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QCD Finite Energy Sum Rules and the Isoscalar Scalar Mesons

QCD Finite Energy Sum Rules and the Isoscalar Scalar Mesons
QCD Finite Energy Sum Rules and the Isoscalar Scalar Mesons

a r X i v :h e p -p h /0111158v 1 13 N o v 2001DCPT/01/108

IPPP/01/54

QCD Finite Energy Sum Rules

and the Isoscalar Scalar Mesons

S.N.Cherry a and M.R.Pennington b a Groupe de Physique Th′e orique,IPN Universit′e de Paris-Sud,F-91406Orsay C′e dex,France.b Institute for Particle Physics Phenomenology,University of Durham,Durham,DH13LE,U.K.Abstract We apply QCD Finite Energy Sum Rules to the scalar-isoscalar current to deter-mine the lightest u d meson in this channel.We use ‘pinch-weights’to improve the reliability of the QCD predictions and reduce the sensitivity to the cut-o?s 0.A decaying exponential is included in the weight function to allow us to focus on the contribution from low mass states to the phenomenological integral.On the theoretical side we include OPE contributions up to dimension six and a contribu-tion due to instantons taken from the Instanton Liquid Model.Phenomenologically,

we incorporate experimental data by using a coupling scheme for the scalar current which links the vacuum polarisation to the ππscattering amplitude via the scalar form factor.We ?nd that the sum rules are well saturated for certain instanton

parameters.We conclude that the f 0(400?1200)de?nitely contains a large u

d component,whereas th

e

f 0(980)most likely does not.We are able to estimate the average light quark mass and ?nd m q (1GeV 2)=5.2±0.6MeV.

1

1Introduction

Currently,experiment suggests that there are more scalar mesons than can be accommo-dated in a single quark-model nonet.Many QCD motivated models predict the existence of non-q qq[3]and K

q states,which are the extra states?In the work that follows we hope to shed some light on this question by attempting to determine which of the5scalar-isoscalar mesons currently listed in the Particle Data Group tables[5]is the lightest u d meson in this channel.To address this question we will use the QCD sum rule technique.The answer has importance for chiral symmetry breaking in QCD, see for instance[6,7].

QCD sum rules are integral expressions that relate the hadronic and partonic regimes, i.e.the low energy world of resonances with the high energy world of(tractable)QCD. Since their conception over twenty years ago[8],QCD sum rules have become an estab-lished technique both for calculating hadronic properties in channels,where the QCD expressions are under control,and,conversely,estimating QCD parameters(such as the masses of the quarks)in channels where there is good experimental information.

Using QCD sum rules in the scalar channel is not a new idea.They were?rst applied to the scalar mesons in[9]where Laplace sum rules were used(for a recent review of Laplace Sum Rules see[10]).Here the phenomenological side was represented using the,now standard,resonance+continuum ansatz,with resonances being represented as δ-functions and the continuum being calculated entirely within perturbative QCD.As only the Operator Product Expansion(OPE)terms,discussed in Sect.3,were taken into account on the theory side,exact mass degeneracy between the lightest isoscalar

and isovector was found,with m f

0=m a

=1.00±0.03GeV.The s

q interpretation of these two mesons could not be ruled out with the data then available.

The e?ects of going beyond the OPE were studied in[12],where instantons(see Sect.4)were included on the theoretical side,but not in the QCD continuum on the phenomenological side.Once again the resonances were treated asδ-functions and only the isospin-1channel was considered.It was concluded that the lightest q

For the light scalar mesons the zero-width approximation is not a good one and the?rst attempt to go beyond it in a sum rule investigation was by Elias et al[13].Here resonances were represented by Breit-Wigner formulae,which,whilst better than aδ-function,still do not adequately describe the complex structure in the scalar sector.A further abstraction was introduced by replacing these Breit-Wigner shapes with a Riemann sum of rectangular https://www.doczj.com/doc/dd5304559.html,place sum rules were used,but in an integral form which requires the calculation of perturbative expressions at rather low energy scales.Again instantons were included, but not in the continuum.In the isovector channel,the a0(980)was found to decouple from the sum rule and the mass of the lightest quarkonium isovector was consistent with the a0(1450).In the isoscalar channel the conclusions were not so clear cut,it was predicted that the lightest quarkonium here should have a width less than half of its mass, and although the f0(980)could not be ruled out as the main contributor a lighter state was preferred.Similar conclusions were reached in[14].This study used both Laplace and Finite Energy sum rules,again requiring perturbative expressions to be evaluated at low energies.The authors noted,that for a consistent treatment of the Borel sum rules,the instanton e?ects should also be included in the QCD continuum contribution. The sum rules were dominated by an isoscalar with mass around1GeV and an isovector with mass around1.5GeV,thus suggesting the f0(980)and a0(1450)as the lightest q

q,K?0(1430).Instantons were included and all QCD integrals were carried out in the complex plane,which improves the convergence of perturbative expres-sions.The isovector decay constants were found to be of comparable size,suggesting a similar structure for both.The author concluded that this favoured a Unitarised Quark Model[16]scenario,where two physical hadrons can arise from one‘seed’state.

