How Wide is the Transition to the Deconfinement

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Presentation transcript:

How Wide is the Transition to the Deconfinement —— A matrix model for the deconfining phase transition Yun Guo* * College of Physical Science and Technology, Guangxi Normal University In collaboration with: A. Dumitru, Y. Hidaka, C. P. Korthals-Altes and R. D. Pisarski What can we learn from Lattice QCD How to construct the matrix model Comparison with Lattice Meisinger, Miller, Ogilvie(MMO), hep-ph/0108009 Dumitru, YG, Hidaka, Korthals-Altes, Pisarski, arXiv:1011.3820 CPOD, Wuhan, 10 Nov. 2011

SU(3) gauge theory without quarks WHOT: (Umeda, Ejiri, Aoki, Hatsuda, Kanaya, Maezawa & Ohno, arXiv:0809.2842) (e-3p)/T4 e/T4 3p/T4 (Weakly) first order transition at Tc ~ 290 MeV Conformal anomaly, (e-3p)/T4: large peak above Tc

pertubation theory vs Lattice Resummed perturbation theory at 3-loop order works down to ~ 3 Tc. (Andersen, Su & Strickland, arXiv:1005.1603) Intermediate coupling: s(Tc) ~ 0.3. (Braaten & Nieto, hep-h/9501375 Laine & Schröder, hep-ph/0503061 & 0603048) From two loop calculation, matching original to effective theory: Not so big... What happens below ~ 3 Tc?

Confinement: <l> = 0 Ansatz: constant background filed, diagonal matrix i, j = 1...N For SU(N), j=1...N qj = 0, modulo 1. Hence N-1 independent qj’s. Polyakov loop : measures ionization of color: <l>↑ Confinement: <l> = 0 Complete QGP: <l> = 1 “semi”-QGP: 0 < <l> < 1 partial ionization Tc ↑ T→

perturbative plus non-pertubative potential At one loop, the potential in a constant A0 background field is given by: 1 Polyakov loop thus predicts a gas of gluons would always be in the deconfined phase. <q> = 0 Higher orders in perturbation theory does not modify this result. Add non-perturbative terms, by hand, to generate <q> ≠ 0 Symmetries of the q’s Periodic: q → q + 1 Z(N) transformation. Ordering of Polyakov loop’s eigenvalues irrelevant.

1-parameter matrix model, N = 2 (Dumitru, YG, Hidaka, Korthals-Altes, Pisarski, arXiv:1011.3820) Add - by hand - a non-pert. potential Vnon ~ T2 Tc2. Also add a term like Vpert: Now just like any other mean field theory. 〈q〉given by minimum of Veff: 〈q〉 depends nontrivially on temperature. Pressure value of potential at minimum:

Three parameters in the model Two conditions: transition occurs at Tc & p(Tc) = 0 Only one free parameter choose c2 to fit (e-3p)/T4: optimal choice Lattice: (Engels, Fingberg, Redlich, Satz & Weber, ’89) MMO model, with c2=0, No free parameter T/Tc

Lattice vs 1-parameter model, N = 2 ⇐ (e-3p)/T4, lattice ⇐ (e-3p)/T4, model ⇓ e/T4, lattice ⇓ e/T4, model ⇑ p/T4, model ⇑ p/T4, lattice

Polyakov loop: 1-parameter matrix model ≠ lattice Lattice: renormalized Polyakov loop. 0-parameter model: close to lattice. 1-parameter model: sharp disagreement. 〈l〉 rises to ~ 1 much faster? Sharp rise also found using Functional Renormalization Group (FRG): (Braun, Gies & Pawlowski, arXiv:0708.2413; Marhauser & Pawlowski, arXiv:0812.1144) ⇓ 1-parameter Lattice: (Cardoso, Cardoso & Bicudo, arXiv:1104.5432) ⇐ 0-parameter ⇐ lattice T/Tc

Interface tension, N = 2  vanishes as T→Tc ,  ~ (t-1)2ν . Ising 2ν ~ 1.26; Lattice: ~ 1.32. Matrix model: ~ 1.5: c2 important. Semi-class.: GKA ’04. Include corr.’s ~ g2 in matrix (T) (ok when T > 1.2 Tc) semi-classical⇒ ⇐ matrix model ⇐ lattice Lattice: (de Forcrand, D’Elia & Pepe, hep- lat/0007034)

Adjoint Higgs phase, N = 2 A0cl ~ q 3, so 〈q〉 ≠ 0 generates an (adjoint) Higgs phase: (Pisarski, hep-ph/0608242; Unsal & Yaffe, arXiv:0803.0344; Simic & Unsal, arXiv:1010.5515) In background field, A = A0cl + Aqu : D0cl Aqu = ∂0 Aqu + i g [A0cl , Aqu] Fluctuations ~ 3 not Higgsed, ~ 1,2 Higgsed, get mass ~ 2T〈q〉 Hence when 〈q〉 ≠ 0, for T < 1.2 Tc, splitting of masses:

T/Tc Adjoint Higgs phase, N = 2 mpert = √2/3 g T m/mpert ~ .56 at 1.5 Tc, from Vnon ⇐ off-diagonal A0 modes ⇐ diagonal A0 mode At Tc: mdiag = 0, moff ~ 2 mpert. T/Tc

(Kaczmarek, Karsch, Laermann & Lattice: A0 mass as T → Tc - up or down? Gauge invariant: 2 pt function of loops: μ/T goes down as T → Tc (Kaczmarek, Karsch, Laermann & Lutgemeier, hep-lat/9908010) Gauge dependent: singlet potential mD/T goes up as T → Tc (Cucchieri, Karsch & Petreczky, hep-lat/0103009; Kaczmarek & Zantow, hep-lat/0503017) Which way do masses go as T → Tc? Both are constant above ~ 1.5 Tc.

