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Ab initio many-body calculation of excitons in solid Ne and Ar

Ab initio many-body calculation of excitons in solid Ne and Ar
Ab initio many-body calculation of excitons in solid Ne and Ar

a r X i v :c o n d -m a t /0412584v 1 [c o n d -m a t .o t h e r ] 21 D e c 2004

Ab initio many-body calculation of excitons in solid Ne and Ar

S.Galami′c -Mulaomerovi′c and C.H.Patterson

Department of Physics and Centre for Scienti?c Computation,University of Dublin,Trinity College,Dublin 2,Ireland

(Dated:February 2,2008)

Absorption spectra,exciton energy levels and wave functions for solid Ne and Ar have been calculated from ?rst principles using many-body techniques.Electronic band structures of Ne and Ar were calculated using the GW approximation.Exciton states were calculated by diagonalizing an exciton Hamiltonian derived from the particle-hole Green function,whose equation of motion is the Bethe-Salpeter equation.Singlet and triplet exciton series up to n =5for Ne and n =3for Ar were obtained.Binding energies and longitudinal-transverse splittings of n =1excitons are in excellent agreement with experiment.Plots of correlated electron-hole wave functions show that the electron-hole complex is delocalised over roughly 7a.u.in solid Ar.

PACS numbers:71.10.Li,71.35.-y,71.35.Aa,78.40.-q

I.INTRODUCTION

Electronic and optical properties of rare gas solids (RGS)Ne and Ar have been studied experimentally 1,2,3,4,5,6,7,8,9,10and theoretically 11,12,13,14,15,16,17,18and have been the subject of several review articles 19,20,21.Optical absorption spectra are characterized by sharp exciton peaks at energies up to sev-eral eV below the fundamental band gap.Excitons in RGS consist of a hole in a p -type valence band and an electron in an s -type conduction band.The momentum of the hole can be either j =3/2(spin triplet)or j =1/2(spin sin-glet).Spin-orbit coupling mixes these states and so pairs of transverse exciton lines,labelled by principal exciton quan-tum numbers n and n ′,are observed in optical absorption ex-periments.When spin-orbit coupling is weak,as in Ne,ener-gies of these excitons ought to be close to the spin singlet and triplet energies.Creation of longitudinal excitons in electron energy loss experiments produces a longitudinal polarisation ?eld which couples to the associated long-range macroscopic electric ?eld and leads to energy splitting of longitudinal (L)and transverse (T)excitons of the same principal quantum number.

An integral equation approach has been applied to excitons in insulators for over 40years 22.This incorporates screened electron-hole attraction and exciton exchange terms in the Hamiltonian.Early applications of this approach to RGS 12,13used an approximation in which the exciton wavefunction was restricted to a single unit cell (one site approximation).Following this,Resca and coworkers developed an approach which took into account the delocalised nature of the exci-ton wavefunction by solving an effective mass equation 14,15,18.In this approach the electron-hole attraction term was un-screened when both electron and hole were on a single site and screened by a macroscopic dielectric constant factor when they were on different sites.Modi?cation of the electron-hole attraction term as a function of electron-hole separation in this way leads naturally to a quantum defect correction,E n =E g ?B ex /(n +δn )2,to the Wannier formula for ex-citon energies,E n =E g ?B ex /n 2.E g is the fundamen-tal band gap and B ex is the exciton binding energy.Resca and Resta 15showed that the former expression could predict exciton energies rather well with a weak dependence of the

quantum defect,δn ,on n.However,subsequent direct mea-surements of the fundamental band gaps in RGS 23showed that the fundamental gap derived from a ?t to the Wannier formula (excluding the n ′=1exciton)yielded a value for E g in good agreement with the experimental values while the quantum defect model yielded quite different values.Bern-storff et al.24concluded that RGS excitons ’do not possess atomic parentage’.Exciton wavefunctions for RGS are there-fore well known to have strong but incomplete localization of the electron and hole on the same site.This intermedi-ate binding character of excitons in RGS means that they are far from the well-separated electron-hole pair limit,which applies to semiconductors and is well described by the ef-fective mass approximation theory 25.A recent calculation 11,which used a screened Coulomb electron-hole interaction and a Slater-Koster parametrization of the band structure,found good agreement with experimental exciton energies and delo-calization of the electron-hole wavefunction over three nearest neighbor distances.

