducing the NTs diameter have been theoretically predicted,17but they remain an open question as the corresponding experimental evidence is still limited.In particular,theoretical calculations predict the existence of a critical diameter ($10À50nm)in ferromagnetic NTs,below which the magnetization reverses by a transverse mechanism,and above which a vortex mode is expected to occur.17How-ever,this critical diameter was not yet found ex-perimentally,as the magnetization reversal modes have only been reported for ferromagnetic NTs with d >100nm.In this work,Ni and Co NW and NT arrays with small diameters ($30À60nm)were fabricated by controlled potentiostatic deposition into highly ordered nanoporous alumina templates (NpATs).A comparative study of the magnetization reversal processes of NW/NT arrays was performed by measuring the angular dependence of the coercivity for each sample.Experimental evidence of the transition between two magnetization reversal modes was achieved for NTs with d $50À60nm and con¯rmed by analytical calculations,showing that for both Co and Ni there is a critical diameter of $50nm,below which a transverse reversal mode occurs,as theoretically predicted.2.Experimental DetailsLong range ordering of hexagonal symmetry of precursor alumina membranes was achieved using a two-step anodization process of high purity (99.999%)aluminum disks.31Interpore distances of 65nm and 105nm were obtained by anodizing at 25V and 2 C in 0.3M sulfuric acid,and at 40V and 4 C in 0.3M oxalic acid,respectively.First anodizations were performed for 24h,while second anodizations lasted for 20h leading to $50 m thick membranes.For subsequent electrodeposition,the nanopores were opened at the bottom by chemical etching of Al in an aqueous solution of 0.2M CuCl 2and 4.1M HCl at room temperature,and chemical dissolution of the alumina bottom barrier layer in 0.5M phos-phoric acid.32Pore widening using phosphoric acid was also performed in selected samples to obtain pore diameters of d $50À60nm.A thin Au layer ($120nm)was then sputtered on the backside of the membrane to serve as the working electrode in a three-electrode cell.For the growth of NTs,a smaller Au layer thickness ($30À60nm;dependingM.P.Proenca et al.S P I N D o w n l o a d e d f r o m w w w .w o r l d s c i e n t i f i c .c o m b y 94.132.87.244 o n 02/05/13. F o r p e r s o n a l u s e o n l y .on the pore diameter)was deposited so as not to completely close the bottom of the pores,followed by the coating of a nonmetallic protective ¯lm at the bottom of the metallic contact.33In this case,electrodeposition results in the formation of NTs along the internal side of the pores.A Pt mesh and Ag/AgCl (in 4M KCl)were used as the counter and reference electrodes,respectively.Ni and Co were electrodeposited inside the nanopores using an aqueous solution of 1.14M NiSO 4Á6H 2O +0.19M NiCl 2Á6H 2O +0.73M H 3BO 3at 35 C,and 0.89M CoSO 4Á7H 2O +0.49M H 3BO 3at 30 C,respectively.The electrodepositions were performed in potentiostatic mode at À1:5V for $2min,using a Solartron 1480MultiStat.The fabricated NWs and NTs had a ¯nal diameter equal to that of the pores of the template [d ¼ð30;50and 60ÞÆ4nm],NT wall thicknesses of t ¼ð8À12ÞÆ3nm,and aspect ratios (length/diameter)higher than 50.Morphological charac-terization was performed using a scanning and a scanning transmission electron microscopes (SEM and STEM,respectively;FEI Quanta 400FEG).Prior to SEM bottom images,the Au contact at the bottom of the NpATs was etched by ion-milling using an ion beam sputter deposition system by the Commonwealth Scienti¯c Corporation.33Sample preparation for STEM imaging was performed by chemically etching the NpAT in 0.2M H 2CrO 4+0.4M H 3PO 4at 60 C and subsequently disperse the NTs in ethanol.Figures 1(a)and 1(b)show SEM bottom images (after $200nm of ion-milling)of the obtained NWs and NTs inside NpATs with pore diameters of d $50À60nm and interpore distance of105nm.Figure 1(c)shows a STEM image of Ni NTs,illustrating the tubular shape with a hollow core and an homogeneous wall thickness along the tube.3.Results and DiscussionTo investigate the magnetization reversal processes of the NW and NT arrays,magnetization hysteretic loops were measured at di®erent angles ( )of applied external magnetic ¯eld (H ),using a vibrat-ing sample magnetometer (VSM;LOT-Oriel EV7).Figure 2shows the magnetic hysteretic loops measured for Ni NTs,with diameters d $60nm and wall thickness t $12nm,evidencing an increase in the coercive ¯eld (H c )for >0 ,followed by a decreasing trend for >70 .Three main modes of magnetization reversal have been previously identi¯ed depending on the geo-metry of the system under study:coherent mode (C),where all magnetic moments rotate simul-taneously;transverse mode (T),where spins rotate progressively by the nucleation and propagation of a transverse domain wall;and vortex mode (V),where a vortex wall is nucleated and propagates.17A simple analytical model has been proposed to account for the angular dependence of the coercive ¯eld of each of the above magnetization reversalprocesses (H ic;i ¼C ,T and V).14,17,34For the coherent magnetization reversal case one can directly apply the Stoner ÀWohlfarth model to estimate the nucleation ¯eld 13:H Cn ¼ÀM Sat1À3N z ðL Þ2ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi1À 2þ 4p 1þ 2;ð1ÞFig.1.SEM bottom (after $200nm of ion-milling)images of (a)Co NW and (b)Ni NT arrays in NpATs with d $50nm and 60nm,respectively.(c)STEM image of Ni NTs.Crossover Between Magnetic Reversal ModesS P I N D o w n l o a d e d f r o m w w w .w o r l d s c i e n t i f i c .c o m b y 94.132.87.244 o n 02/05/13. F o r p e r s o n a l u s e o n l y .where ¼tan 1=3ð Þ,N z is the demagnetization factor of a wire/tube along the z (long)axis,and M Sat is the saturation magnetization (¼4:9Â105and 1:4Â106A m À1for Ni and Co,respectively).Since the Co NWs and NTs fabricated in this work are polycrystalline (not shown),evidencing a mix-ture of cubic and hexagonal crystalline phases,the magnetocrystalline anisotropy constant is very small and was not included in our calculations.It was also shown that the coercivity can be written as a function of the nucleation ¯eld as 13:H Ccð Þ¼j H Cn ð Þj 0 45 2j H C n ð ¼45 Þj Àj H C n ð Þj 45 90:(ð2ÞFor a generalized description of our geometricalsystem,it is convenient to de¯ne the ratio ¼d i =d ,where d i and d are the inner and outer tube diam-eters,respectively (inset of Fig.2).In this work,we have $0:4and 0.7for the fabricated NTs with d $30nm and 50À60nm,respectively.On the other hand, ¼0for NWs.The dependence of the demagnetization factor on was calculated by Escrig et al.,and is given by 35:N z ðL Þ¼d L ð1À 2ÞÂZ 11Àe À2yL =dy 2½J 1ðy ÞÀ J 1ð y Þ 2dy ;ð3Þwhere J 1is the Bessel function of the ¯rst kind and order one.For the transverse mode an adapted Stoner ÀWohlfarth model has been proposed.16In this model,the nucleation ¯eld of a system that reverses its magnetization by means of the nucleation and propagation of a transverse domain wall is assumed to be equivalent to the nucleation ¯eld of a system with an e®ective volume that reverses its magneti-zation by coherent rotation.The e®ective volume considers the transverse domain wall width (w T ),which can be estimated depending on geometrical parameters.10,17We can therefore use Eqs.(1)À(3)to calculate H T c ( ),replacing L with w T .Finally,the angular dependence of the nucleation ¯eld in the vortex mode can be estimated using 36:H V n M Sat¼ðN z À 2ÞðN x À 2ÞffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiðN z À 2Þ2sin 2 þðN x À 2Þ2cos 2q ;ð4Þwhere ¼2qL ex =d ,L ex ¼ffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi2A = 0M 2Satq is the ex-change length,A is the magnetic sti®ness constant (here considered 0:9Â10À11J m À1for Ni and 3:0Â10À11J m À1for Co)10,37and q satis¯es 38:qJ 0ðq ÞÀJ 1ðq ÞqY 0ðq ÞÀY 1ðq Þ¼ qJ 0ð q ÞÀJ 1ð q ÞqY 0ð q ÞÀY 1ð q Þ;ð5Þwhere J p and Y p correspond to the Bessel functions of the ¯rst and second kind,respectively,and order p .Considering the wire/tube symmetry,one has N x ¼N y ¼ð1ÀN z Þ=2.In the V mode,the coercivity is very close to the absolute value of thenucleation ¯eld,and we thus use H V c ¼ÀH Vn ,as in previous works.14,21,37Figures 3and 4show the angular dependence of the coercivity for the Co and Ni samples,respect-ively.In the NW arrays,the coercivity always decreases as increases,showing a monotonic behavior.The coercivity estimated using the coher-ent magnetization reversal mode gives much higher values than those experimentally obtained (Fig.3).As previously reported by Landeros et al.,17coherent magnetization reversal is only present in very short wires/tubes where L %w T or less.For long NWs the reversal of magnetization is achieved through the nucleation and propagation of a transverse domain wall.Our analytical calculations con¯rm the pre-sence of a transverse magnetization reversal mode for all NW arrays [Figs.3and 4,(a)and4(b)].Fig.2.Magnetic hysteretic loops of ordered Ni NT arrays with d $60nm and d i $36nm,measured at di®erent angles of applied magnetic ¯eld,with a 10 step.M.P.Proenca et al.S P I N D o w n l o a d e d f r o m w w w .w o r l d s c i e n t i f i c .c o m b y 94.132.87.244 o n 02/05/13. F o r p e r s o n a l u s e o n l y .Fig.3.Angular dependence of the coercive ¯eld measured experimentally (squares)and calculated analytically (C mode:blue solid;T mode:red dashed;and V mode:green dotted)for Co NW [(a)and (b)]and NT [(c)and (d)]arrays in NpATs with di®erent outer diameters (coloronline).Fig.4.Angular dependence of the coercive ¯eld measured experimentally (squares)and calculated analytically (C mode:blue solid;T mode:red dashed;and V mode:green dotted)for Ni NW [(a)and (b)]and NT [(c)and (d)]arrays in NpATs with di®erent outer diameters (color online).Crossover Between Magnetic Reversal ModesS P I N D o w n l o a d e d f r o m w w w .w o r l d s c i e n t i f i c .c o m b y 94.132.87.244 o n 02/05/13. F o r p e r s o n a l u s e o n l y .The same is observed in the case of NT arrays with very small outer diameters ($30nm)[Figs.3and 4,(c)].However,NT arrays with d &50nm il-lustrate a non-monotonic behavior,where H c starts by increasing with ,reaching a maximum value at T ¼0 ,and then decreases for > T [Figs.3and 4,(d)].This inhomogeneous behavior evidences a transition from two di®erent magnetization reversal processes (transverse and vortex modes).The analytical calculations obtained for the magnetization reversal modes of NT arrays with d &50nm are plotted in Figs.3(d)and 4(d),for Co and Ni,respectively.Since the system reverses its magnetization by the mode that o®ers the lowest coercivity,the analytical calculations allow the identi¯cation of the magnetization reversal modes expected for each system.The good agreement found between the analytical calculations and the experimental data of the angular dependence of coercivity [Figs.3(d)and 4(d)]evidences the exist-ence of a crossover between the vortex