In the work that follows we will apply QCD Finite Energy Sum Rules introduced in Sect.2to the scalar-isoscalar channel.On the theoretical side we will include in Sects.3 and4instanton e?ects as well as the OPE terms up to dimension six and use the contour improvement prescription to increase the convergence of perturbative expressions.On the the phenomenological side in Sect.5we will incorporate experimental data directly by relating the hadronic vacuum polarisation to theππscattering amplitude via the pion’s scalar form-factor.The sum rules are evaluated in Sect.6and we present our conclusions in Sect.7.

3

2The Sum Rules

The connection between quarks and hadrons is through the vacuum polarisation,Π(s). This is de?ned by the correlation function of two currents,i.e.

Π(s)=i d4x e iqx 0|T{J(x)J(0)}|0 ,(1) where s=q2=?Q2and the currents are chosen so as to select the desired channel.In this work we are considering the scalar-isoscalar mesons and so we choose the Renormalisation Group invariant current

J(x)=m q

u(x)u(x)+√n(x)n(x),(2)

where m q≡1

π s00w(s)ImΠ(s)d s=?1

a phenomenological parameterisation).On the right-hand side we have an integral in the non-physical region(complex s),and here we use?eld theory(i.e.QCD)to calculate the integrand.The assumption that Eq.(3)holds for a range of values of s0is a statement of global quark-hadron duality,i.e.the integral of an hadronic expression is equal to the integral of an expression written in terms of partonic degrees of freedom.

Early sum rule work used positive integer powers of s as weight functions.In this work we wish to investigate the lightest meson in the I=J=0channel,and so we choose a decaying exponential,w(s)=exp(?s/M2).On the phenomenological side,this weight function will suppress the region of the integral s>M2,and so by varying M2we can control which regions of the integrand contribute most signi?cantly to the sum rule.If we also include integer powers of s in the weight function then we can build up a family of sum rules.

Almost by de?nition,at energies where resonances dominate the spectral density,the implications of QCD are not straightforwardly calculable.If QCD were tractable then the technology of QCD sum rules would be redundant.This means that,for moderate values of s0,our straightforward QCD description ofΠ(s)must fail,at the very least, in the region of the positive real axis(see Fig.1).However,it is believed[17]that it is only in the region of the positive,real axis that the straightforward QCD description is particularly unreliable and that in the rest of the s-plane calculable QCD provides a good description of the correlator.Consequently we introduce a zero into the weight function at the point where the circle joins the real axis,i.e.s0.Thus our sum rules have the weight function w(s)=s k(1?s/s0)e?s/M2and we denote them by the symbol T k.Elsewhere in the literature they are often referred to as’pinched weight’sum rules.Then the left hand side of Eq.(3)becomes

T k(s0,M2)≡1

s0 exp ?s

Although the current Eq.(2)is RG-invariant,the correlator it gives rise to is not.As well as making the calculation of the correlator within QCD more di?cult,this would also lead to an unwanted scale dependence in our?nal results.The second derivative of this correlator,Π′′(s),is RG-invariant.AsΠ′′(s)is also analytic within the contour shown in Fig.1,we could choose to write the sum rules completely in terms of this quantity,but ImΠ′′(s)is not directly related to any physical quantity and so we would lose our link to experiment.Instead we use partial integration to re-express the theoretical side of the sum rules in terms ofΠ′′(s).To do this we write the integral on the theoretical side as

i1= v′′(s)Π(s)d s.(5) We now integrate this expression by parts twice to give,

i1=v′(s)Π(s)?v(s)Π′(s)+ v(s)Π′′(s)d s,(6) and arrange the constants of integration which appear in v(s)and v′(s)so that these functions disappear at s=s0.Then our sum rule is