The integral equation approach was applied to diamond 26,27and silicon 28by Hanke and Sham in the 1970’s using a tight-binding parameterization of the band structure.Strinati 29showed how the equation of motion for the particle-hole Green function,the Bethe-Salpeter equation 30,for core-hole excitons could be reduced to an effective eigenvalue prob-lem.Recent ab initio calculations of valence excitons in crys-talline solids 31,32,33have been based on this effective eigen-value problem and the Bethe-Salpeter formalism has been reviewed 34.In this paper we present ab initio calculations of excitonic absorption spectra and correlated electron-hole wave functions for excitons in Ne and Ar.Quasiparticle band energies are calculated using the GW approximation 35and the Bethe-Salpeter formalism 34,which includes statically screened electron-hole attraction and exciton exchange terms,is used to calculate the optical spectrum.This is generated us-ing matrix elements between the ground state and correlated electron-hole excited states and the longitudinal-transverse (LT)splitting of excitons is investigated.

The remainder of the paper is arranged as follows:In Sec-tion II the theoretical formalism is presented,in Section III re-sults of calculations of optical spectra and correlated electron-hole wave functions in solid Ne and Ar are given and ?nally

2 conclusions are given in Section IV.

II.THEORETICAL BACKGROUND

A.Quasiparticle energies

The starting point in our approach is to generate the quasi-

particle energies and wave functions of the system.Quasi-

particle energies are obtained by solving the quasiparticle

equation36,

H(r)ψQP

m

(r)+ Σ(r,r′,E)ψQP m(r′)d r′=?mψQP m(r),(1)

using perturbation theory.The unperturbed Hamiltonian is a

Kohn-Sham Hamiltonian and the self-energy operator,Σ,is

obtained using the GW approximation(GW A).Quasiparti-

cle wave functions,ψQP

m (r),are approximated by eigenfunc-

tions of the unperturbed Kohn-Sham Hamiltonian.Density functional theory(DFT)within the Perdew-Wang generalized gradient approximation37(PWGGA)is used to obtain DFT eigenvectors and eigenvalues.Details of GW calculations as well as quasiparticle band structures along symmetry lines for Ar and Ne are given in Ref.[35].The CRYSTAL code38 was used to generate single-particle wave functions for Ne and Ar in an all-electron Gaussian orbital basis and the Coulomb potential was expanded in plane waves.GW and BSE cal-culations were carried out using the EXCITON39code.The spin-orbit interaction was omitted from the calculations and experimental lattice constants were used19.

B.Electron-hole excitations and optical spectra Correlated electron-hole states,|N,S ,can be represented in a basis of single-particle quasi-electron(conduction,c)and quasi-hole(valence,v)states,

|N,S = k vc A S k vc?a??b?|N,0 = k vc A S k vc|k vc ,(2) where?a?and?b?create a quasi-hole and quasi-electron,re-spectively,in the many-body ground state|N,0 .Coupling

coef?cients,A S

k vc ,and excitation energies,?S,are obtained

by solving the BSE in the form34,

(E k c?E k v)A S k vc+ k′v′c′ vc k|Ξ|v′c′k′ A S k′v′c′=?S A S k vc,(3) whereΞdenotes the electron-hole interaction and energies E k c and E k v are quasiparticle energies obtained within the GW A.The interaction kernel,Ξ,is given as a sum of two terms34:the screened electron-hole attraction,also called the direct interaction,Ξd,and the exchange interaction,Ξx,which results from bare Coulomb repulsion.Neglecting any dynami-cal screening,the matrix element of the direct term in a plane-wave basis is given by,

vc k|Ξd|v′c′k′ =?

4πe2

|q+G||q+G′|× v′k′|e?(q+G)·r|v k c k|e??(q+G′)·r|c′k′ δq,k′?k.(4)

ε?1

GG′

(q,ω=0)is the symmetrized,inverted,static RPA di-electric matrix40,G and G′span the reciprocal lattice and?denotes the crystal volume.When computing the matrix el-ements in Eq.(4)special care has to be taken for the case q→0.If G=G′=0the interaction diverges as1/q2.This contribution is separated from the left side of Eq.(3)and in-tegrated over a small sphere of volume V=V BZ/N k where V BZ is the volume of the Brillouin zone and N k is the num-ber of k points,as suggested by Arnaud and Alouani33.This divergence contributes notably only when v=v′and c=c′. In addition a divergence of type1/q occurs when one of the G vectors is zero.These terms are neglected,because their contribution either averages to zero or vanishes in the limit of a large number of k points33.