and the transverse reversal modes,occurring at theoretically predicted angles very close to the experimentally obtained maxima.The small di®erences between the experimental data and the analytical calculations can be explained by deviations from the NTs cross-section from perfect circular shape and dipolar in-teractions of neighboring NTs.16,21,344.ConclusionIn summary,the angular dependence of the coer-civity was measured for Ni and Co NW and NT arrays with small diameters (between 30and 60nm).For NTs with d &50nm we reported ex-perimental evidence for an angular dependent transition of magnetization reversal modes,which had been theoretically predicted.Analytical calcu-lations then allowed us to identify a transverse reversal mode for all NW and NT arrays with d $30nm,and a transition between the vortex and transverse reversal modes occurring for NTs with d $50À60nm.Due to the additional degree of freedom provided by the hollow core in the NT centre,the fabrication of tubular structures shown here with di®erent inner and outer diameters pro-vides the ¯rst step toward the design of a sensor device with NT arrays of di®erent inner/outer diameter ratios,with enhanced sensitivity by pro-viding a broader angle of detection.AcknowledgmentsMPP and CTS are thankful to FCT for doctoral and post-doctoral grants SFRH/BD/43440/2008and SFRH/BPD/82010/2011,respectively.JE acknowledges ¯nancial support from FONDECYT 1110784,Grant ICM P10-061-F by the Fondo de Innovaci ón para la Competitividad-MINECON,and the Financiamiento Basal para Centros Cien-t í¯cos y Tecnol ógicos de Excelencia FB0807.JV acknowledges ¯nancial support through FSE/POPH.MV thanks the Spanish Ministry of Econ-omia y Competitividad,MEC,under project MAT2010-20798-C05-01and Spanish-Chilean CSIC-USACH Bilateral Project 2010CL0018.JPA also thanks the Funda ção Gulbenkian for its ¯nan-cial support within the \Programa Gulbenkian de Est ímulo àInvestiga ção Cient í¯ca".The authors acknowledge funding from FCT through the Associated Laboratory —IN.References1.R.Bardhan,l,A.Joshi and N.J.Halas,Acc.Chem.Res.44,936(2011).2.G.Polizos,V.Tomer,E.Manias and C.A.Randall,J.Appl.Phys.108,074117(2010).3.K.D.Sattler,Handbook of Nanophysics:Nanotubes and Nanowires (CRC Press,USA,2010).4.S.S.P.Parkin,M.Hayashi and L.Thomas,Science 320,190(2008).5.M.Daub,M.Knez,U.Gosele and K.Nielsch,J.Appl.Phys.101,09J111(2007).6.J.Bachmann,J.Jing,M.Knez,S.Barth,H.Shen,S.Mathur,U.Gosele and K.Nielsch,J.Am.Chem.Soc.129,9554(2007).7.S.J.Son,J.Reichel,B.He,M.Schuchman and S.B.Lee,J.Am.Chem.Soc.127,7316(2005).8.K.Nielsch,F.J.Castano,S.Matthias,W.Lee and C.A.Ross,Adv.Eng.Mater.7,217(2005).9. 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a r X i v :c o n d -m a t /0607711v 2 [c o n d -m a t .s t r -e l ] 1 S e p 2006Magnon Bose condensation in symmetry breaking magnetic field S.V.Maleyev,V.P.Plakhty,S.V.Grigoriev,A.I.Okorokov and A.V.Syromyatnikov Petersburg Nuclear Physics Institute,Gatchina,Leningrad District 188300,Russia E-mail:maleyev@.spb Abstract.Magnon Bose condensation (BC)in the symmetry breaking magnetic field is a result of unusual form of the Zeeman energy that has terms linear in the spin-wave operators and terms mixing excitations which momenta differ in the wave-vector of the magnetic structure.The following examples are considered:simple easy-plane tetragonal antiferromagnets (AFs),frustrated AF family R 2CuO 4,where R=Pr,Nd etc.,and cubic magnets with the Dzyaloshinskii-Moriya interaction (MnSi etc.).In all cases the BC is important when the magnetic field is comparable with the spin-wave gap.The theory is illustrated by existing experimental results.1.Introduction Magnon Bose condensation (BC)in magnetic field was intensively studied in spin singlet materials (see for example [1]and references therein).In this case magnons condens in the field just above the triplet gap.In this paper we consider magnon BC that appears in the symmetry breaking magnetic field.The theoretical discussion is illustrated by experimental observation of this BC in frustrated antiferromagnet (AF)Pr 2CuO 4and cubic helimagnets MnSi and FeGe.To clarify our idea we begin with consideration of conventional AFs.In textbooks two limiting cases are considered.First,the magnetic field is directed along the sublattices.In this case the system remains stable up to the critical field H C =∆,where ∆is the spin-wave gap.Then the first order transition occurs to the state in which the field is perpendicular to sublattices (spin-floptransition).Second,the field is perpendicular to initial staggered magnetization.The system remains stable but the spins are canted toward the field by the angle determined by sin ϑ=−H/(2SJ 0),where J 0=Jz ;J and z are the exchange interaction and the number of nearest neighbors,respectively.At H +2SJ 0the spin-flip transition occurs to the ferromagnetic state.To the best of our knowledge the first consideration of the symmetry breaking field was performed theoretically in [2]in connection with experimental study of the magnetic structure of the frustrated AF R 2CuO 4,where R=Pr,Nd,Sm and Eu [3,4].In these papers the non-collinear structure was observed using the neutron scattering in the field directed at angle of δ=450to the sublattices.It was found in[2]that in inclinedfield the Zeeman energy has unusual form with terms which are linear in the spin-wave operators and term mixing magnons which momenta differ in the AF vector k0.As a result the BC arises of the spin-waves with momenta equal to zero and±k0.Similar situation exists in cubic helimagnets MnSi etc.[5].If thefield is directed along the helix wave-vector k the plain helix transforms into conical structure and then the ferromagnetic spin state occurs at criticalfield H C.But if H⊥k the magnon condense with momenta zero,±k,±2k etc.This leads to the following observable phenomena:i)a transition to the state with k directed along thefield at H⊥∼H C1=∆√S/2(a l−a+l),l=1,2 and a l(a+l)are Bose operators.As a result the Zeeman energy has unusual formH Z=H a+q+k0a q+iϑN,i.e. these operators has to be considered as classical variables as in the Bogoliubov theory of the BC in dilute Bose gas.Due to thefirst term in(2)we must consider the operatorsa±k0and a+∓kas classical variables too.Minimizing the full Hamiltonian with respectto these variables we obtainE=(∆2sin22ϕ)/(16J0)−S2J0ϑ2−(H H⊥)2/[4J0(∆2(ϕ,H)],(3)where thefirst term is the energy of the square anisotropy.In cuprates with S=1/2ithas quantum origin and arises due to pseudodipolar in-plane interaction[9].The secondterm is the energy of the spin canting in perpendicularfield.The last term is the BCenergy and∆2(ϕ,H)=∆2cos4ϕ+H2⊥−H2 is the spin-wave gap in thefield[2].This contribution becomes important at H∼∆.The spin configuration is determined byd E/dϕ=0and equilibrium condition d2E/dϕ2≥0.This theory was verified by neutrons scattering[10,11].In diagonalfield H (1,1,0)the spin configuration in frustrated Pr2CuO4is governed by Eq.(3)and the intensityof the(1/2,1/2,−1)is given by I∼1+sin2ϕ[2].Neglecting the BC term we getsin2ϕ=−(H/H C)2,where H C=∆.As a result at H→H C we obtain I∼H C−H. But very close to H C the BC term becomes important and we have a crossover to I∼(H C−H)1/2.It is clearly seen infigure2.This crossover was observed in[10,11].3.Frustrated AFsIn frustrated R2CuO4AFs there are two copper spins in unit cell belonging to different CuO2planes(see inset infigure1).From symmetry considerations these spins do not interact in the exchange approximation.The orthogonal spin structure is a result of the interplane pseudodipolar interaction(PDI)[2,3]and the ground state energy is given by∆2E=on T we obtain H C≃7.8T andγC≃5.30that is in stronger disagreement wit the experiment.The experimentally obtained anglesαandγat T=18K andδ=9.50are shown infigure4[12].The transition to the collinear state withα∼−450andγC∼200 was observed.Again the non-BC theory can not explain the experimental data.For example it givesγC≃2.50.Explanation of all these experimental data using the BC theory will be given elsewhere.4.BC in helimagnetsIn helimagnets MnSi etc.Dzyaloshinskii-Moriya interaction(DMI)stabilizes the helical structure and the helix wave-vector has the form k=SD[ˆa׈b]/A,where D is the strength of the DMI,A is the spin-wave stiffness at momenta q≫k,ˆa andˆb are unit orthogonal vectors in the plane of the spin rotation.The classical energy depends on thefield component H along the vector k and the cone angle of the spin rotation is given by sinα=−H/H C,where H C=Ak2is the criticalfield of the transition into ferromagnetic state[5].However at H⊥≪H C rotation of the helix axis toward thefield direction and the second harmonic2k of the spin rotation were observed[6-8].Both phenomena are related to the magnon BC in perpendicularfield[5].The linear and mixing terms appear in the Zeeman energy in much the same way as it was discussed above:H Z=(H a−i H b)2the real form of the BC energy is not so simple.It is determined by nonlinear interactions but consideration of this problem is out of the scope of this paper.As a result the perpendicular susceptibility is proportional to1/(∆2−H2⊥/2)and 2k harmonic appears.The last was observed by neutron scattering[6-8].Intensities of corresponding Bragg satellites have the formI±∼[∆2/(∆2−H2⊥/2)]2[1∓(kP)]δ(q∓2k),(7) where P is the neutron polarization.If H⊥→∆√5.ConclusionsWe discuss a few examples of the magnon BC in symmetry breaking magneticfield.BC appears due to unusual terms in Zeeman energy.Obviously this phenomenon is very general and can be observed in other ordered magnetic systems.Effects related to the BC has to be more pronounced in thefield of order of the sin-wave gap.6.AcknowledgmentsThis work is partly supported by RFBR(Grants03-02-17340,06-02-16702and00-15-96814),Russian state programs”Quantum Macrophysics”,”Strongly Correlated electrons in Semiconductors,Metals,Superconductors and Magnetic Materials””Neutron Research of Solids”,Japan-Russian collaboration05-02-19889-JpPhysics-RFBR and Russian Science Support Foundation(A.V.S.).References1Crisan M,Tifrea I,Bodea D and Grosu I2005Phys.Rev.B721644142Petitgrand D,Maleyev S,Bourges P and Ivaniv A1999Phys.Rev.B5910793D.Petitgrand,Moudden A,Galez P and Boutrouille P1990J.Less-Common Metals164-165768 4ChattpodhayaT,Lynn J,Rosov N,Grigereit T,Barilo S and Zigunov D1994Phys.Rev.B49 99445Maleyev S2006Phys.Rev.B731744026Lebech B,Bernard J and Feltfoft1989J.Phys.:Condens.Matter161057Okorokov A,Grigoriev S,Chetverikov Yu,Maleyev S,Georgii R,B¨o ni P,Lamago D,EckerslebeH and Pranzas P2005Physica B3562598Grigoriev S,Maleyev S,Chetverikov Yu,Georgii R,B¨o ni P,Lamago D,Eckerlebe H and Pranzas P2005Phys.Rev B721344029Yildirim T,Harris A,Aharony A and Entin-Wohlman O1995Phys.Rev.B521023910Plakhty V,Maleyev S,Burlet P,Gavrilov S and Smirnov O1998Phys.Lett.A25020111Ivanov A and Petitgrand D2004J.Mag.Mag Materials272-27622012Plakhty V,Maleyev S,Gavrilov S,Bourdarot F,Pouget S and Barilo S2003Europhys.Lett.61 53413Ivanov A,Bourges P and Petitgrand D1999Physica B259-261879FiguresaFigure 1.Spin configuration in the field.Full and dashed arrows correspond to zero and nonzero field,respectively.Addition spin canting in H ⊥is shown by broken arrows.Inset:spin configuration in neighboring planes of frustrated AF.Figure 2.Log-Log plot of the (1/2,1/2,−1)Bragg intensity in diagonal field,h ∼(H C −H ).Figure3.Thefirst order transition in thefield directed along b axis.Calculated intensities for the spinflop configurations when spins are perpendicular to thefield (white arrows).Figure4.Field dependence of anglesαandγatδ=9.50.)10a H mT =)50b H mT =)150c H mT=Figure 5.Bragg reflections in the field along (1,1,0).a)Four strong spots corresponds to ±(1,1,1)and ±(1,1,−1)reflections.Weak spots are the double Bragg scattering.b)The 2k satellites appear.c)The helix vector is directed along the field.。