1

2πi |s|=s0v(s)[Π′′(s)]QCD d s.(7) 3The Operator Product Expansion

In order to calculate the vacuum polarisation within QCD we make use of the Operator Product Expansion(OPE)[20].This replaces the matrix element of the product of currents in Eq.(1)by a linear combination of local operators ordered in terms of increasing dimensionality,

Π(s=?Q2)= n C n(Q2) O n .(8)

The?rst term in this expansion is the purely perturbative contribution,with higher dimension terms giving the contribution due to various condensates.We will consider terms up to dimension six,higher order terms are expected to be negligible.Expressions are available in the literature for the dimension zero term to four-loop order,the dimension four term to two loops and the dimension six term at leading order.We quote these expressions with refernces to the original works for the full information.All expressions are given in the

The dimension zero expression can be found in [21]

and

is

given

by Π

′′0(Q 2)=6m 2q

3

?2log Q 2144

?356

log Q 24log 2Q 29

+b 14ζ(3) + ?27204ζ(3) log Q 28log 2Q 224

log 3Q 2

864?

915192

ζ(5),and ζ(n )is the Riemann Zeta function.As Π′′(s )is renormalisation group invariant,we are free to make any convenient choice of the renormalisation scale.We use the ‘contour improvement’prescription,whereby the logs in Eq.(9)are ‘re-summed’by making the choice μ2=Q 2.This improves the convergence of the perturbative series by removing the dependence on large powers of possibly large logs which would appear in the (unknown)higher order terms.The contour improved perturbative contribution to our correlator is then,Π′′0(Q 2)=6m 2q (Q 2)3+a 2s (Q 2) 50712ζ(3) +a 3s (Q 2) ?47816+4752Q 6 6 m q

3

?I g 18 +I s 4a s (Q 2)28π2

,(11)

7

where

I G=?9 a s G2

9 +4a s m s24

+3m4s3 ,(12)

and

I s= m s

7π2 124 .(13)

The leading order dimension six contribution can be taken from[25]and we follow this reference in taking this term at the?xed scale of1GeV.The dimension six contribution is then

Π′′6(Q2)=3m2q(1GeV2)

qσμνGμνaλa q

+π2a s qσμνλa q +2qγμλa q

2{γμ,γν}andλa are the usual Gell-Mann matrices

normalised such that Tr[λaλb]=2δab.Currently there is no reliable method to calculate the vacuum expectation values appearing in Eq.(14),so we follow standard practice and relate these dimension six condensates to the(RG variant)dimension three light quark condensate qσμνGμνaλa q ,this is done via the parameterisation

g qq ,(15) and for the four-quark condensates, qσμνλa q and qγμλa q ,via the vac-uum saturation hypothesis[8].To take into account the possible violation of the vacuum saturation hypothesis we include a multiplicative factor V vs.Thus our?nal expression for the dimension six contribution is

Π′′6(Q2)=6m2q

qq ?

176π2a s V vs

qq 2 .(16)

In order to evaluate all these expressions we need to calculate the running coupling and quark masses at complex values.This is done by solving the four-loop Renormalisation Group Equations that de?ne the QCDβandγfunctions(our conventions for these functions are given in Appendix A).

For the coupling,we choose to solve the implicit equation

a s(μ2)a s(m2τ)d a′m2τ =0,(17)

8

iteratively using Newton’s method.As input,we take the experimental valueαs(m2τ)=

0.334±0.022,as measured by the ALEPH collaboration[28].For reference,had we

used the standard expansion forαs,then at four-loops and with three active?avours,

this central input value would correspond toΛQCD≈365MeV.For higher values of αs(m2τ),or correspondinglyΛQCD,the radiative corrections to Eq.(10)become more

important and start to swamp the higher dimension terms,i.e it becomes more important

to include higher loop corrections to the perturbative contribution than to include the

condensates.It has been argued[29]that the sum rule methodology could become invalid

forΛQCD 330MeV.This is especially problematic for attempts to determine condensate

values via the sum rule technique.As this is not our aim and considering the success of

previous sum rule studies with similar and higher values ofαs(m2τ)(andΛQCD),we feel

justi?ed in applying sum rules to this problem.

