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lattice QCD at finite temperature and density kazuyuki kanaya kanaya@ . .ac.jp 08/10/15

lattice QCD at Þnite temperature - Tsukuba

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Page 1: lattice QCD at Þnite temperature - Tsukuba

lattice QCDat finite temperature

and density

kazuyuki kanayakanaya@ . .ac.jp

08/10/15

Page 2: lattice QCD at Þnite temperature - Tsukuba

contents

introduction to lattice QCD at T > 0 and/or µ ≠ 0 how we calculate where we need care

status: how far are we ? watʼs new at Lattice 2008 ? (just keywords)

phase diagram

2

Page 3: lattice QCD at Þnite temperature - Tsukuba

lattice QCD at T > 0 / µ ≠ 0 how we calculate •••

T > 0: Matsubara formalism euclidian path integral of LQCD with finite euclidian-time extent.

vary T by varying a in terms of g at fixed Nt

‣ or by varying Nt at fixed a3

b0 =1

16π2

(11− 2

3NF

), b1 =

1(16π2)2

(102− 38

3NF

)

+ NP corrections

: asymptotic scaling

Nt

Ns

T =1

Ntaa

Z = Tre−H/T =∫

DqDq̄DUe−S;

a = const.× (b0g2)−b1/(2b20)e−1/(2b0g2)

Page 4: lattice QCD at Þnite temperature - Tsukuba

lattice QCD at T > 0 / µ ≠ 0 how we calculate ••• (2)

thermodynamic quantities from derivatives of Z trace anomaly (interaction measure)

For derivatives in V and T, e.g., , we need separate derivatives in at and as on anisotropic lattice and Karsch coefficients, whose NP values not easy.

integral method in conventional fixed Nt approachusing the thermodyn. relation for large V,

4

ε− 3p = −T

V

d lnZ

d ln a= −T

V

∂β

∂ ln a︸ ︷︷ ︸NP beta fn.

∂ lnZ

∂β︸ ︷︷ ︸〈··· 〉

β = 6/g2

p = T∂ lnZ

∂V

p =T

VlnZ =

T

V

∫ β

β0

∂ lnZ

∂βdβ p(β0) ≈ 0

Page 5: lattice QCD at Þnite temperature - Tsukuba

5

HotQCD (≈ RBC-Bi + MILC)NF = 2+1improved staggered (AsqTad, p4)mπ ≈ 220 MeVR. Gupta, Lattice 2008

RBC-BiNF = 2+1improved staggered (p4)mπ ≈ 220 MeVM. Cheng et al.PRD 77 (2008) 014511

Page 6: lattice QCD at Þnite temperature - Tsukuba

lattice QCD at T > 0 / µ ≠ 0 how we calculate ••• (3)

This requires T=0 (large Nt) simulations at each ß too. • subtraction of T=0 UV divergences • determination of LCP • etc=> 70-90% of the computer time!

T-integral method in the fixed a approach (Talk by Umeda)using the thermodyn. relation of grand canonical system at µ=0,

==>

Merits: • subtraction by a common T=0 simulation • obviously on a LCP •=> large reduction of the computer time.

6

T∂

∂T

( p

T 4

)=

ε− 3p

T 4

p

T 4=

∫ T

T0

dTε− 3p

T 5

Page 7: lattice QCD at Þnite temperature - Tsukuba

7

200 400 600 800 10000

1

2

3

4

5

6

(!−3p)/T4

3p/T4

!/T4

continuum S.B. limit

T[MeV]

anisotropic lattice"=4#=6.1

T-integral method (WHOT-QCD: Umeda et al. @ Lattice 2008)

Page 8: lattice QCD at Þnite temperature - Tsukuba

lattice QCD at T > 0 / µ ≠ 0 how we calculate ••• (4)

8

µ ≠ 0: sign (complex phase) problem

Quark kernel not -hermete at µ ≠ 0

=> complex Boltzmann weight => large cancellations due to phase fluctuatons while fluctuations ~ O(1), V = lattice vol. => MC simulation O(e+V) expensive.

M(µ)† = γ5M(−µ)γ5

[detM(µ)]∗ = detM(−µ) "= detM(µ)

γ5

⟨eiθ

⟩∼ e−V

∫Dq Dq̄e−Sq(µ) = detM(µ)

U4 = eiaA4 =⇒ U4eiaµq (positive direction);

U4e−iaµq (negative direction)

Z =∫

DqDq̄DUe−S; S = Sg +∑

q̄M [U ] q

Page 9: lattice QCD at Þnite temperature - Tsukuba

lattice QCD at T > 0 / µ ≠ 0 how we calculate ••• (4)

9

µ ≠ 0 Methods for small µ ★ Taylor expansion in µ around µ = 0 <= major studies ★ reweighting from µ = 0★ analytic continuation from imaginary µ★ canonical ensemble

=> RHIC/LHC region OK crit. point ??