PHYSICAL REVIEW B87,195201(2013)Mn-doped monolayer MoS2:An atomically thin dilute magnetic semiconductorAshwin Ramasubramaniam*Department of Mechanical and Industrial Engineering,University of Massachusetts Amherst,Amherst,Massachusetts01003,USADoron Naveh†Faculty of Engineering,Bar-Ilan University,Ramat-Gan52900,Israel(Received21March2013;revised manuscript received30April2013;published13May2013) We investigate the electronic and magnetic properties of Mn-doped monolayer MoS2using a combinationoffirst-principles density functional theory(DFT)calculations and Monte Carlo simulations.Mn dopantsthat are substitutionally inserted at Mo sites are shown to couple ferromagnetically via a double-exchangemechanism.This interaction is relatively short ranged,making percolation a key factor in controlling long-rangemagnetic order.The DFT results are parameterized using an empirical model to facilitate Monte Carlo studies ofconcentration-and temperature-dependent ordering in these systems,through which we obtain Curie temperaturesin excess of room temperature for Mn doping in the range of10–15%.Our studies demonstrate the potential forengineering a new class of atomically thin dilute magnetic semiconductors based on Mn-doped MoS2monolayers.DOI:10.1103/PhysRevB.87.195201PACS number(s):73.22.−f,75.50.PpI.INTRODUCTIONDilute magnetic semiconductors(DMSs)have been the focus of extensive research over the last decade,driven by the prospect of realizing a new generation of electronic devices—so-called spintronic devices—that can exploit both the charge and spin of carriers.1–4To this end,a significant amount of theoretical and experimental effort has been devoted to understanding the role of magnetic impurities such as Mn and Co in technologically important III-V and II-VI semiconductors,as discussed in several reviews.1–5Among several challenges that persist in the development of spintronic devices,perhaps the most significant hurdle remains the control of the ordering temperature,which should ideally be well above room temperature to enable practical applications. The search for such room-temperature DMSs remains an active quest spanning a wide class of materials(e.g.,III-Vs,II-VIs, oxides,half-Heusler alloys).4The purpose of this paper is to extend the search for room-temperature DMSs to a relatively unexplored class of materials,the layered transition-metal dichalcogenides (TMDs).These materials have been the focus of much recent attention as they can be readily exfoliated to yield atomically thin layers for nanoelectronics,much like graphene. Notably,unlike graphene,several of these layered TMDs are semiconducting,6–8which makes them serious candidates for digital electronics.Recent demonstrations of MoS2de-vices such asfield-effect transistors,9,10logic circuits,11and phototransistors12are already promising.With respect to mag-netic properties,there have been recent experimental reports of magnetism in MoS2nanosheets,attributed to the presence of magnetic edge states;13irradiated MoS2,attributed to a combination of point defects and edge states;14and in MoS2 single crystals,attributed to zigzag edges at grain boundaries.15 Theoretical calculations also provide evidence for magnetic ordering at edges of nanoribbons16,17and nanoflakes,18as well as defect and dopant-induced magnetism.19We are unaware of any systematic studies of magnetism in layered TMDs via substitutional doping of magnetic transition-metal atoms, which is the focus of this work.In the following,we explore the effect of substitutional Mn doping in MoS2monolayers—in analogy with the commonly-used strategy in III-V and II-VI DMSs—and examine the potential for development of MoS2-based DMSs.To this end,we employfirst-principles density functional theory (DFT)calculations tofirst understand the electronic origins of ferromagnetic interactions between substitutional Mn dopant atoms and,thereafter,to parametrize a Monte Carlo(MC) model,which we employ for temperature-dependent studies of magnetic ordering in Mn-doped MoS2monolayers.We demonstrate that exchange interactions in Mn/MoS2DMSs are primarily governed by the double-exchange mechanism and are relatively short ranged,making percolation a key factor in magnetic ordering.Based on our DFT-parameterized MC simulations,we suggest that dopant concentrations in the range of10–15%might be sufficient to provide room-temperature ferromagnetism in Mn/MoS2DMSs,paving the way for experimental verification and application in spintronic devices.II.RESULTS AND DISCUSSIONA.Electronic structure calculationsFirst-principles calculations were performed using the Vienna ab initio package(V ASP)20at two different levels of theory:standard Kohn-Sham DFT with the Perdew-Burke-Ernzerhof(PBE)exchange-correlation(XC)functional21and hybrid DFT using the Heyd-Scuseria-Ernzerhof(HSE)ex-change correlation functional.22A detailed description of the DFT calculations is provided in the Appendix.Semilocal XC functionals,such as PBE,are known to suffer from self-interaction errors,which lead to excessive delocalization of the electronic wave functions.Such artifacts become particularly apparent when treating the d electrons of Mn and Mo as the occupied d states appear at excessively high energies, altering both the precise mechanism as well as the range of exchange interactions.Various strategies have been adopted in the literature to mitigate these self-interaction errors in DMSs; we refer the reader to the review in Ref.4and the referencesASHWIN RAMASUBRAMANIAM AND DORON NA VEH PHYSICAL REVIEW B87,195201(2013)therein.Here,we have chosen to employ the HSE functional,which reduces the self-interaction error by incorporating afraction of exact exchange,leading to a better descriptionof the electronic wave functions.23For monolayer MoS2,in particular,the fundamental gap from HSE calculationsappears to approximate the optical gap of the material.7,24In the following,we will compare and contrast the electronicstructure of Mn dopants in monolayer MoS2using both thePBE and HSE functionals,and,furthermore,examine theinfluence of the electronic structure on the exchange couplingand Curie temperature of the resulting DMSs.Before examining interactions between multiple Mn dopantatoms,we considerfirst the electronic structure of a singlesubstitutional Mn atom in monolayer MoS2.Figures1(a)and1(b)display the spin density(ρ↑−ρ↓)for a single substitutional Mn atom in a4×4supercell of monolayerMoS2.The overall magnetic moment of the supercell is1μBcorresponding to the single excess d electron provided by theMn atom.From the bond lengths listed in Fig.1(b),it is clearthat there is a loss of D3h(trigonal prism)symmetry at theMn dopant site.25A significant portion of the spin density islocalized on the Mn atom.The neighboring S atoms(labeledS1and S2)are antiferromagnetically coupled to the Mn dopant;the p character of the spin-polarized orbitals of the S atoms isclearly visible.Out of the six Mo atoms that were originally thenearest neighbors of the dopant site,only the four closest Moatoms(labeled Mo2and Mo3)couple antiferromagneticallyto the Mn atom while the two most distant ones(labeled Mo1)couple ferromagnetically to the Mn atom.We attribute this difference in magnetic coupling to the loss of trigonal symmetry at the Mn dopant site upon atomic relaxation.While the general features noted thus far are similar in both the PBE and HSE cases,there are distinct differences,the most obvious being the extent of spin polarization in the vicinity of the Mn dopant.Specifically,by projecting the spin density onto atomic orbitals and integrating over the PAW sphere,we obtain a local magnetic moment of1.04μB and2.77μB on the Mn atom at the PBE and HSE levels,respectively.This suggests that the Mn(IV)atom adopts a low-spin d3configuration at the PBE level,while the HSE functional prefers a high-spin d3configuration,which explains the greater extent of spin polarization in the immediate vicinity of the Mn atom in the latter case.Additional insight into the electronic structure of the Mn-doped MoS2monolayer can be obtained from the electronic density of states(DOS)displayed in Figs.2(a)and2(b). Within ligand-field theory,the trigonal prismatic coordination of the Mo atom lifts the degeneracy of the Mo4d levels. The lowest-energy band is of Mo4d z2character and is fully occupied;next in energy are degenerate,unoccupied Mo4d xy and Mo4d x2−y2bands,followed by the degenerate Mo4d zx and Mo4d yz bands of highest energy.6,26Experiments and first-principles calculations,suggest a more nuanced picture wherein hybridization occurs between the Mo4d z2,d xy, d x2−y2,and S3p orbitals;these hybridized states dominate the conduction and valence band edges of MoS2.6,27–32TheFIG.1.(Color online)(a),(b)Spin density(ρ↑−ρ↓)for a single Mn dopant atom in a4×4monolayer MoS2supercell(6.25%Mn doping)and(c),(d)for twofirst-nearest-neighbor Mn dopants in the same supercell(12.5%Mn doping;ferromagnetic ground state).Yellow and cyan isosurfaces represent positive and negative spin densities(±0.054e/˚A3),respectively.At6.25%doping,the dopant Mn atom has a local magnetic moment of1.04μB and2.77μB at the PBE and HSE levels,respectively.At12.5%doping,the average local moments of the Mn atoms are1.32μB and2.86μB at the PBE and HSE levels,respectively.The S atoms that are bonded to the Mn atom,as well as several of the Mo atoms in the immediate vicinity of the Mn atom,display antiferromagnetic coupling to the dopant.Mn-DOPED MONOLAYER MoS2:AN ATOMICALLY...PHYSICAL REVIEW B87,195201(2013)FIG.2.