5. Thermal Transition for Two Quark Flavours 41
5.5. Strength of the Anomaly
5.5.2. F ree Sreening Masses
Sreeningmasses from thefree theory areexpetedto be realised for asymptoti
tem-peratures
T → ∞
. Besidesprovidingalimitingvaluetheyanalsobelookedattolearnabout volume and utodependene.
Asforinnite temperature therearenointerations, sreeningmassesfrom all
han-nels are expeted to be degenerate. This is illustrated by gure 5.13, where free
or-relators for the pseudo-salar and salaravour non-singlethannels are shown. They
havebeenalulatedbyanumerial inversionofthepropagator withrespettothefree
gaugeeld,
U = 1
.1e-16 1e-14 1e-12 1e-10 1e-08 1e-06 0.0001 0.01 1
0 5 10 15 20 25 30 35 z
ps, N τ =2 sc, N τ =2 ps, N τ =12 sc, N τ =12
Figure5.13.:Free pseudo-salarandsalarorrelatorsfor
N σ = 32
,N τ
=2,12.The value for the free ontinuum meson sreening mass was rst onjetured by
Eletsky and Ioe [183 ℄. A omplete ontinuum alulation was then given in [184 ℄.
Aordingly, the freesreeningmassis dened by
D(p 1 = p 2 = 0, p 3 =
iM
sr/2, p 4 = πT ) = 0 ,
(5.35)where
D(p)
isthepropagator'sdenominatorfortherespetivefermionformulationunder onsideration. Thefator2intheaboverelationanbeinterpretedphysiallyfromthefatthatthesreenedmesonidegreesoffreedomareonstitutedbytwovalenequarks.
We give a alulation for the lattie in appendix C.2 whih is based on mapping the
integrationvariablesontoaunitirle. Byinspetion ofthepolestruture,weanthen
relatetheorrelatortoanexponentialdeaygovernedbyasreeningmassinaordane
withequation(5.35).
For free staggered fermions, the leading order uto eets must be of
O (1/N τ 2 )
.Aordingly, thesreening masshastheform
(M
sr)
staggT = 2
s
π 2 + m 2 q T 2 − 1
3
2π 4 + m T 4 4 q + 2π 2 m T 2 q 2 q
π 2 + m T 2 q 2
1
N τ 2 + . . . ,
(5.36)where
m q
is thefreequarkmass. Wilson fermions,ontheotherhand,suerfromO (a)
eetsthatareintroduedbyanitemass. Takingintoaountapossiblytwistedmass
with
m 2 q = µ 2 0 + m 2 0
,thesreening massisgivenby(M
sr)
tmT = 2 s
π 2 + m 2 q
T 2 − π 2 + m 2 q T 2
! −1/2
m 0 m 2 q T 3
1 N τ
−
1
4 π 2 + m 2 q T 2
! −3/2
m 2 0 m 4 q
T 6
(5.37)+ π 2 + m 2 q T 2
! −1
7
12 π 4 + π 2
48 + m 2 q
48T 2 + m 2 q π 2
2T 2 − m 2 0 m 2 q T 4
!
1
N τ 2 + . . . .
Thus at maximaltwist, i.e.
m 0 = 0
,thequantityisO (a)
-improved,(M
sr)
mtmT = 2
s
π 2 + m 2 q T 2
− π 2 + m 2 q T 2
! −1
7
12 π 4 + π 2
48 + m 2 q
48T 2 + m 2 q π 2 2T 2
! 1
N τ 2 + . . . .
(5.38)Fromtheaboveformulae itan beseenthattheleading disretisationartefatsofall
onsidered lattie formulations are negative, i.e. at least inleading order and
non-interatinglimitthelattiesreeningmassunderestimatesitsontinuumounterpart.
Contrary to that, perturbative ontinuum alulations [185 , 186 ℄ indiate a positive
ontribution introdued byinterations.
Anothersoureofdeviationfromtheontinuuminteratingvaluestemsfromthenite
volume usedinlattie simulations. To getanestimatefor thiseet, we have obtained
valuesforthefreesreeningmassonlattiesofdierentextentwithamaximallytwisted
mass propagator using
µ 0 /T = 0.006
, see gure 5.14. In this ase we have used theeetive mass as dened in equation (5.29) at
z = L/4
to determine the sreeningmass. Whereas we do notnd promiment plateau behaviour for smalllatties, we nd
agreement between the eetive masses from equation (5.29) and equation (5.31) at
the given position. From Florkowski and Friman [184℄ we know that the asymptoti
behaviourofthe massless meson orrelator at hightemperaturesisgiven by
C(z) ≃ 1
z 2 e −2πT z (1 + 2πT z) .