Intermediate-large µ ????still challenging

Page 10: lattice QCD at Þnite temperature - Tsukuba

10

Bielefeld-SwanseaNF = 2, improved KS (p4)mq

bare / T = 0.4, Nt = 4Allton et al., PRD 71 (2005) 054508

Page 11: lattice QCD at Þnite temperature - Tsukuba

lattice QCD at T > 0 / µ > 0 where we need care •••

we are not very close to the cont. limit yet. fixed Nt studies mostly at Nt = 4-8

lattice artifacts due to large a and small NtAt Tc ≈ 180 MeV, we have:

=> Nt ≥ 8 hopefully

T-integral method in fixed a approachlarge Nt around Tc (Nt > 10 with usual a)=> lattice artifacts smaller there

11

Page 12: lattice QCD at Þnite temperature - Tsukuba

lattice QCD at T > 0 / µ > 0 where we need care ••• (2)

lattice quarks- naïve lattice fermions: doubler problem (improved) staggered (Kogut-Susskind) quarks‣ relatively cheap => most extensively used‣ degeneracy of 4 quarks with O(a2) mixing.

original idea= 4 flavors, but not easy to dissolve=> “fourth root trick” to drop additional 3 “tastes”

- still many additional valence “quarks” => many “hadrons”- still different flavor+taste symmetry- nonlocality - O(4) scaling for NF = 2 QCD not seen yet.

12

detM =⇒ [detM ]1/4 by hand

=> universality class??

Page 13: lattice QCD at Þnite temperature - Tsukuba

lattice QCD at T > 0 / µ > 0 where we need care ••• (3)

lattice quarks (2) (improved) Wilson fermions‣ more expensive => need various improvements‣ flavor symmetry & locality naturally realized

QCDPAX/CP-PACS NF = 2, µ = 0 (ʻ96-ʼ03): O(4) scaling confirmed, phase structure quark masses are still heavyWHOT-QCD (ʻ06-): screening masses, µ ≠ 0

• Taylor expansion method with various improvements• T-integral method for lighter quarks

13

Page 14: lattice QCD at Þnite temperature - Tsukuba

14

CP-PACSNF = 2, improved WilsonmPS/mV = 0.65-0.95, Nt = 4AliKhan et al., PRD 63 (2000) 034502

h = 2 mq

t = ß - ßchiral trans.

fit withO(4) critical exponents

}QCDO(4) Heisenberg model

Page 15: lattice QCD at Þnite temperature - Tsukuba

lattice QCD at T > 0 / µ > 0 where we need care ••• (4)

lattice quarks (3) lattice chiral fermions (DW, overlap)

still expensive (O(100) times more computer time)

first results of DW simulations (RBC/HotQCD) “in infancy” (C. DeTar, plenary @ Lattice 2008)

15

Page 16: lattice QCD at Þnite temperature - Tsukuba

lattice QCD at T > 0 / µ > 0 where we need care ••• (5)

and more finite volume effects and FSS violation of chiral symmetry MEM • • •

please enjoy

16

Page 17: lattice QCD at Þnite temperature - Tsukuba

status

how far are we?

Page 18: lattice QCD at Þnite temperature - Tsukuba

how was it at ?

Started with plenaries by C. DeTar on “QCD Thermodynamics” S. Ejiri on “LQCD at finite density”

18

Williamsburg, VA, USA, July 14-19, 2008

38 talks and 6 posters on T > 0 / µ > 0

Page 19: lattice QCD at Þnite temperature - Tsukuba

38 talks

19

6 posters

T > 0 µ > 0

C. Miao Lattice Calculation of Hadronic ...

Page 20: lattice QCD at Þnite temperature - Tsukuba

C. DeTar on “QCD Thermodynamics” large NF =2+1 simulations near the physical point:

HotQCD with impr.stag. at mπ ≈ 220 MeV. new ideas:

T-integral method for EOS (WHOT-QCD), etc. Tc confusion diminished:

chiral suscept. problematic for TcTc ~ 170-190 MeV

. . .20

Page 21: lattice QCD at Þnite temperature - Tsukuba

S. Ejiri on “LQCD at finite density” isentropic EOS (MILC, RBC-Bi, HotQCD) results with Wilson-type quarks (WHOT-QCD):

had. fluctuations enhanced toward crit. pt. technical developments for µ > 0 simulations . . .

21

Page 22: lattice QCD at Þnite temperature - Tsukuba

phase diagram at µ = 0 theoretical expectations from effective models

22

3d Z(3) Potts!3d O(4) scaling!

tricritical point!

2nd order line: !

mud (ms*-ms)5/2!

near the !tricritical point!

3d Ising scaling!

~

3d Ising scaling!