(Color online)Density of states(DOS)for(a),(b)6.25%Mn-doped and(c),(d)12.5%Mn-doped monolayer MoS2calculated using PBE and HSE functionals.The Fermi level of the doped monolayer is set as the zero of the energy scale.The semicore4p states of the undoped and doped monolayers(∼35eV below the Fermi level)are aligned to clearly show the emergence of gap states in the doped monolayer.At the HSE level the monolayer remains semiconducting in both spin channels for both dopant concentrations.At the PBE level, the monolayer becomes half-metallic at12.5%Mn doping.fundamental band gap of the monolayer is 1.6eV with the PBE and 2.05eV with the HSE functional.7Upon substituting an Mo(IV)d2atom by an Mn(IV)d3atom,the degeneracy of the spin channels is broken and defect levels are formed within the MoS2band gap(Fig.2).An analysis of the atom-projected DOS,displayed in the Supplementary Material,33reveals that the primary contributions to these gap states arise from the4d z2,4d xy,and4d x2−y2states of the Mn atom and its neighboring spin-polarized Mo atoms, as well as the3p states of the spin-polarized S atoms. The PBE DOS shows a negligible gap in the majority spin channel while the minority spin channel continues to display an appreciable gap,indicating that the doped monolayer is essentially half-metallic,while the DOS obtained by HSE features a clear gap in both spin channels—the majority-spin gap being smaller—suggesting that the doped monolayer is a magnetic semiconductor.We consider next the interaction of two Mn dopant atoms in monolayer MoS2(4×4supercell;12.5%doping).For brevity,we only discuss the case of Mn dopants infirst-nearest-neighbor substitutional sites;the picture is qualita-tively the same for second-and third-nearest-neighbor cases. Figures1(c)and1(d)display the spin densities at the PBE and HSE levels.By projecting the spin density onto PAW spheres,we obtain average local moments of1.32μB and 2.86μB on the Mn atoms at the PBE and HSE levels, respectively,indicating that the Mn dopants once again adopt low-spin d3and high-spin d3configurations depending upon the level of theory employed.The corresponding density of states are displayed in Figs.2(c)and2(d);atom-projected DOS are displayed in the Supplementary Material.33Upon comparing the PBE results for6.25%and12.5%Mn doping, we observe that the doped monolayer is unambiguously half-metallic in the latter case.The three peaks straddlingASHWIN RAMASUBRAMANIAM AND DORON NA VEH PHYSICAL REVIEW B87,195201(2013) the Fermi level in the6.25%Mn case merge into a singlebroad peak in the12.5%Mn case.This places the Fermilevel within the partially occupied majority band of theimpurities occupying only the bonding states while leaving theantibonding minority states unoccupied,which is suggestiveof an operative double-exchange mechanism.4In the HSEcalculations,both spin channels remain semiconducting andthe Fermi level remains within the band gap.The impurity dstates are still contained within the gap of the host material,which would again suggest that double exchange ought todominate the exchange coupling.However,the inclusion of afraction of exact exchange in the HSE functional lowers theenergy of the occupied d levels,analogous to previous reports4on Mn-doped III-Vs that employ some form of self-interactioncorrection(e.g.,the DFT+U approach,34–36SIC-LSD,37,38etc.).This would imply a decrease in the strength of thecomputed exchange coupling constants at the HSE levelrelative to the PBE situation.As we will show later,thisis also manifested in lower Curie temperatures when usingHSE-parameterized exchange coupling coefficients relative tothe PBE ones.To estimate the strength of exchange coupling,we reportin Table I the energy differences between the ferromag-netic ground state and the metastable antiferromagnetic state( AF M−F M)for two Mn atoms placed atfirst,second,andthird nearest-neighbor Mo sites.These are the only uniqueneighbor arrangements in a4×4supercell.At the PBE level,we also report energy differences forfirst-nearest-neighborMn dopants in larger supercells;HSE calculations were notperformed for these additional cases due to the enormouscomputational cost.From the presented data,it is clear thatthe Mn dopant atoms preferentially display ferromagneticcoupling at both the PBE and HSE level.It is also clearthat the HSE functional predicts stronger but shorter-rangedexchange interactions relative to PBE,which is to be expectedbased on the electronic DOS presented previously.For thevarious nearest-neighbor configurations studied here,we alsoreport in Table I the relative energy differences between theferromagnetic ground states( E F M).From these data,we seethat thefirst-nearest-neighbor configuration of Mn dopantsis energetically lower by0.3–0.7eV(depending upon thelevel of theory)than the second-or third-nearest-neighborTABLE I.Energy differences( AF M−F M)between the ferromag-netic ground state and the antiferromagnetic high-energy metastablestate for two Mn dopants placed at identical substitutional sites in theMoS2monolayer.Also displayed are energies of the ferromagneticground state for different spatial arrangements of Mn atoms(m th-nearest-neighbor)relative to thefirst-nearest-neighbor configuration( E F M=E m th−nnF M −E1st−nnF M).AF M−F M(eV) E F M(eV)Supercell Configuration PBE HSE PBE HSE 4×41st n.n.0.180.220.00.02nd n.n.0.060.070.370.663rd n.n0.03−0.000.430.65 6×61st n.n.0.178×81st n.n.0.17cases,which suggests a strong thermodynamic driving force for clustering of dopant atoms.While this result would suggest the need for kinetically trapping Mn dopant atoms to produce a uniform,dilute distribution of magnetic impurities,the ability to produce ferromagnetic Mn clusters in the host MoS2lattice might also be technologically useful.B.Monte Carlo simulationsIt is well known that ordering in DMSs is strongly influ-enced by percolation;the mean-field approximation cannot capture this behavior and tends to systematically overestimate the Curie temperature in these systems.4,36,39–41Therefore,to allow for a proper description of spatial disorder and magnetic percolation in the Mn/MoS2DMS,we parameterized the first-principles exchange interactions between Mn atoms and incorporated these within a Monte Carlo model.The exchange coupling coefficient J(r)is parameterized using the functional formJ(r)=cr3exp[−r/r0],if r r c0,otherwise,(1)where r is the distance between two impurities,r0is the screening length,r c is the cutoff in the interaction range,and c is a constant of proportionality.42The cutoff length was set to the radius of the tenth nearest-neighbor shell(14.48˚A). The remaining parameters were obtained byfitting the energy differences AF M−F M to the model in Eq.(1).The parameters obtained from thefits to the PBE data are c=5.965eV/˚A3 and r0=25.957˚A.The HSE data,while more limited than the PBE set,yield bestfit parameters of c=12.971eV/˚A3and r0=4.944˚A.The exchange coupling energies that result from these parametrizations are displayed in Fig.3(a),the discrete points representing each neighbor shell up through the cutoff distance.As expected from the data in Table I,the HSE cou-pling is stronger atfirst-nearest-neighbor separation but drops off more rapidly than its PBE counterpart.It is worth noting that there are certainly more sophisticated techniques to extract exchange coupling coefficients based on linear response,43 frozen magnons,44etc.Such approaches are beyond the scope of the present work and will be considered elsewhere.For now, the total-energy approach adopted here is sufficient to bring out the principal features of magnetic interactions in DMSs and has adequate precedent in the literature.35,41With the exchange coupling coefficients in hand,it is straightforward to set up a Metropolis Monte Carlo(MC) calculation45to simulate the role of disorder and percolation in Mn/MoS2DMSs.Briefly,the entire problem was mapped to a Heisenberg model on a triangular lattice,i.e.,the underlying lattice formed by the Mo sites.46We examined system sizes ranging from20×20to100×100containing dopant concen-trations ranging from5%to15%.Configurational disorder was simulated using40different random initial conditions,and all thermodynamic properties were calculated by averaging over these distinct runs.Two procedures were used to estimate the Curie temperature(T C).In the absence of an external magnetic field,the magnetic susceptibility(χ=[ M2 − |M| 2]/k B T) diverges at the critical temperature in the thermodynamic limit. On afinite lattice the susceptibility displays a broadened peak; we use the position of this peak from the largest simulatedMn-DOPED MONOLAYER MoS2:AN ATOMICALLY...PHYSICAL REVIEW B87,195201(2013)FIG.3.(Color online)(a)Exchange coupling coefficient obtained from the model in Eq.(1).Symbols correspond to each neighbor shell up to the tenth-nearest neighbor.The HSE exchange coupling is stronger atfirst-nearest-neighbor separation but drops off more rapidly than its PBE counterpart with increasing distance,which leads to lower Curie temperatures(T C)in the range of5–12.5%doping as seen in(b).At sufficiently high concentrations,the stronger nearest-neighbor interaction at the HSE level begins to dominate and leads to higher values of T C than the PBE-based estimates.lattice as one estimate of the Curie temperature.The secondestimate is obtained from the Binder cumulant method.47Binder’s cumulant,defined asU4=1−m43 m2 2,(2)is only weakly dependent on system size and the common point of intersection of the U4versus temperature curves for various system sizes furnishes an estimate of T C.For our DMSs,we find that the two estimates for T C are in poor agreement at low dopant concentration,most likely due to lack of percolation in the lattice.At higher concentrations( 10%for PBE; 13% for HSE),the two estimates come into better agreement. Here,we choose to consistently use the susceptibility data for estimating T C.In Fig.3(b),we display estimates for T C as a function of dopant concentration using both the PBE and HSE parameterized exchange coupling.As seen from Fig.3(b),the HSE predictions of T C are consistently—and often significantly—lower than their PBE counterparts.This is essentially a manifestation of the shorter range of HSE exchange interactions as alluded to before.At a fundamental level,these significant differences underscore the need for functionals that can describe exchange and correlation effects more accurately.We see a sharp increase in T C beyond10% and13%Mn doping at the PBE and HSE levels,respectively, which is most likely indicative of the onset of percolation.The eventual increase in the HSE estimate for T C as compared to the PBE estimate at15%doping is due to the stronger nearest-neighbor exchange coupling at the HSE level.Collectively, these results point towards the distinct possibility of achieving room-temperature ferromagnetism in MoS2monolayers for Mn doping in the range of10–15%.III.CONCLUSIONSIn summary,we conducted a combined DFT and Monte Carlo study of ferromagnetic ordering in Mn-doped monolayer MoS2.Our DFT studies show that the electronic structure of the resulting DMSs,as well as the strength and range of exchange interactions,are quite sensitive to the level of theory employed.This is most clearly manifested in the lower Curie temperatures obtained with the hybrid HSE XC functional,which corrects for some of the self-interaction error in semilocal functionals through the mixing of a fraction of exact exchange.Wefind that exchange interactions in Mn/MoS2DMSs are primarily governed by the