(5.39)This ensures the orret innite distane behaviour, i.e.
m
e(z → ∞ ) = 2πT
.How-ever, for atual simulations, one hasto deal with a nite extent in
z
-diretion. If the5 5.5 6 6.5 7 7.5 8 8.5 9
0 0.01 0.02 0.03 0.04 0.05 0.06 0.07
16 8 6 4
M scr /T
1/N 2 τ N τ
continuum
N σ /N τ =2 N σ /N τ =4 N σ /N τ =6 N σ /N τ =8 infinite volume
Figure5.14.:Freesreeningmassasafuntionofthelattiespaingsquared,
∼ 1/N τ 2
,forfourvaluesoftheaspetratio. Thedatahavebeenobtainedbynumerialinversionof
thefreepropagator,thesolidlinesonsiderallutoeetswhereasthedashed
linesonlyonsidertheleading
1/N τ 2
ontributions.sreeningmassisobtainedfromtheeetivemassatagivendistane,
z = L/n
,thedis-repanyanbealulated,f.[177 ℄. For thispurpose,onehastoexpandthedierene
m
e(L/n) − 2πT
for asmall inverse spatialextent ndingM
srT = M
srT V →∞
+ n N τ
N σ
(5.40)formassless quarks.
Ingure5.14 and 5.15we show orrespondingtsto the freesreening masses.
Fig-ure5.14shows the
N τ
-dependeneat xed aspetratio. For thelattie spaingdepen-denewe use the omplete funtional form as impliitly dened by equation (5.35) in
orderto takepointsatalllattie spaingsinto aount. Thethinnerdashedlines
orre-spondtotheformulaupto
O (1/N τ 2 )
. Theyseemtobeanappropriatedesriptionofthe datapointsforlattieswithN τ & 6
. Thissituationissomewhatbetterthan forthefreepressure, disussed insetion 4.2, where ner lattiesareneeded to ahieve
a 2
-saling.Theonlyfreet parameter leftistheoeient of theontribution linearin1/
N σ
,seeequation(5.40). Aording to theaboveonsiderations,this parametershouldbeequal
to 4, we atually t 4.362(22). For this t we have inluded all points but theone at
N τ = 4
withaspetratio 2 thatislearly out of therangeofanyapproximation.The disrepany of approximately 9% between the expeted value and the tted
onemight beexplainedbynitemasseetswhiharenotinluded inequation(5.40).
However,modiationsduetoanitemass
µ 0 /T ≪ π
shouldberathersmall. Therefore,itismorelikelythatweseehigherordersofthedoubleexpansionin
1/N τ
andtheaspetratio.
Figure5.15showsthevolume dependene atxedlattie spaing
N τ = 4
. Asbefore,thepointwithanaspetratio of2hasbeenomittedfromthet. Theremainingpoints
5 5.5 6 6.5 7
0 0.02 0.04 0.06 0.08 0.1 0.12 M scr /T
1/N σ N τ =4
numerical values analytical formula linear fit to [0.0.08]
Figure 5.15.:Free sreeningmassasa funtion oftheinverse spatialextent for
N τ = 4
andlinearttoallpointsexepttheoneforthesmallestvolume.
give a linear behaviour with tted ordinate 5.28812(21) and slope
4.30(11) · N τ
. Theslopeisothenaivepreditionof4butisinneagreementwiththepreviouslyobtained
valuefor thedataat xed aspetratio.
In onlusion the leading order uto and nite volume eets for free sreening
masses an be modelled,
M
sr1 N τ
, 1 N σ
= M
sr(0, 0) + c (L) N τ
N σ − c (a) 1
N τ 2 ,
(5.41)withpositiveoeients
c (L,a)
thatdependsolelyonthefermions'disretisationsheme thatneeds to beO (a)
-improved, ofourse.Notethatontraryto the above ndings,oneexpetsexponentiallysuppressednite
volume eets for the zero temperature interating spetrum[133 ℄. However, the
or-respondingproofisbasedonthealulation ofzerotemperaturesattering amplitudes.
The lineardependeneof freesreening masseshas alsobeen foundin[177 ℄ where also
arestorationofthe exponentialbehaviourisobservedwhenapproahing
T c
fromabove.Therefore we do not expet nite volume eets as severe as in the free ase for our
dynamial sreeningmasses at