Page 23: lattice QCD at Þnite temperature - Tsukuba

phase diagramat µ = 0 (2)

LQCD simulations

23

3d Z(3) Potts!3d O(4) scaling!

3d Ising scaling!

-0.15 0

0.15

0.15

0

-0.15

Re !

Im !

QCDPAXPRD46 (’92)

Wilson-type: OKstaggered-type: not seenDW/overlap: not tested yet

Wilson-type, staggered-type: look OKDW/overlap: not tested yet

Dissent argument by the Pisa group: 1st order at NF=2 (Nt=4, unimproved staggered)

Page 24: lattice QCD at Þnite temperature - Tsukuba

phase diagram at µ = 0 (3) location of the physical point

24

Caveats: • Staggered quarks could not reproduce the O(4) scaling. • How about Wilson-type ?? or DW/ovelap ??? (old unimpr.Wil.=> 1st order)

Intensively studied only with staggered quarks. => crossover

Page 25: lattice QCD at Þnite temperature - Tsukuba

25

de Forcrand and Phillipsen, Lattice 2006unimproved staggered, Nt=4, exact algorithm

Y. Aoki et al., nature05120 (’06) improved staggered (stout), continuum extrap. with Nt=4-10finite size scaling study=> Crossover at the phys. pt.

Page 26: lattice QCD at Þnite temperature - Tsukuba

what usually assumed based on model studies + lattice staggered quark results

phase diagram at µ ≠ 0

26

quark-gluon plasma

phase

hadron

phase color super

conductor? nuclear

matter

µq

Tquark-gluon plasma

phase

hadron

phase color super

conductor? nuclear

matter

µq

T

µ=0

ms ≈ msphys

mud ≈ 0ms ≈ ms

phys

mud ≈ mudphys

Assuming crossoverat µ = 0.

crit.pt.

Page 27: lattice QCD at Þnite temperature - Tsukuba

27

Bielefeld-SwanseaNF = 2, mud/T = 0.4improved stag. (p4), Nt = 4Allton et al., PRD71, 054508 (’05)

0.5 1 1.5 2T/T0

0

5

10

15

20

µq/T=1.2µq/T=1.0µq/T=0.8µq/T=0.6µq/T=0.4µq/T=0.2µq/T=0.0

χq/T2

0.5 1 1.5 2T/T0

0

5

10

15

20

µq/T=1.2µq/T=1.0µq/T=0.8µq/T=0.6µq/T=0.4µq/T=0.2µq/T=0.0

χI/T2

WHOT-QCDNF = 2, mPS/mV = 0.65improved Wilson, Nt = 4KK, Lattice 2008

Page 28: lattice QCD at Þnite temperature - Tsukuba

28

RBC-BiNF = 2+1, mπ ≈ 220 MeVimproved stag. (p4), Nt = 4, 6C. Miao, Lattice 2008

µ = 0

Page 29: lattice QCD at Þnite temperature - Tsukuba

29

phase diagram at µ ≠ 0 (2)

where is the critical point?

quark-gluon plasma

phase

hadron

phase color super

conductor? nuclear

matter

µq

T

Assuming crossoverat µ = 0.

• Lee-Yang zero (Fodor and Katz)<= critique by Ejiri (PRD73,054502(’06))

• radius of convergence of Taylor expansion:NF=2, 2+1, staggered-type quarks, Nt=4 mostly

compiled by C. Schmidt, Lattice 2008

Page 30: lattice QCD at Þnite temperature - Tsukuba

30

phase diagram at µ ≠ 0 (3)

Naive expectation

de Forcrand-Phillipsen

imaginary µ methodunimproved stag., Nt=4JHEP01 077, Lattice 2008

=> slightly negative curvature at µ=0.The crit. surface should bend back!

Page 31: lattice QCD at Þnite temperature - Tsukuba

summary

LQCD: direct bridge between1st principles of QCD <=> hadron / QGP physics

Predictions availabele.caveats: several systematic errors not well controlled yet.

Simulations becoming constantly realistic.Direct studies just at the physical point started.

(plenary by Y. Kuramashi, Lattice 2008)Feed back to finite temperature and density will be stareted soon.

Page 32: lattice QCD at Þnite temperature - Tsukuba

thank you

Page 33: lattice QCD at Þnite temperature - Tsukuba

lattice QCD at T > 0 how we calculate •••

line of constant physics (LCP) A physical system (with various a, i.e various g) is given by a line in the coupling parameter space:

Nf=2 QCD with improved Wilson quarks(CP-PACS Collab., WHOT-QCD Collab.)LCP by at T = 0.

Different line = different worldOur world is given by LCP for

To heat up a given physical system in fixed Nt approaches,we have to follow the LCP for this system.

33

= 6/g2

mPS/mV

mPS/mV = mπ/mρ = 135/770