double-exchange mechanism and are relatively short-ranged,making percolation a key factor for magnetic ordering.Based on our DFT-parameterized MC simulations,we predict that dopant concentrations in the range of10–15%ought to lead to room-temperature ferromagnetism in Mn/MoS2DMSs.It remains to be seen whether these predictions can be realized experimentally.At the very least,previous experiments have demonstrated the ability to dope MoS2films,nanoparticles, and nanotubes with transition metals such as Re,48Ti,49Cr,50 and Mn.51Our theoretical predictions will hopefully motivate additional investigations along similar lines with the aim of tailoring the magnetic properties of doped few-layer MoS2for novel electronic applications.APPENDIX:COMPUTATIONAL METHODS Allfirst-principles calculations were performed using the Vienna ab initio simulation package(V ASP).20The projector-augmented wave(PAW)method52,53was used to represent the nuclei plus core electrons.Electron exchange and correlation was treated using both the Perdew-Burke-Ernzerhof(PBE)21 parametrization of the generalized-gradient approximation as well as the Heyd-Scuseria-Ernzerhof(HSE)22hybrid func-tional.From convergence tests,the kinetic energy cutoff was set at400eV;the Brillouin zones for4×4supercells were sampled with a2×2×1 -centered k-point mesh,whereas a single point was used for larger supercells.A Gaussian smearing of0.05eV was employed in conjunction with an energy tolerance of10−4eV for electronic relaxation.The cell vectors werefixed at the equilibrium value for the MoS2ASHWIN RAMASUBRAMANIAM AND DORON NA VEH PHYSICAL REVIEW B87,195201(2013)monolayer and atomic positions relaxed with a tolerance of 0.01eV/˚A.Periodic images were separated by at least10˚A of vacuum normal to the monolayer to eliminate spurious interlayer coupling.*ashwin@†doron.naveh@biu.ac.il1S.A.Wolf,D.D.Awschalom,R.A.Buhrman,J.M.Daughton, S.von Mol´n ar,M.L.Roukes,A.Y.Chtchelkanova,and D.M. 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a rX iv:082.1740v1[c ond-mat.ot her]12Feb28Temperature dependent magnetization dynamics of magnetic nanoparticles A.Sukhov 1,2and J.Berakdar 21Max-Planck-Institut f¨u r Mikrostrukturphysik,Weinberg 2,D-06120Halle/Saale,Germany 2Institut f¨u r Physik,Martin-Luther-Universit¨a t Halle-Wittenberg,Heinrich-Damerow-Str.4,06120Halle,Germany Abstract.Recent experimental and theoretical studies show that the switching behavior of magnetic nanoparticles can be well controlled by external time-dependent magnetic fields.In this work,we inspect theoretically the influence of the temperature and the magnetic anisotropy on the spin-dynamics and the switching properties of single domain magnetic nanoparticles (Stoner-particles).Our theoretical tools are the Landau-Lifshitz-Gilbert equation extended as to deal with finite temperatures within a Langevine framework.Physical quantities of interest are the minimum field amplitudes required for switching and the corresponding reversal times of the nanoparticle’s magnetic moment.In particular,we contrast the cases of static and time-dependent external fields and analyze the influence of damping for a uniaxial and a cubic anisotropy.PACS numbers:75.40.Mg,75.50.Bb,75.40.Gb,75.60.Jk,75.75.+a1.IntroductionIn recent years,there has been a surge of research activities focused on the spin dynamics and the switching behavior of magnetic nanoparticles[1].These studies are driven by potential applications in mass-storage media and fast magneto-electronic devices. In principle,various techniques are currently available for controlling or reversing the magnetization of a nanoparticle.To name but a few,the magnetization can be reversed by a short laser pulse[2],a spin-polarized electric current[3,4]or an alternating magneticfield[5,6,7,8,9,10,11,12,13].Recently[6],it has been shown for a uniaxial anisotropy that the utilization of a weak time-dependent magneticfield achievesa magnetization reversal faster than in the case of a static magneticfield.For this case[6],however,the influence of the temperature and the different types of anisotropy on the various dependencies of the reversal process have not been addressed.These issues,which are the topic of this present work,are of great importance since,e.g. thermal activation affects decisively the stability of the magnetization,in particular when approaching the superparamagnetic limit,which restricts the density of data storage[14].Here we study the possibility of fast switching atfinite temperature with weak externalfields.We consider magnetic nanoparticles with an appropriate size as to display a long-range magnetic order and to be in a single domain remanent state(Stoner-particles).Uniaxial and cubic anisotropies are considered and shown to decisively influence the switching dynamics.Numerical results are presented and analyzed for iron-platinum nanoparticles.In principle,the inclusion offinite temperatures in spin-dynamics studies is well-established(cf.[19,20,23,15,16,1]and references therein) and will be followed here by treatingfinite temperatures on the level of Langevine dynamics.For the analysis of switching behaviour the Stoner and Wohlfarth model (SW)[17]is often employed.SW investigated the energetically metastable and stable position of the magnetization of a single domain particle with uniaxial anisotropy in the presence of an external magneticfield.They showed that the minimum static magneticfield(generally referred to as the Stoner-Wohlfarth(SW)field or limit)needed to coherently reverse the magnetization is dependent on the direction of the applied field with respect to the easy axis.This dependence is described by the so-called Stoner-Wohlfarth astroid.The SWfindings rely,however,on a static model at zero temperature.Application of a time-dependent magneticfield reduces the required minimum switchingfield amplitude below the SW limit[6].It was,however,not yet clear howfinite temperatures will affect thesefindings.To clarify this point,we utilize an extension of the Landau-Lifshitz-Gilbert equation[18]includingfinite temperatures on the level of Langevine dynamics[19,20,23].Our analysis shows the reversal time to be strongly dependent on the damping,the temperature and the type of anisotropy. These dependencies are also exhibited to a lesser extent by the critical reversalfields. The paper is organized as follows:next section2presents details of the numerical scheme and the notations whereas section3shows numerical results and analysis for Fe50Pt50 and Fe70Pt30nanoparticles.We then conclude with a brief summary.2.Theoretical modelIn what follows we focus on systems with large spins such that their magnetic dynamics can be described by the classical motion of a unit vector S directed along the particle’s magnetizationµ,i.e.S=µ/µS andµS is the particle’s magnetic moment at saturation. The energetics of the system is given byH=H A+H F.(1) where H A(H F)stands for the anisotropy(Zeeman energy)contribution.Furthermore, the anisotropy contribution is expressed as H A=−Df(S)with D being the anisotropy constant.Explicit form of f(S)is provided below.The magnetization dynamics,i.e.the equation of motion for S,is governed by the Landau-Lifshitz-Gilbert(LLG)equation [18]∂S(1+α2)S× B e(t)+α(S×B e(t)) .(2) Here we introduced the effectivefield B e(t)=−1/(µS)∂H/∂S which contains the external magneticfield and the maximum anisotropyfield for the uniaxial anisotropy B A=2D/µS.γis the gyromagnetic ratio andαis the Gilbert damping parameter.The temperaturefluctuations will be described on the level of the Langevine dynamics[19]. This means,a time-dependent thermal noiseζ(t)adds to the effectivefield B e(t)[19].ζ(t)is a Gaussian distributed white noise with zero mean and vanishing time correlator ζi(t′)ζj(t) =2αk B TB A,τ=ωa t,ωa=γB A.(4) The LLG equation reads then∂S(1+α2)S× b(τ)+α(S×b(τ)) ,(5) where the effectivefield is now given explicitly byb(τ)=−1∂S+Θ(τ)(6)withΘi(τ′)Θj(τ) =ǫδi,jδ(τ−τ′);ǫ=2αk B TD.(8) q is a measure for the thermal energy in terms of the anisotropy energy.And d=D/(µS B A)expresses the anisotropy constant in units of a maximum anisotropyenergy for the uniaxial anisotropy and is always1/2.The stochastic LLG equation(5) in reduced units(4)is solved numerically using the Heun method which converges in quadratic mean to the solution of the LLG equation when interpreted in the sense of Stratonovich[20].For each type of anisotropy we choose the time step∆τto be one thousandth part of the corresponding period of oscillations.The values of the time interval in not reduced units for uniaxial and cubic anisotropies are∆t ua=4.61·10−15s and∆t ca=64.90·10−15s,respectively,providing us thus with correlation times on the femtosecond time scale.The reason for the choice of such small time intervals is given in [19],where it is argued that the spectrum of thermal-agitation forces may be considered as white up to a frequency of order k B T/h with h being the Planck constant.This value corresponds to10−13s for room temperature.The total scale of time is limited by a thousand of such periods.Hence,we deal with around one million iteration steps for a switching process.Details of realization of this numerical scheme could be found in references[21,22,20].We note by passing,that attempts have been made to obtain, under certain limitations,analytical results forfinite-temperature spin dynamics using the Fokker-Planck equation(cf.