The momentum dependence of the quark mass is given by

m q(μ2)=m q(1GeV2)exp a s(μ2)a s(1GeV2)γ(a′)

2π2 K1(ρc

Taking two derivatives we obtain

Π′′i(s)=3ρ2c m2q

Q2)+K21(ρc

qq|ππ .(21)

Inserting a complete set of hadronic states into the correlator Eq.(1)and keeping only the lowest state,i.e.two pions,gives the spectral density in the elastic region,

ImΠ(s)

32π2|d(s)|2,(22) whereβ(s)=

where the coupling function,α(s),is real for real s>4m2π.Substituting Eq.(23) into Eq.(22)and making use of the elastic unitarity relationship Im T=β|T|2,we obtain

ImΠ(s)

32π2

Im T

π=f

Im T(s)

K.Even after

this has opened theππ?nal state will continue to pick out the non-strange contribution to the sum over states.Thus we might expect Eq.(26)to give a reasonable approximation to the true spectral density even above1GeV.We call this Coupling Scheme I.

The multi-pion?nal states mentioned above will increase the n

π=f

(Im T(s))2

K threshold,whereas Coupling Scheme I ignores all

inelastic channels and so will underestimate the spectral density,Coupling Scheme II takes into account all inelastic channels,including those with hidden strangeness,and so may be an overestimate.

As input we take the parameterisation of the I=J=0ππscattering data carried out by Bugg et al[39].However,when continued down to threshold this fails to reproduce the scattering length predicted by Chiral Perturbation Theory(χPT)and so in the region

11

Im T

Energy (GeV)

Figure2:A sketch showing the absorptive part of the I=J=0ππscattering

amplitude as calculated from the data set described in the text(line).Superim-

posed are experimental points from[42](diamonds),[43](boxes),[44](triangles)

and[45](circles).

below450MeV we use the Roy equation extrapolation of the classic Ochs-Wagner phase-shifts[40],as carried out by Pennington and used in the discussion ofγγ→ππ[41].

Fig.2shows a sketch of the absorptive part of the isospin zero,S-wave amplitude forππscattering as calculated from our data set.From this we can clearly see that the f0(400?1200)and the f0(1370)appear as peaks,while the f0(980)and the f0(1500) show up as sharp dips.Thus these latter two states,and in particular the f0(980),will largely decouple from the spectral density and if saturation of the sum rules is achieved with either of our two Coupling Schemes,it will not be due in any great part to the f0(980)or f0(1500).By varying both M2and s0it may be possible to determine which of the f0(400?1200)and the f0(1370)plays the dominant role in saturation,but for the evaluation of the Wilson coe?cients in the OPE to be trustworthy,we would expect s0 to be too high to exclude the f0(1370).Nevertheless,as the decaying exponential in the weight functions of our sum rules suppresses the integrand for s>M2,it is still possible to determine which resonance is most important for saturation.

12

5.2Normalisation

A value for the normalisation factor f,can be determined by making a comparison with the spectral density obtained using an Omn`e s representation[46]of the form factor.This representation is given by

d(s)=d(0)exp s s′(s′?s) ,(28) whereφ(s)is the phase of I=J=0ππscattering.The form factor at zero momentum transfer,which normalises the Omn`e s function,can be determined from the Feynman-Hellman Theorem[47]and is given by

?m2π

d(0)=m q

qq =?m2πf2π[48],and thus we see that

d(0)=m2π.(30) Going to next-to-leading order inχPT would introduce a correction to Eq.(30)of the order of1%(see for example[49]),which is safe to neglect.

To evaluate the integral in Eq.(28)exactly requires knowledge of the scattering phase in the high energy region where it is unknown.However,the integrand is dominated by the region around s.So if we restrict our comparison to the low energy region then the behaviour of the phase above some point s1,where s1?s,will not greatly a?ect the value of the integral.We take s1to correspond to the last data point and approximate the phase above this point as a constant,φ1.Thus,the spectral density,as calculated from the Omn`e s representation,is written

ImΠ(s)

β(s) s1π? s14m2πφ(s′)d s′

32π2

01

2

3

4

5

6

7

I m

Π

/

π

(10-

6

G e V

4)Energy (GeV)

Figure 3:The spectral density below 400MeV as calculated from our Coupling Scheme (points)and the single channel Omn`e s representation (solid line).

6Results

In any sum rule calculation,we hope to ?nd regions of the parameter space where the theoretical and phenomenological sides are equal.We measure this saturation of the sum rules by introducing the double ratios

D k (s 0,M 2)=[T

k +1/T k ]had

Parameter

0.334

qq From GMOR relation[48]

a s G2

m s?(195MeV)4

159MeV

qq

m20Sum rule Estimate[50]

V vs

ρc

νTo be determined

Table1:Standard values of all parameters used to evaluate the sum rules.