The exchange term of the interaction for singlet states has the form34,

vc k|Ξx|v′c′k′ =

4πe2

G2

c k|e?G·r|v k v′k′|e??G·r|c′k′ .(5)

The G=0term omitted from Eq.(5)is responsible for LT splitting of singlet excitons41.It has the form,

4πe2

E k c?E k v

.?Q?Q T.

v′k′|p|c′k′

?q2 S|

v,c,k v k|e??q·r|c k A S k vc|2

3 In Eq.(7)optical transitions are given as a coherent sum

of the transition matrix elements of the contributing electron-

hole pair con?gurations,including the coupling coef?cients,

A S k vc.Without the electron-hole interaction,excitations are

given by vertical transitions between independent electron and

hole states.In that limit Eq.(7)reduces to the well known

RPA dielectric function,

εRP A M (ω)=1+2lim

q→0

8πe2

E c k?E v k?ω?i0+

.

(8)

In calculatingεM from Eq.(7),three valence bands,one conduction band and2048Monkhorst-Pack42special k points in the full Brillouin zone were used.An arti?cial broad-ening of0.05eV was introduced in spectral lines.Several

groups34,43,44have used low symmetry,shifted k points to achieve well converged excitonic spectra.Excitons in RGS belong to an intermediate regime,where they are localised in real space and delocalised in reciprocal space(see Section III). Convergence of excitonic spectra can therefore be achieved using special points only.65G vectors were used to calculate the direct part of the interaction,Eq.(4),and up to500were used for the exchange interaction,Eq.(5).An all-electron basis containing5s,4p and2d Cartesian Gaussian orbitals on the atomic nuclear site was used for Ne and a similar basis with7s,6p and4d orbitals on the atomic nuclear site plus2s, 2p and1d orbital on the octahedral interstitial site was used for Ar.The basis used for Ne is smaller than that used pre-viously for a GW calculation on Ne while the Ar basis is the same as used previously(basis set2in Ref.[35]).

III.RESULTS

A.Optical Spectra

1.Neon

The BSE eigenvalue problem was solved for Ne using an exciton exchange term which either included or omitted the LT splitting term(Eq.(6)).Exciton energies and binding en-ergies,E B=E g?E n,are given in Table I and are compared to earlier calculations.In the work by Andreoni et al.13,n=1 and n′=1excitons were calculated using matrix elements and a band structure from an augmented plane wave(APW) calculation and excitons with higher principal quantum num-bers were calculated using the effective mass approximation (EMA).In the work by Martinelli and Pastori Parravicini45 the electron-hole attraction term in the integral equation was treated using a model screened Coulomb potential.Experi-mental exciton energies in Table I are from optical transmis-sion data by Saile and Koch4.Both L and T excitons were observed in thin?lm optical absorption data and the L exci-ton energy of17.75eV from the BSE calculation is in good agreement with a value of17.74eV from electron energy loss data10.

The imaginary part of the macroscopic dielectric function,ε2,derived from Kramers-Kronig transformation of re?ec-

2

4

6

8

10

16182022

16182022

ε

2

ω [eV]

GAP

Ne

x10

x10

BSE

EXP

FIG.1:Imaginary part of the macroscopic dielectric function for Ne calculated using BSE wave functions and from experimental data by Skibowski19.

TABLE I:Exciton energy levels,E n,band gaps,E g,binding en-ergies,E B and LT splittings in solid Ne in eV.Theoretical results from an augmented plane wave(APW)calculation for the n=1 and n′=1states and an effective mass approximation(EMA)cal-culation for n and n′>1,a model screened electron-hole poten-tial calculation and a BSE calculation are compared to experimental peak positions in optical transmission data.The APW and EMA calculations include spin-orbit coupling.Fundamental band gaps and longitudinal-transverse splittings,?LT,are given in the last two rows.

n E n a E n b E n c E B c E n d E B d

E g21.6721.6921.6921.58

?LT e0.230.300.25

a APW/EMA calculation Ref.13.

b SK calculation Ref.45.

c BSE calculation This work.

d Experiment Ref.4.

e j=1/2exciton.

tion measurements by Skibowski19and a BSE calculation(Eq.