[15,16]and references therein).For the general case discussed here one has however to resort to fully numerical approaches.3.Results and interpretationsWe consider a magnetic nanoparticle in a single domain remanent state(Stoner-particle) with an effective anisotropy whose origin can be magnetocrystalline,magnetoelastic and surface anisotropy.We assume the nanoparticle to have a spherical form,neglecting thus the shape anisotropy contributions.In the absence of externalfields,thermal fluctuations may still drive the system out of equilibrium.Hence,the stability of the system as the temperature increases becomes an important issue.The time t at which the magnetization of the system overcomes the energy barrier due to the thermal activation,also called the escape time,is given by the Arrhenius lawt=t0e DπµS k B TαγThe relation between K u and D u is D u=K u V u,where V u is the volume of Fe50Pt50nanoparticles.In the calculations for Fe50Pt50nanoparticles the following q valueswere chosen:q1=0.001,q2=0.005or q3=0.01which correspond to the realtemperatures56K,280K or560K,respectively(these temperatures are below theblocking temperature).The corresponding escape times are t q1≈2·10217s,t q2≈1075s and t q3≈7·1031s,respectively.In some cases we also show the results for an additional temperature q01=0.0001with the corresponding real temperature to be equal to5K.The corresponding escape time for this is t q01≈104300s.These times should be compared with the measurement period which is about t m≈5ns,endorsing thus the stability ofthe system during the measurements.For Fe70Pt30the parameters are as follows:The diameter of the nanoparticles2.3nm, the strength of the anisotropy K c=8·105J/m3,the magnetic moment per particle µp=2000·µB,the Curie-temperature is T c=420K[24],and D c=K c V c(V c is the volume.)For Fe70Pt30nanoparticles the values of q we choose in the simulations are q4=0.01,q5=0.03or q6=0.06which means that the temperature is respectively 0.3K,0.9K or1.9K.The escape times are t q4≈1034s,t q5≈2·105s and t q6≈2·10−2s, respectively.Here we also choose an intermediate value q04=0.001and the realtemperature0.03K with the corresponding escape time to be equal to t q04≈10430s. The measurement period is the same,namely about5ns.All values of the escape timeswere given forα=0.1.Central to this study are two issues:The critical magneticfield and the corresponding reversal time.The critical magneticfield we define as the minimumfield amplitude needed to completely reverse the magnetization.The reversal time is the corresponding time for this process.In contrast,in other studies[6]the reversal time is defined as the time needed for the magnetization to switch from the initial position to the position S z=0,our reversal time is the time at which the magnetization reaches the very proximity of the antiparallel state(Fig.1).The difference in the definition is in so far important as the magnetization position S z=0atfinite temperatures is not stabile so it may switch back to the initial state due to thermalfluctuations and hence the target state is never reached.3.1.Nanoparticles having uniaxial anisotropy:Fe50Pt50A Fe50Pt50magnetic nanoparticle has a uniaxial anisotropy whose direction defines the z direction.The magnetization direction S is specified by the azimuthal angleφand the polar angleθwith respect to z.In the presence of an externalfield b applied at an arbitrarily chosen direction,the energy of the system in dimensionless units derives from˜H=−d cos2θ−S·b.(11) The initial state of the magnetization is chosen to be close to S z=+1and we aim at the target state S z=−1.Figure1.(Color online)Magnetization reversal of a nanoparticle when a staticfieldis applied at zero Kelvin(q0=0,black)and at reduced temperature q3=0.01≡560K(blue).The strengths of thefields in the dimensionless units(4)and(8)are b=1.01and b=0.74,respectively.The damping parameter isα=0.1.The start position ofthe magnetization is given by the initial angleθ0=π/360between the easy axis andthe magnetization vector.3.1.1.Staticfield For an external static magneticfield applied antiparallel to the z direction(b=−b e z)eq.(11)becomes˜H=−d cos2θ+b cosθ.(12) To determine the criticalfield magnitude needed for the magnetization reversal we proceed as follows(cf.Fig.1):Atfirst,the externalfield is increased in small steps. When the magnetization reversal is achieved the corresponding values of the critical field versus the damping parameterαare plotted as shown in the inset of Fig.3.The reversal times corresponding to the critical staticfield amplitudes of Fig.3are plotted versus damping in Fig.4.In the Stoner-Wohlfarth(static)model the mechanism of magnetization reversal is not due to damping.It is rather caused by a change of the energy profile in the presence of thefield.The curves displayed on the energy surface in Fig.2mark the magnetization motion in the E(θ,φ)landscape.The magnetization initiates fromφ0=0andθ0and ends up atθ=π.As clearly can be seen from thefigure,reversal is only possible if the initial state is energetically higher than the target state.This”low damping”reversal is,however,quite slow,which will be quantified more below.For the reversal at T=0, the SW-model predicts a minimum staticfield strength,namely b cr=B/B A=1(the dashed line in Fig.3).This minimumfield measured with respect to the anisotropyfield strength does not depend on the damping parameterα,provided the measuring time is infinite.For T>0 the simulations were averaged over500cycles with the result shown in Fig.3.The one-cycle data are shown in the inset.Fig.3evidences that with increasing temperature thermalfluctuations assist a weak magneticfield as to reverse the magnetization. Furthermore,the required criticalfield is increased slightly at very large and strongly at very small damping with the minimum criticalfield being atα≈1.0.The reason forthe magnetization starts atθ0=0(the vector product in equation(2)vanishes).The reversal time in the SW-limit is then given byt rev=g(θ0,b)1+α22γD 1b−cosθ πθ0.(14)From this relation we infer that switching is possible only if the appliedfield is larger than the anisotropyfield and the reversal time decreases with increasing b.This conclusion is independent of the Stoner-Wohlfarth model and follows directly from the solution of the LLG equation.An illustration is shown by the dashed curve in Fig.4,which was a test to compare the appropriate numerical results with the analytical one.As our aim is the study of the reversal-time dependence on the magnetic moment and on the anisotropy constant,we deem the logarithmic dependence in Eq.(14)to be weak and writeg(b,µS,D)≈µSB2µ2S−4D2.(15)This relation indicates that an increase in the magnetic moment results in a decreaseof the reversal time.The magnetic moment enters in the Zeeman energy and thereforethe increase in magnetic moment is very similar to an increase in the magneticfield.An increase of the reversal time with the increasing anisotropy originates from the factthat the anisotropy constant determines the height of the potential barrier.Hence,thehigher the barrier,the longer it takes for the magnetization to overcome it.For the other temperatures the corresponding reversal times(also averaged over500cycles)are shown in Fig. 4.In contrast to the case T=0,where an appreciabledependence on damping is observed,the reversal times forfinite temperatures showa weaker dependence on damping.Ifα→0only the precessional motion of themagnetization is possible and therefore t rev→∞.At high damping the system relaxes on a time scale that is much shorter than the precession time,giving thus rise to anincrease in switching times.Additionally,one can clearly observe the increase of thereversal times with increasing temperatures,even though these time remain on thenanoseconds time scale.3.1.2.Alternatingfield As was shown in Ref.[6,7,15]theoretically and in Ref.[5] experimentally,a rotating alternatingfield with no staticfield being applied can also be used for the magnetization reversal.A circular polarized microwavefield is applied perpendicularly to the anisotropy axis.Thus,the Hamiltonian might be written in form of equation(11)and the appliedfield isb(t)=b0cosωt e x+b0sinωt e y,(16) where b0is the alternatingfield amplitude andωis its frequency.For a switching of the magnetization the appropriate frequency of the applied alternatingfield should beFigure4.(Color online)Reversal times corresponding to the critical staticfields inFig.3vs.damping averaged over500cycles.Inset shows the as-calculated numericalresults for q3=0.01≡560K(one cycle).Figure 5.(Color online)Magnetization reversal in a nanoparticle using a timedependentfield forα=0.1and at a zero temperature.Thefield strength and frequencyin the units(4)are respectively b0=0.18andω=ωa/1.93.Inset shows for this casethe magnetization reversal for the temperature q3=0.01≡560K with b0=0.17andthe same frequency.chosen.In Ref.[15]analytically and in[6]numerically a detailed analysis of the optimal frequency is given which is close to the precessional frequency of the system.The role of temperature and different types of anisotropy have not yet been addressed,to our knowledge.Fig.5shows our calculations for the reversal process at two different temperatures. In contrast to the static case,the reversal proceeds through many oscillations on a time scale of approximately ten picoseconds.Increasing the temperature results in an increase of the reversal time.Fig.6shows the trajectory of the magnetization in the E(θ,φ)space related to the case of the alternatingfield pared with the situation depicted in Fig. 2,the trajectory reveals a quite delicate motion of the magnetization.It is furthermore, noteworthy that the alternatingfield amplitudes needed for the reversal(cf.Fig.7)are substantially lower than their static counterpart,meaning that the energy profile of the.(17)αThe proportionality coefficient contains the frequency of the alternatingfield and the critical angleθ.The solution(17)follows from the LLG equation solved for the case when the phase of the externalfield follows temporally that of the magnetization,which we checked numerically to be valid.The reversal times associated with the critical switchingfields are shown in(Fig.8).Qualitatively,we observe the same behavior as for the case of a staticfield.The values of the reversal times for T=0are,however,significantly smaller than for the static case.For the same reason as in the staticfield case,an increased temperature results in an increase of the switching times.Figure7.(Color online)Critical alternatingfield amplitudes vs.damping fordifferent temperatures averaged over500times.Inset shows not averaged data for.q3=0.01≡560Kto the criticalfield amplitudes of Fig.7for different temperatures.Inset shows thecase of zero Kelvin.3.2.Nanoparticles with cubic anisotropy:Fe70Pt30Now we focus on another type of the anisotropy,namely a cubic anisotropy which is supposed to be present for Fe70Pt30nanoparticles[24].The energetics of the system is then described by the functional form˜H=−d(S2x S2y+S2y S2z+S2x S2z)−S·b,(18) or in spherical coordinates˜H=−d(cos2φsin2φsin4θ+cos2θsin2θ)−S·b.(19) In contrast to the previous section,there are more local minima or in other words more stable states of the magnetization in the energy profile for the Fe70Pt30nanoparticles. It can be shown that the minimum barrier that has to be overcome is d/12which is twelve times smaller than that in the case of a uniaxial anisotropy.The maximal one is only d/3.The magnetization of these nanoparticles isfirst relaxed to the initial state close toFigure9.(Color online)Trajectories of the magnetization in theθ(φ)space(q0=0).In the units(4)we choose b=0.82andα=0.1.√φ0=π/4andθ0=arccos(1/3).In order to be close to the starting state for the uniaxial anisotropy case we chooseφ0=0.2499·π,θ0=0.3042·π.3.2.1.Static drivingfield A staticfield is applied antiparallel to the initial state of the magnetization,i.e.√b=−b/B A.3In principle,the criticalfield turns out to be constant for allαbut for an infinitely large measuring time.Since we set this time to be about5nanoseconds,the criticalfields increase for small and high damping.On the other hand,at lower temperatures smaller criticalfields are sufficient for the(thermal activation-assisted)reversal process.The behaviour of the corresponding switching times presented in Fig.12only supplements the fact of too low measuring time,which is chosen as5ns for a better comparison of these results with ones for uniaxial anisotropy.Indeed,constant jumps in the reversal times for T=0K as a function of damping can be observed.The reasonFigure10.