6.1The Instanton Parameters

The?rst task is to determineν2,the scale of the quark mass in the instanton contribution. To evaluate Eq.(20),we introduce a new parameter,λ,which is equal to the ratio of m2q(ν2)to m2q(1GeV2),i.e.,

λ= m q(ν2)β(a′)d a′ ,(33) where the second equality follows from Eq.(18).In Fig.4we show the stability curves obtained for various values of this parameter using Coupling Scheme II and s0=3.7GeV2. We have found that the saturation of the sum rules is practically independent of s0in the region3GeV2 s0 4GeV2and so no signi?cance should be attached to this choice of s0.However,it was found that saturation could not be achieved with the standard value ofρc=(600MeV)?1,and in Fig.4we pre-empt the results of Figs.5and6by using the non-standard valueρc=(480MeV)?1.

It is immediately clear that the sum rules are far from satis?ed whenλ=0,i.e.when the instanton contribution is removed.However,the sum rules are well saturated for λ≈1.2and we have found that the best value isλ=1.25,which we will use from now on.This value ofλcorresponds to a scaleν=0.96GeV.

As stated earlier saturation can only be achieved by use of a non standard value of ρc.In Figs.5and6we show the e?ect that varying this parameter has on the saturation curves.We see that good saturation is achieved for1/ρc=470?490MeV,with the‘best’value beingρc=(480MeV)?1≈0.42fm.This value is slightly larger(25%)than the estimate[32]based on the size of the gluon condensate which has become the standard value employed in the Instanton Liquid Model.However,it is entirely consistent with current lattice determinations which tend to?nd sizes in the range0.32–0.43fm and, unless stated otherwise,we will use this‘best’value ofρc from now on.

15

D

M2 (GeV2)

Figure4:The saturation curves obtained for various values ofλ,withρc=

(480MeV)?1and all other parameters as listed in Table1.

6.2Saturation

As shown in Fig.6,once the instanton parameters have been determined the quality of the saturation of our sum rules is very good.This means that the f0(980),being largely decoupled from our Coupling Schemes,does not play an important role in this saturation. On the other hand,the saturation curves are seen to be?at from quite low values of M2. With our weight function suppressing the portion of the integrand s>M2relative to the low energy region,the shape of the curves implies that saturation is achieved long before the f0(1370)contributes signi?cantly to the phenomenological integral.This suggests that it is the f0(400?1200)that plays the most important role in saturating our sum rules.

As the values of the condensates have not been?xed de?nitively,we have performed a number of tests to determine how sensitive the saturation of our sum rules is to variations of these input values.To test the dependence on the size of the gluon condensate,we write

a s G2 =c a s G2 0(34) where a s G2 0is the standard value listed in Table1.In Fig.7we show the saturation curves for various values of this factor,c.We see that the saturation is not strongly dependent on the size of the gluon condensate,but the best results are obtained in the

16

D M 2 (GeV 2)Figure 5:The saturation curves obtained for various values of ρc ,with λ=1.25and

all other parameters as listed in Table 1.D M 2 (GeV 2)Figure 6:As Fig.5but for ?ner steps in ρc .

17

D

M2 (GeV2)

Figure7:The saturation curves,D0,for various values of the gluon condensate.

D

M2 (GeV2)

Figure8:The saturation curves,D0,for various values of the vacuum saturation violation parameter,V vs.

18

range 0≤c ≤2.In Fig.8we see how deviations from vacuum saturation a?ect our results.We ?nd reasonable agreement for 0≤V vs ≤2,suggesting that vacuum saturation may be violated by 100%with little e?ect.For the remaining OPE parameters,varying their values from 0to 200%was found to have no noticeable e?ect.However,the best results are obtained with the strong coupling taken to be close to the central value quoted in Table 1.

6.3The Average Light Quark Mass

Another way to measure whether the sum rules are saturated is by making a prediction for a physical quantity.As M 2is an unphysical parameter,for ‘sensible’values of s 0this prediction should be e?ectively independent of M 2over a wide range.From Eq.(18),we

see that the theoretical side of our sum rules contains an overall factor of m 2q (1GeV 2),

we can thus make an estimate for the average light quark mass from

m q (1GeV 2)= [T k ]calc .(35)

If the graph of this quantity against M 2is found to be ?at then we can say that the sum

4.84.9

5

5.1

5.25.3

5.4

5.5

00.51 1.52 2.53 3.54

m q (M e V )M 2 (GeV 2)Figure 9:The quark mass curves for our two Coupling Schemes.The dashed line shows Coupling Scheme I and the solid line corresponds to Coupling Scheme II.