(7))for singlet states without the LT splitting in the exchange term are shown in Fig.1.The experimental spectrum shows excitonic absorption at17.49,20.24,20.87and21.30eV19. These are the n′=1,2,3,4(singlet)exciton energies for Ne and they are nearly all coincident with data for Ne by Saile

4

and Koch4(Table I),where data for triplet exciton energies are available also.Singlet and triplet BSE calculations show the?rst two exciton absorption features at17.45(17.25)and 19.95(19.90)eV.While there is good agreement between re-sults of the BSE calculation and experiment for n′and n=1 states,exciton binding energies for n′and n>1are overes-timated.This may be a result of incomplete screening of the electron-hole interaction caused by the limited basis set used in this calculation.Differences in n and n′binding energies decrease with increasing quantum number.Singlet/triplet en-ergy splittings in BSE calculations for the?rst two states are 0.20and0.05eV and these compare to0.14and0.11eV in experiment(Table I).For higher states the BSE predicts es-sentially no splitting while a small splitting is still found in experiment.

When the LT splitting term(Eq.6)is included in the singlet state exchange,the n′=1exciton shifts to17.75eV,which corresponds to an LT splitting of0.30eV.The experimental LT splitting energy in the n=1′exciton is0.25eV and the calculation by Andreoni et al.13gave a value of0.23eV.The L exciton energy coincides with the experimental value of17.75 eV determined by optical absorption in a thin?lm4and a value of17.74eV obtained from electron energy loss experiments10. The LT splitting for the n′=2exciton from a BSE calculation is much smaller and has a value of0.03eV.Energies of T excitons remain essentially the same when the exchange term in Eq.(6)is included.

2.Argon

Singlet and triplet exciton energies and binding energies for Ar derived from BSE calculations and experiment are given in Table II.Experimental exciton binding energies in Ar are reproduced well in parametrized calculations by Andreoni et al.12and by Baroni et al.17.Binding energies from BSE calcu-lations are also in good agreement with experiment,although BSE exciton energy levels lie below experimental values be-cause the band gap is underestimated by0.5eV in the GW calculation used to generate the quasiparticle energies in Eq.

3.Exciton binding constants for j=3/2and j=1/2states have been estimated from experiment6,46.By?tting n and n′>1exciton peak positions to a Wannier plot(i.e.with no quantum defect)we?nd B ex to range between2.06and2.23 eV for the j=1/2exciton and between2.17and2.30eV for the j=3/2exciton.These values are in good agreement with collected data by Bernstorff et al.2

4.When the n and n′=2 levels from the BSE calculation are?tted we?nd a binding constant of2.56eV and when we use the n and n′=3lev-els we?nd a binding constant of2.16eV.The experimental LT splitting energy in the n=1′exciton is0.15eV.The LT splittings derived from the BSE calculation(0.36eV)is signi?cantly larger than that derived from the calculation by Andreoni et al.12(0.19eV)and the experimental value.

The imaginary part of the macroscopic dielectric function from experiment and a BSE calculation for the j=1/2exci-ton are shown in Fig.2.The experimental optical spectrum contains both the n=1and n′=1peaks because spin-TABLE II:Exciton energy levels,E n,band gaps,E g,binding en-ergies,E B,LT splittings and binding constants,B ex,in solid Ar in eV.Theoretical results from an augmented plane wave(APW)cal-culation for the n=1and n′=1states and an effective mass ap-proximation(EMA)calculation for n and n′>1,a model screened electron-hole potential calculation and a BSE calculation are com-pared to experimental peak positions in optical transmission data. The APW and EMA calculations include spin-orbit coupling.Funda-mental band gaps,longitudinal-transverse splittings,?LT,and bind-ing constants from are given in the last three rows.

n E B a E B b E n c E B c E n d E B d E g13.6914.25

?LT e0.190.360.15

B ex2.562.06

a Ref.12.

b Ref.17.

c BSE calculation This work.

d Experiment Ref.6.

e j=1/2exciton.

TABLE III:Fitted exciton binding constants,B ex,and band gaps, E g,in solid Ar in eV.n and n′>1levels have been used for raw experimental data.The n=2and n′=2energies and the GW value for E g have been used for BSE data and result in the same binding energies for j=1/2and j=3/2series.

j B ex a E g a B ex b E g b B ex c E g c

5

024681012141618202224101214161820

10121416

18

ε2

ω [eV] Exp

ω [eV] Theory G A P

Ar

x5

x5

BSE

EXP

FIG.2:Imaginary part of the macroscopic dielectric function for Ar calculated using BSE wave functions and from experimental data by Saile 19.The fundamental gap predicted by the GWA calculation for Ar is less than the experimental gap by 0.5eV .The scale for the BSE spectrum has been shifted by 0.5eV in order to align fundamental gaps in theory and experiment and facilitate comparison of experi-mental and theoretical

spectra.