(Color online)Magnetization reversal of a nanoparticle when a staticfieldb=0.82is applied and forα=0.1at zero temperature(black).The magnetizationreversal forα=0.1,b=0.22and q6=0.06≡1.9K is shown with blue color.Figure11.(Color online)Critical staticfield amplitudes vs.the damping parametersfor different temperatures averaged over500times.Inset shows not averaged data forq6=0.06≡1.9K.Fig.11vs.damping averaged over500times.why the reversal times forfinite temperatures are lower is as follows:The initial state for T=0K is chosen to be very close to equilibrium.This does not happen forfinite3).The magnetization trajectories depicted in Fig.13reveal two interesting features: Firstly,particularly for small damping,the energy profile changes very slightly(due to the smallness of b0)while energy is pumped into the system during many cycles. Secondly,the system switches mostly in the vicinity of local minima to acquire eventually the target state.Fig.14hints on the complex character of the magnetization dynamics in this case.As in the staticfield case with a cubic anisotropy the criticalfield amplitudes shown in Fig.15are smaller than those for a uniaxial anisotropy.Obviously, the reason is that the potential barrier associated with this anisotropy is smaller in this case,giving rise to smaller amplitudes.As before an increase in temperature leads to a decrease in the criticalfields.The reversal times shown in Fig.16exhibit the same feature as in the cases for uniaxial anisotropy:With increasing temperatures the corresponding reversal times increase.A physically convincing explanation of the(numerically stable)oscillations for the reversal times is still outstanding.Figure14.(Color online)Magnetization reversal in a nanoparticle using a time dependentfield forα=0.1and q0(black)and for q6=0.06≡1.9K(blue).Other parameters are as in Fig.13.Figure15.(Color online)Critical alternatingfield amplitudes vs.damping for different temperatures averaged over500cycles.Inset shows the single cycle data at q6=0.06≡1.9K.Figure16.(Color online)The damping dependence of the reversal times corresponding to the critical fields of the Fig.15for different temperatures averaged over500runs.Inset shows the T=0case. 4.SummaryIn this work we studied the criticalfield amplitudes required for the magnetization switching of Stoner nanoparticles and derived the corresponding reversal times forstatic and alternatingfields for two different types of anisotropies.The general trends for all examples discussed here can be summarized as follows:Firstly,increasing the temperature results in a decrease of all criticalfields regardless of the anisotropy type. Anisotropy effects decline with increasing temperatures making it easier to switch the magnetization.Secondly,elevating the temperature increases the corresponding reversal times.Thirdly,the same trends are observed for different temperatures:The criticalfield amplitudes for a staticfield depend only slightly onα,whereas the critical alternating field amplitudes exhibit a pronounced dependence on damping.In the case of a uniaxial anisotropy wefind the critical alternatingfield amplitudes to be smaller than those for a staticfield,especially in the low damping regime and forfinite pared with a staticfield,alternatingfields lead to smaller switching times(T=0K).However, this is not the case for the cubic anisotropy.The markedly different trajectories for the two kinds of anisotropies endorse the qualitatively different magnetization dynamics. In particular,one may see that for a cubic anisotropy and for an alternatingfield the magnetization reversal takes place through the local minima leading to smaller amplitudes of the appliedfield.Generally,a cubic anisotropy is smaller than the uniaxial one giving rise to smaller slope of criticalfields,i.e.smaller alternatingfield amplitudes. It is useful to contrast our results with those of Ref.[15].Our reversal times for AC-fields increase with increasing temperatures.This is not in contradiction with the findings of[15]insofar as we calculate the switchingfields atfirst,and then deduce the corresponding reversal times.If the switchingfields are kept constant while increasing the temperature[15]the corresponding reversal times decrease.We note here that experimentally known values of the damping parameter are,to our knowledge,not larger than0.2.The reason why we go beyond this value is twofold.Firstly,the values of damping are only well known for thin ferromagneticfilms and it is not clear how to extend them to magnetic nanoparticles.For instance,in FMR experiments damping values are obtained from the widths of the corresponding curves of absorption.The curves for nanoparticles can be broader due to randomly oriented easy anisotropy axes and,hence,the values of damping could be larger than they actually are.Secondly,due to a very strong dependence of the critical AC-fields(Fig.7,e.g.)they can even be larger than staticfield amplitudes.This makes the time-dependentfield disadvantageous for switching in an extreme high damping regime.Finally,as can be seen from all simulations,the corresponding reversal times are much more sensitive a quantity than their criticalfields.This follows from the expression(13), where a slight change in the magneticfield b leads to a sizable difference in the reversal time.This circumstance is the basis for our choice to average all the reversal times and fields over many times.This is also desirable in view of an experimental realization,for example,in FMR experiments or using a SQUID technique quantities like criticalfields and their reversal times are averaged over thousands of times.The results presented in this paper are of relevance to the heat-assisted magnetic recording,ing a laser source.Our calculations do not specify the source of thermal excitations but they capture the spin dynamics and switching behaviour of the system upon thermalexcitations.AcknowledgmentsThis work is supported by the International Max-Planck Research School for Science and Technology of Nanostructures.References[1]Spindynamics in confined magnetic structures III B.Hillebrands,A.Thiaville(Eds.)(Springer,Berlin,2006);Spin Dynamics in Confined Magnetic Structures II B.Hillebrands,K.Ounadjela (Eds.)(Springer,Berlin,2003);Spin dynamics in confined magnetic structures B.Hillebrands, K.Ounadjela(Eds.)(Springer,Berlin,2001);Magnetic Nanostructures B.Aktas,L.Tagirov,F.Mikailov(Eds.),(Springer Series in Materials Science,Vol.94)(Springer,2007)and references therein.[2]M.Vomir,L.H.F.Andrade,L.Guidoni,E.Beaurepaire,and J.-Y.Bigot,Phys.Rev.Lett.94,237601(2005).[3]J.Slonczewski,J.Magn.Magn.Mater.,159,L1,(1996).[4]L.Berger,Phys.Rev.B54,9353(1996).[5]C.Thirion,W.Wernsdorfer,and D.Mailly,Nat.Mater.2,524(2003).[6]Z.Z.Sun and X.R.Wang,Phys.Rev.B74,132401(2006).[7]Z.Z.Sun and X.R.Wang,Phys.Rev.Lett.97,077205(2006).[8]L.F.Zhang,C.Xu,Physics Letters A349,82-86(2006).[9]C.Xu,P.M.Hui,Y.Q.Ma,et al.,Solid State Communications134,625-629(2005).[10]T.Moriyama,R.Cao,J.Q.Xiao,et al.,Applied Physics Letters90,152503(2007).[11]H.K.Lee,Z.M.Yuan,Journal of Applied Physics101,033903(2007).[12]H.T.Nembach,P.M.Pimentel,S.J.Hermsdoerfer,et al.,Physics Letters90,062503(2007).[13]K.Rivkin,J.B.Ketterson,Applied Physics Letters89,252507(2006).[14]R.W.Chantrell and K.O’Grady The Magnetic Properties offine Particles in R.Gerber,C.D.Wright and G.Asti(Eds.),Applied Magnetism(Kluwer,Academic Pub.,Dordrecht,1994).[15]S.I.Denisov,T.V.Lyutyy,P.H¨a nggi,and K.N.Trohidou,Phys.Rev.B74,104406(2006).[16]S.I.Denisov,T.V.Lyutyy,and P.H¨a nggi,Phys.Rev.Lett.97,227202(2006).[17]E.C.Stoner and E.P.Wohlfarth,Philos.Trans.R.Soc.London,Ser A240,599(1948).[18]ndau and E.Lifshitz,Phys.Z.Sowjetunion8,153(1935).[19]W.F.Brown,Phys.Rev.130,1677(1963).[20]J.L.Garcia-Palacios and zaro,Phys.Rev.B58,14937(1998).[21]Algorithmen in der Quantentheorie und Statistischen Physik J.Schnakenberg(Zimmermann-Neufang,1995).[22]U.Nowak,p.Phys.9,105(2001).[23]adel,Phys.Rev.B73,212405(2006).[24]C.Antoniak,J.Lindner,and M.Farle,Europhys.Lett.70,250(2005).[25]I.Klik and L.Gunther,J.Stat.Phys.60,473(1990).[26]C.Antoniak,J.Lindner,M.Spasova,D.Sudfeld,M.Acet,and M.Farle,Phys.Rev.Lett.97,117201(2006).[27]S.Ostanin,S.S.A.Razee,J.B.Staunton,B.Ginatempo and E.Bruno,J.Appl.Phys.93,453(2003).。
a rX iv:c ond-ma t/997324v1[c ond-m at.stat-m ec h]21J u l1999Nonmonotonic external field dependence of the magnetization in a finite Ising model:theory and MC simulation X.S.Chen 1,2,a ,V.Dohm 2,b and D.Stauffer 3,c 1Institute of Particle Physics,Hua-Zhong Normal University,Wuhan 430079,P.R.China 2Institut f¨u r Theoretische Physik,Technische Hochschule Aachen,D-52056Aachen,Germany 3Institute for Theoretical Physics,Cologne University,D-50923K¨o ln,Germany Abstract Using ϕ4field theory and Monte Carlo (MC)simulation we in-vestigate the finite-size effects of the magnetization M for the three-dimensional Ising model in a finite cubic geometry with periodic bound-ary conditions.The field theory with infinite cutoffgives a scal-ing form of the equation of state h/M δ=f (hL βδ/ν,t/h 1/βδ)where t =(T −T c )/T c is the reduced temperature,h is the external field and L is the size of system.Below T c and at T c the theory predicts a nonmonotonic dependence of f (x,y )with respect to x ≡hL βδ/νat fixed y ≡t/h 1/βδand a crossover from nonmonotonic to monotonic behaviour when y is further increased.These results are confirmed by MC simulation.The scaling function f (x,y )obtained from the field theory is in good quantitative agreement with the finite-size MC data.Good agreement is also found for the bulk value f (∞,0)at T c .PACS:05.70.Jk,64.60.