19

rules are saturated.Although the actual value of the quark mass extracted will depend on the constant f ,its M 2dependence will not,thus as a test of saturation Eq.(35)is independent of any uncertainties in the normalisation of the hadronic side.Once again we will use only the lowest sum rule,i.e.T 0,to estimate the quark mass.

4.84.9

5

5.1

5.25.3

5.4

5.5

00.51 1.52 2.53 3.54m q (M e V )M 2 (GeV 2)ρc = (470 MeV)-1ρc = (480 MeV)-1ρc = (490 MeV)-1(a)Average Instanton Size

4.84.95

5.15.25.35.45.500.51 1.52 2.53 3.54

m q (M e V )M 2 (GeV 2) c = 0c = 1c = 2(b)The Gluon Condensate 4.84.9

5

5.1

5.25.3

5.4

5.5

00.51 1.52 2.53 3.54

m q (M e V )M 2 (GeV 2)V vs = 0V vs = 1V vs = 2(c)Vacuum Saturation Violation Parameter

Figure 10:The e?ect of various parameters on the quark-mass curves.

In Fig.9we show the curve obtained from Eq.(35)using the instanton parameters determined in Sect.6.1for our two Coupling Schemes.We notice immediately that the curve is extremely ?at,in particular for Coupling Scheme II.In both cases the variation is less than 1%in the range 0.6GeV 2≤M 2

20

高考完形填空真题

The journey my daughter Cathy has had with her swimming is as long as it is beautiful. Cathy suffered some terrible 16 in her early childhood. After years of regular treatment, she17became healthy. Two years ago, while Cathy was watching the Olympics, a dream came into her sweet little head— to be a swimmer. Last summer, she wanted to18our local swim team. She practiced hard and finally19it. The team practice,20 ,was a rough start. She coughed and choked and could hardly21 her first few weeks. Hearing her coughing bitterly one night, I decided to22her from it all. But Cathy woke me up early next morning, wearing her swimsuit23to go! I told her she shouldn’swimt after a whole night’coughing,s but she refused to24 and insisted she go . From that day on, Cathy kept swimming and didn ’ t 25 a single practice. She had a 26intention within herself to be the best she could be. My ten-year-old was growing and changing right before my eyes, into this27 human being with a passion and a mission. There were moments of28of course: often she would be the last swimmer in the race. It was difficult for Cathy to accept that she wasn29---ever. But that’didnta’ t stop her from trying. Then came the final awards ceremony at the end of the year. Cathy didn’ t expect any award but was stil 30 her friends and praise their accomplishments. As the ceremony was nearing the end, I suddenly heard the head coach31 ,“ The highest honor goes to Cathy!” Looking around, he continued,“ Cathy has inspired32 us and enthusiasm.33skills and talents bring great success, the most valuable asset(财富 )one can hold is the heart.” It was the greatest34of my da ughter’ s life. With all she hadbeen35in her ten years, this was the hour of true triumph( 成功 ). 16.A. failure B. pressure C. loss D. illness 17.A. usually B. finally C. firstly D. frequently 18.A. improve B. train C. join D. contact 19.A. increased B. found C. created D. made 20.A. however B. therefore C. otherwise D. instead 21.A. use B. survive C. save D. waste 22.A. pull B. tell C. hide D. fire 23.A. afraid B. nervous C. ready D. free 24.A. take off B. set off C. give up D. show up 25.A. attend B. miss C. ban D. Start 26.A. rich B. weak C. firm D. kind 27.A. trusted B.determined C.experienced D. embarrassed 28.A. frustration B. delight C. excitement D. surprise 29.A. beginner B.learner C. partner D. winner 30.A. cheer on B. compete with C. respond to D. run after 31.A. admitting B.explaining C.announcing D. whispering 32.A. humor B. will C. honesty D. wisdom 33.A. Although B. Since C. Once D. Because 34.A. discovery B. choice C. influence D. moment 35.A. through B. under C. across D. around My fiance (未婚夫) and I were excited about shopping for our first home. But our funds were 16 , and none of the houses in our price range seemed satisfactory. One agent 17 a house in particular. Although her description sounded wonderful, the price was18our range, so we declined. But she kept urging us to have a look 19. We finally did and it was20at first sight. It was Our Home, small and charming, overlooking a quiet lake. Walking through the rooms and talking with the owners, a nice elderly couple, we felt the warmth and21of the

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