Lattice vs 0- and 1- parameter matrix models, N = 3 Results for N=3 similar to N=2. 0-parameter model way off. Good fit (e-3p)/T4 for 1-parameter model, Again, c2 ~ 1, so at Tc, terms ~ q2(1-q)2 almost cancel. ⇐ Points: lattice Lattice: (Bielefeld, hep-lat/9602007 Datta & Gupta, arXiv:1006.0938) ⇐ 1-parameter ⇐ 0-parameter T/Tc

Lattice vs 1- parameter model, N = 3 ⇐ e-3p/T4, lattice ⇐ e-3p/T4, model ⇓ e/T4, model ⇓ e/T4, lattice ⇑ p/T4,model ⇑ p/T4, lattice

Polyakov loop: matrix models ≠ lattice Renormalized Polyakov loop from lattice does not agree with either matrix model 〈l〉 - 1 ~ 〈q〉2, by 1.2 Tc, 〈q〉 ~ .05, negligible. Again, for T > 1.2 Tc, the T2 term in pressure due entirely to the constant term, c3! Rapid rise of 〈l〉 as with FRG. (Braun, Gies & Pawlowski, arXiv: 0708.2413) 1-parameter ⇓ ⇑ 0-parameter Lattice: (Gupta, Hubner & Kaczmarek, arXiv:0711.2251) ⇐ lattice Cannot reconcile by shift in zero point energy T/Tc

Interface tension, N = 3 Order-order interface tension, , from matrix model close to lattice. (Tc)/Tc2 nonzero but small, ~ .02. Results for N =2 and N = 3 similar - ? ⇐ matrix model, N = 2 lattice, N=3 ⇒ Semi-classical⇒ ⇐ matrix model, N = 3 Lattice: (de Forcrand, D’Elia & Pepe, hep-lat/0007034, de Forcrand & Noth, hep-lat/0506005)

Adjoint Higgs phase, N = 3 Splitting of masses only for T < 1.2 Tc: Measureable from singlet potential, 〈tr L†(x) L(0)〉, over all x. mpert = g T, m/mpert ~ .8 at 1.5 Tc, from Vnon. ⇐ 2 off-diagonal ⇐ 4 off-diagonal ⇐ 2 diagonal modes At Tc: mdiag small, but ≠ 0

Matrix model for N ≥ 3 Latent heat, e(Tc)/Tc4: 1-parameter model too small: 1-para.: 0.33. BPK: 1.40 ± .1; DG: 1.67 ± .1. Latttice latent heat: (Beinlich, Peikert & Karsch (BPK), hep-lat/9608141; Datta & Gupta (DG), arXiv:1006.0938) To get the latent heat right, two parameter model. 2-parameter model, c3(T). Like MIT bag constant. WHOT: c3(1) ~ 1. Fit c3(1) to DG latent heat. Thermodynamics, order-disorder interface tensions improve.

Thermodynamics of 2-parameter model, N = 4 ⇓ e/T4, model ⇐ e/T4, lattice ⇓ (e-3p)/(T2Tc2), model ⇑ (e-3p)/(T2Tc2), lattice ⇑ p/T4, model ⇑ p/T4, lattice

Thermodynamics of 2-parameter model, N = 6 ⇓ e/T4, model ⇐ e/T4, lattice ⇓ (e-3p)/(T2Tc2), model ⇑ (e-3p)/(T2Tc2), lattice ⇑ p/T4, model ⇑ p/T4, lattice

Conclusions Need to include quarks! We construct an effective model as a function of the expectation values of the Polyakov loop. We fixed the parameters in this model by fitting the lattice data of conformal anomaly, then use the model to compute other quantities. Transition region: from model < 1.2 Tc! from lattice data < 4 Tc... Above 1.2 Tc, pressure dominated by constant term ~ T2 . (due to small expectation value of q.) Need to include quarks! Can then compute temperature dependence of: shear viscosity, energy loss of light quarks, damping of quarkonia...

Thank You for Your Attention

Backup

〈q〉 ≠ 0 at all T, but numerically, negligible above ~ 1.2 Tc Width of transition region, 0- vs 1-parameter 1-parameter model: 〈q〉! 0 much quicker above Tc sharper (e-3p)/T4 Physically: sharp (e-3p)/T4 implies region where 〈q〉 is significant is narrow. 〈q〉 ≠ 0 at all T, but numerically, negligible above ~ 1.2 Tc ⇐ 0-parameter ⇓ 1-parameter T/Tc Above ~1.2 Tc, the T2 term in the pressure is due entirely to the constant term, c3! This agrees with the lattica data (WHOT).

Lattice data for N ≥ 3 Scaled by ideal gas values, e and p for N = 3, 4 and 6 look very similar N = 3, 4, 6 N=3: (Boyd et al, hep-lat/9602007); N = 4 & 6: (Datta & Gupta, arXiv:1006.0938)

Conformal anomaly ≈ N independent For SU(N), “peak” in (e-3p)/T4 just above Tc. Approximately uniform in N. N = 3, 4, 6 long tail? (Datta & Gupta, arXiv:1006.0938)

Tail in the conformal anomaly To study the tail in (e-3p)/T4, multiply by T2 (divided by (N2-1) Tc2): (e-3p)/T2 approximately constant N = 3, 4, 6 (Datta & Gupta, arXiv:1006.0938)

Interface tensions: order-order & order-disorder Interface tension: box long in z. Each end: distinct but degenerate vacua. Interface forms, action ~ interface tension: T > Tc: order-order interface = ‘t Hooft loop: measures response to magnetic charge (Korthals-Altes, Kovner & Stephanov, hep-ph/9909516) Also: if trans. 1st order, order-disorder interface at Tc . z