-i a e-mail:chen@physik.rwth-aachen.deb e-mail:vdohm@physik.rwth-aachen.dec e-mail:stauffer@thp.uni-koeln.de1IntroductionThe scaling equation of state near a critical point provides fundamental in-formation on the critical behaviour of a thermodynamic system.For bulk Ising-like systems accurate predictions have been made recently[1]on the basis of theϕ4field theory in three dimensions.Testing these predictions by Monte Carlo simulations[2]would be of considerable interest.Such simu-lations,however,are necessarily made only forfinite systems and thus phe-nomenological concepts likefinite-size scaling[3]are needed to perform ex-trapolations from mesoscopic lattices.In order to test the theory in a more conclusive way it is desirable to go be-yond the phenomenologicalfinite-size scaling concept and to calculate explic-itly thefinite-size effects on the equation of state,i.e.,on the magnetization as a function of the temperature T and externalfield h in afinite geometry. Although suchfield-theoretic calculations[4,5,6,7]are perturbative and not exact they have been found to be in good agreement with the MC simulations. So far the calculations of thermodynamic quantities were restricted to the case of zero externalfield h.Atfinite h,only the order-parameter distribu-tion function was calculated[8,9,10].In the present paper we extend these calculations to the equation of state of the three-dimensional Ising model in afinite cubic geometry atfinite h.For simplicity these calculations are performed at infinite cutoffand thus our results neglect lattice effects.The latter have been shown[11,12]to yield(exponentially small)non-universal non-scaling contributions.Here we focus our interest on the universal scal-ing part of the equation of state.Our theory predicts non-monotonic effects in the h dependence of the equation of state which we then confirm with surprisingly good agreement by standard Monte Carlo simulations.The identification of such non-monotonic effects is of great practical impor-tance.If,for example,the critical temperature T c(L)of a lattice with L31sites in three dimensions varies asymptotically as T c(L)−T c(∞)∝1/L y with some correlation length exponent y=1/ν,then a plot of the numerical T c(L)versus1/L y gives the extrapolated T c(∞)as an intercept.If,however, higher order terms make the curve T c(L)non-monotonic,then such a plot for finite L,where the non-monotonicity is not yet visible,would give a wrong estimate for T c(∞).Similar effects would make estimates of other quantities unreliable,and there exist examples of such estimates in the literature.2Field-theoretic calculationsWe consider theϕ4model with the standard Landau-Ginzburg-Wilson Hamil-tonianH(h)= V 12(▽ϕ)2+u0ϕ4−h·ϕ (1) whereϕ(x)is a one-componentfield in afinite cube of volume V=L d and h is a homogeneous externalfield.We assume periodic boundary conditions. Accordingly we haveϕ(x)=L−d kϕk e i k·x(2) where the summation k runs over discrete k=2πm j,m j=0,±1,±2,...,j=1,2,...,d in the range−Λ≤k j<Λ,i.e., Lwith a sharp cutoffΛ.The temperature enters through r0=r0c+a0t,t= (T−T c)/T c.As pointed out recently[12]the Hamiltonian(1)for periodic boundary con-ditions with a sharp cutoffΛdoes not correctly describe the exponential size dependence of physical quantities offinite lattice models in the region ξ≫L.Instead of(1),a modified continuum Hamiltonian with a smooth cutoff[12]would be more appropriate.Even better would be to employ the lattice version of theϕ4theory to describe the non-scaling lattice effects of2finite Ising models in the regionξ≫L.In the present paper,however,we shall neglect such effects by taking the limitΛ→∞(see below).Thefluctuating homogeneous part of the order-parameter of the Hamiltonian (1)isΦ=V−1 V d d xϕ(x)=L−dϕ0.As previously[4,5]ϕis decomposed asϕ(x)=Φ+σ(x)(3)whereσ(x)includes all inhomogeneous modesσ(x)=L−d k=0ϕk e i k·x.(4)The order-parameter distribution function P(Φ)≡P(Φ,t,h,L)is defined by functional integration overσ,P(Φ,t,h,L)=Z(h)−1 Dσe−H(h),(5) whereZ(h)= ∞−∞dΦ Dσe−H(h)(6) is the partition function of system.This distribution function depends also on the cutoffΛwhich implies non-scalingfinite-size effects[11,12].From the order-parameter distribution function P(Φ)we can calculate the magnetiza-tionM=<|Φ|>= ∞−∞dΦ|Φ|P(Φ).(7)The functional integration overσin Eqs.(5)and(6)can only be done per-turbatively[4,5,6].Recently a novel perturbation approach was presented [7,8].Using this approach the order-parameter distribution can be written in the formP(Φ)=e−H ef f(Φ)/ ∞−∞dΦe−H ef f(Φ)(8)3where the(bare)effective Hamiltonian of the Ising-like system readsH eff(Φ)=H0(Φ,h)−1Z1[y0m(r0)]},(9)H0(Φ,h)=L d(1L2m2).The function Z1[y]in Eq.(9)is defined asZ1[y]= ∞0ds s exp(−1∞−∞dz exp[−F(x,q,z)],(13) with x=hLβδ/ν,q=tL1/ν,z=ΦLβ/νandF(x,q,z)=c2(x,ˆq)ˆz2+c4(x,ˆq)ˆz4−x·z−1Z1[y m(˜r L(x,ˆq,0))]}.(14)Hereˆq=Q∗t(L/ξ0)1/νandˆz=(2Q∗)β(Φ/A M)(L/ξ0)β/νare dimensionless variables normalized by the asymptotic amplitudesξ0and A M of the bulk cor-relation lengthξ=ξ0t−νat h=0above T c and of the bulk order-parameter M bulk=A M|t|βat h=0below T c.The bulk parameter Q∗is known[13]. The coefficients c2(x,ˆq)and c4(x,ˆq)read for d=3c2(x,ˆq)=(64πu∗)−1ˆq˜ℓ(x,ˆq)3−(2β+1)/ν(1+12u∗),(15)c4(x,ˆq)=(256πu∗)−1˜ℓ(x,ˆq)3−4β/ν(1+36u∗),(16)4where u∗is thefixed point value of the renormalized coupling[13].In three dimensions we havey m(˜r L(x,ˆq,ˆz))=[6πu∗˜ℓ(x,ˆq)]−1/2[˜r L(x,ˆq,ˆz)˜ℓ(x,ˆq)2+4π2m2],(17)˜r L(x,ˆq,ˆz)=ˆq˜ℓ(x,ˆq)−1/ν+(3/2)˜ℓ(x,ˆq)−2βνˆz2.(18)The auxiliary scaling function˜ℓ(x,ˆq)of theflow parameter is determined by ˜ℓ(x,ˆq)3/2=(4πu∗)1/2[˜y(x,ˆq)+12ϑ2(˜y(x,ˆq),ˆx)],(19)˜y(x,ˆq)=(4πu∗)−1/2˜ℓ(x,ˆq)3/2−1/νˆq,(20)ˆx=A M(2Q∗)−βξβ/ν0(4πu∗)1/4√2˜y s2−s4)2˜y s2−s4).(22)From Eqs.(7)and(12)we obtain the scaling formM(h,t,L)=L−β/νf M(hLβδ/ν,tL1/ν),(23)f M(x,q)= ∞−∞dz|z|exp[−F(x,q,z)]bulk amplitudesξ0=0.495,A M=1.71in units of the lattice constant(of the sc Ising model)and the bulk critical exponentsβ=0.3305,ν=0.6335. Thus our determination of the scaling function f(x,y)does not require a new adjustment of nonuniversal parameters.Taking the limit hLβδ/ν→∞atfixed t/h1/βδ,we obtain the scaling form of the bulk equation of stateh/Mδ=f b(t/h1/βδ)=f(∞,t/h1/βδ).(27)At T=T c wefind from Eqs.(23)-(27)h/Mδ≡D c=f(∞,0)=0.202(28) in three dimensions(in units of the lattice constant).3Monte Carlo simulationStandard heat bath techniques were used for the Glauber kinetic Ising model, with multi-spin coding(16spins in each64-bit computer word).Since the effect could be seen best in lattices of intermediate size L≃80for L×L×L spins,memory requirements were tiny and only trivial parallelization by replication,not by domain decomposition,was used.However,thousands of hours of processor time were needed since we see the non-monotonic effects clearly in ourfigure if h/Mδis plotted.The exponentδis nearlyfive and thus five percent accuracy in h/Mδrequires one percent accuracy in the directly simulated magnetization M.Earlier simulations by the same author and algorithm[15]did not show the non-monotonic effects at T=T c because they were not searched for;at that time thefield-theoretical predictions presented above were not yet known.6But even if they had been known it is doubtful that with the Intel Paragon used in[15]instead of the Cray-T3E now the non-monotonic trends would have been seen in about the same computer time.Because of the limited system size,errors in the magnetization of order1 +const/Lβ/ν≃1+const/√finite-size deviation from the bulk value of M should vanish exponentially in L,and not with a power law∝1/L d(as predicted by perturbation the-ory based on the separation of the zero-mode[4-7]).Fig.2a shows again non-monotonic behaviour,in both three andfive dimensions.But only in three dimensions these data are accurate enough to distinguish between a tail varying exponentially and one∝1/L d;Fig.2b clearly supports the the-oretically predicted[11,12]exponential variation.(These three-dimensional data were taken with Ito’s fast algorithm[18].)In order to make contact with bulk properties we also used simulations at the critical isotherm with12923spins[15].From the simulations we obtain the bulk value of h/Mδas D c=0.21±0.02.Ourfield-theoretic result in Eq.(28)is in very good agreement with this value.It is interesting to compare our simulation result also with other bulk theories. From series expansion Zinn and Fisher[17]obtained C c=0.299for the amplitude of the bulk susceptibility at the critical isothermχ=C c|h|−γ/βδwithγ=1.2395,ν=0.6320.This leads to D c=0.182according to therelation D c=(C cδ)−δ.D c is also contained in the universal combination of amplitudes[16](29)Rχ=ΓD c Aδ−1MwhereΓis the amplitude of the bulk susceptibilityχ=Γt−γabove T c at h=0 and A M is the amplitude of the spontaneous magnetization M bulk=A M|t|βbelow T ingϕ4field theory at d=3dimensions Guida and Zinn-Justin [1]have obtained Rχ=1.649.They also used theǫ=4−d expansion and obtained Rχ=1.674atǫ=ing these values for Rχand the high-temperature series expansion results[14]Γ=1.0928,A M=1.71and δ=(dν+γ)/(dν−γ)withγ=1.2395,ν=0.6335,we obtain from Eq.(29) D c=0.205(d=3field theory)and D c=0.202(ǫ-expansion),respectively, in good agreement with our theoretical result,Eq.(28),and with our MC8simulation.In summary,our simulations confirmed a posteriori our theoretical predic-tions of Sect.2for the asymptoticfinite-size effects in the three-dimensional Ising model.The agreement in Fig.1is remarkable in view of the fact that the non-universal parameters of the theory were adjusted only to bulk parameters of the Ising model at h=0and not to anyfinite-size MC data.AcknowledgmentsSupport by Sonderforschungsbereich341der Deutschen Forschungsgemein-schaft and by NASA under contract numbers960838,1201186,and100G7E094 is acknowledged.X.S.C.thanks the National Science Foundation of China for support under Grant No.19704005,D.S.thanks the German Supercomputer Center in J¨u lich for time on their Cray-T3E.9References[1]R.Guida and J.Zinn-Justin,Nucl.Phys.B489,626(1997).[2]Applications of the Monte Carlo Method in Statistical Physics,editedby K.Binder,Topics in Applied Physics36,Springer,Berlin-Heidelberg 1987,in particular chapter1.[3]M.E.Fisher,in Critical Phenomena,Proceedings of the1970Interna-tional School of Physics”Enrico Fermi”,Course51,edited by M.S.Green(Academic,New York,1971).[4]E.Br´e zin and J.Zinn-Justin,Nucl.Phys.B257,867(1985).[5]J.Rudnick,H.Guo and D.Jasnow,J.Stat.Phys.41,353(1985).[6]A.Esser,V.Dohm and X.S.Chen,Physica A222,355(1995);A.Esser,V.Dohm,M.Hermes and J.S.Wang,Z.Phys.B97,205(1995);X.S.Chen,V.Dohm and A.L.Talapov,Physica A232,375(1996).[7]X.S.Chen,V.Dohm and N.Schultka,Phys.Rev.Lett.77,3641(1996).[8]X.S.Chen and V.Dohm,Physica A235,555(1997).[9]X.S.Chen and V.Dohm,Int.J.Mod.Phys.B12,1277(1998).[10]J.Rudnick,y and D.Jasnow,Phys.Rev.E58,2902(1998).[11]X.S.Chen and V.Dohm,Eur.Phys.J.B7,183(1999).[12]X.S.Chen and V.Dohm,Eur.Phys.J.B,in press.[13]R.Schloms and V.Dohm,Nucl.Phys.B328,639(1989);Phys.Rev.B42,6142(1990);V.Dohm,Z.Phys.B60,61(1985).[14]A.M.Liu and M.E.Fisher,Physica A156,35(1989).10[15]D.Stauffer,Physica A244,344(1997),appendix.[16]A.Aharony and P.C.Hohenberg,Phys.Rev.B13,3081(1976).[17]S.Zinn and M.E.Fisher,Physica A226,168(1996).[18]N.Ito,Int.J.Mod.Phys.C7,99(1996).11Figure CaptionsFig. 1.Scaling plot(in units of the lattice constant,see Ref.[9])of h/Mδversus x=hLβδ/νbelow T c with t/h1/βδ=−1.0in part a,t/h1/βδ=0(that means T=T c)in part b,t/h1/βδ=1.0in part c,and t/h1/βδ=1.6in part d. Monte Carlo data for L=32and80.Solid line is the theoretical prediction Eqs.(23)-(26);no Monte Carlo data are shown in part d,where h/Mδis a monotonic function of externalfield x=hLβδ/ν.Fig.2.a)Monte Carlo data for the spontaneous magnetization in units of the lattice constant in three(diamonds and plusses)andfive(square) dimensions at T/T c=0.99,versus linear lattice size L.The horizontal line M=0.3671for three dimensions is determined from L=2496.b)Selected three-dimensional data from part a)are shown as M(L=∞)−M(L)versus L in a semilogarithmic plot.The straight line represents an exponential decay[11,12],the two curved lines are power law decays1/L2 and1/L3which fail tofit the data.Thefive-dimensional data of part a) were not accurate enough to distinguish between an exponential and a1/L5 decay.12。