2

distance from the hole [a.u]

2 distance from the electron [a.u]

FIG.4:Same as

Fig.3along the line AB :electron distribution (left panel)and hole distribution (right panel).Blue circles present atom positions.

onto nearest neighbor sites.A more quantitative display of the electron-hole correlation function is obtained by plotting the modulus squared of the wave function along a line con-taining three Ar atoms (Fig.(4)).These results con?rm ear-lier conclusions 2,11,47that the ?rst exciton is delocalized over nearest neighbor atoms and give for the ?rst time detailed in-formation on the structure of correlated electron-hole func-tions in Ar in real space.

IV .CONCLUSIONS

An exciton Hamiltonian has been diagonalized to obtain singlet and triplet exciton series for Ne up to n =5and Ar up to n =3.Exciton binding energies for n ′=1singlet and n =1triplet excitons for both Ne and Ar are in excellent agreement with experiment.The longitudinal-transverse split-ting of the n ′=1singlet excitons in Ne is in good agreement with experiment;while the value obtained from a BSE cal-culation for Ar exceeds the experimental value (0.36eV c.f.0.15eV),one might expect Ar to have a larger splitting than Ne,as predicted by the BSE calculation (0.36eV c.f.0.30eV),because of a larger polarisability density in Ar.

The band gap for Ne derived from a GW calculation is 21.69eV and agrees very well with the experimental value of 21.58eV .The band gap for Ar from a GW calculation is 13.69eV and underestimates the experimental value of 14.25eV by 4%.The excellent agreement between theory and ex-periment for the band gap of Ne is fortuitous and is a result of using a relatively small basis set with functions located only on atomic sites.When s and p Gaussian orbitals were added to the basis at octahedral interstitial sites of the fcc lattice,the GW band gap was reduced to 20.04eV 35,an underes-timate of the experimental value by 7%.Underestimation of experimental band gaps to this extent is typical of perturbative GW calculations which start with self-consistent Kohn-Sham Hamiltonians,as this work does.

Overestimation of exciton binding energies with n ≥2for Ne,but not for Ar,for which a superior basis set was used,suggests that the limited basis set used for Ne does not ade-quately account for screening of the electron-hole attraction

6

for more extended excitons.When a BSE calculation was performed for Ne using a basis which contained additional interstitial site basis functions,the optical spectrum contained spurious features above the?rst exciton absorption,although the GW calculation with this basis set35did not suffer from similar problems.Binding energies of n=1and n′=1exci-tons are expected to be much less affected by underscreening than those with larger principal quantum numbers since the electron and hole are in close proximity in those states and Coulomb potential is poorly screened at that range.

Plots of correlated electron-hole wave functions for the n=1exciton in Ar show that the extent of delocalisation of the electron-hole pair is quite limited,con?rming that these excitons belong to an intermediate regime between Frenkel and Wannier types.

Acknowledgments

This work was supported by Enterprise-Ireland under Grant number SC/99/267and by the Irish Higher Education Author-ity under the PRTLI-IITAC2program.The authors wish to thank N.Vast for useful discussions.

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How to manage time Time treats everyone fairly that we all have 24 hours per day. Some of us are capable to make good use of time while some find it hard to do so. Knowing how to manage them is essential in our life. Take myself as an example. When I was still a senior high student, I was fully occupied with my studies. Therefore, I hardly had spare time to have fun or develop my hobbies. But things were changed after I entered university. I got more free time than ever before. But ironically, I found it difficult to adjust this kind of brand-new school life and there was no such thing called time management on my mind. It was not until the second year that I realized I had wasted my whole year doing nothing. I could have taken up a Spanish course. I could have read ten books about the stories of successful people. I could have applied for a part-time job to earn some working experiences. B ut I didn’t spend my time on any of them. I felt guilty whenever I looked back to the moments that I just sat around doing nothing. It’s said that better late than never. At least I had the consciousness that I should stop wasting my time. Making up my mind is the first step for me to learn to manage my time. Next, I wrote a timetable, setting some targets that I had to finish each day. For instance, on Monday, I must read two pieces of news and review all the lessons that I have learnt on that day. By the way, the daily plan that I made was flexible. If there’s something unexpected that I had to finish first, I would reduce the time for resting or delay my target to the next day. Also, I would try to achieve those targets ahead of time that I planed so that I could reserve some more time to relax or do something out of my plan. At the beginning, it’s kind of difficult to s tick to the plan. But as time went by, having a plan for time in advance became a part of my life. At the same time, I gradually became a well-organized person. Now I’ve grasped the time management skill and I’m able to use my time efficiently.

英语演讲稿:未来的工作

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