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Beijing. San Diego. Symmetry Restoration and Breaking. Is there a first order phase transition in QCD? Under what conditions will the phase transition and, hence, the chiral symmetry restoration and breaking of center Z(3) symmetry occur?. Finite Density Q C D Phase Transition
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Beijing San Diego
Symmetry Restoration and Breaking • Is there a first order phase transition in QCD? • Under what conditions will the phase transition and, hence, the chiral symmetry restoration and breaking of center Z(3) symmetry occur?
Finite Density QCD Phase Transition from Lattice Calculation • Finite Density Algorithm with Canonical Approach • Winding Number Expansion Method • Results on NF = 2, and 4 with Wilson Fermion • NF = 3 with Clover Fermion χQCDCollaboration: Anyi Li, Andrei Alexandru, KFL, and XiangfeiMeng PKU, June 29, 2009
Quark Gluon Plasma (QGP) Phase Hardonic Phase
RHIC : Au-Au collisions with 200 GeV/A PHOBOS BRAHMS PHENIX STAR Relativitic Heavy Ion Collider
RHIC Relativistic (ideal) hydrodynamics + initial cond. + freezeout + … Soft physics from lattice QCD -- EoS, Tc etc Hard physics from pQCD -- jet energy loss etc L. Landau (1953) Current Methodology to study QGP T. Hatsuda Lattice ‘06
Phase DiagramUnder Study T Crossover μ We want to study here
Finite density lattice QCD calculations: Multi-parameter Reweighting Taylor Expansion Imaginary Chemical Potential Canonical Ensemble with Reweighting …
Canonical Ensemble Approach: is real
T T S S A0 A0 T T S S A1 A2
Avoid the Overlap Problem KFL (Int. Jou. Mod. Phys. B16, 2017 (2002)) The earlier procedure is like projection after variation (Peierls and Yoccoz) Need variation after projection (Zeh-Rouhaninejad-Yoccoz) Accept/reject based on detB. Unfortunately, this introduces fluctuation problem! Because
Canonical ensembles Discrete Fourier transform Canonical approach K. F. Liu, QCD and Numerical Analysis Vol. III (Springer,New York, 2005),p. 101. Andrei Alexandru, Manfried Faber, Ivan Horva´th,Keh-Fei Liu, PRD 72, 114513 (2005) Standard HMC Accept/Reject Phase Continues Fourier transform Useful for large k WNEM 21 Finite density simulation with the canonical ensemble Anyi Li - Lattice 2008 Williamsburg
Instability of discrete Fourier transform It’s difficult to pick up the high frequency modes with discrete Fourier transform Winding number expansion in canonical approach to finite densityXiangfeiMeng - Lattice 2008 Williamsburg
Winding number expansion (I) In QCD Tr log loop loop expansion In particle number space Where Winding number expansion in canonical approach to finite densityXiangfeiMeng - Lattice 2008 Williamsburg
T T S S A0 A0 T T S S A1 A2
Winding number expansion (II) For So The first order of winding number expansion Here the important is that the FT integration of the first order term has analytic solution is Bessel function of the first kind . Winding number expansion in canonical approach to finite density Xiangfei Meng - Lattice 2008 Williamsburg
Winding number expansion test (I) K=12 Winding number expansion in canonical approach to finite density Xiangfei Meng - Lattice 2008 Williamsburg
Winding number expansion test (III) Winding number expansion in canonical approach to finite density Xiangfei Meng - Lattice 2008 Williamsburg
Observables Polyakov loop Baryon chemical potential Phase 29 Finite density simulation with the canonical ensemble Anyi Li - Lattice 2008 Williamsburg
Phase Diagrams T T First order ? ρq ρh Mixed phase ρ μ
T plasma hadrons coexistent ρ Phase diagram Two flavors Four flavors ? T plasma hadrons coexistent ρ 31 Finite density simulation with the canonical ensemble Anyi Li - Lattice 2008 Williamsburg
Baryon Chemical Potential for Nf = 4 (mπ ~ 1 GeV) 32 Finite density simulation with the canonical ensemble Anyi Li - Lattice 2008 Williamsburg
Phase Boundaries from Maxwell Construction Nf = 4 Wilson gauge + fermion action Maxwell construction : determine phase boundary 33 Finite density simulation with the canonical ensemble Anyi Li - Lattice 2008 Williamsburg
T plasma hadrons coexistent ρ Phase diagram Two flavors Four flavors ? T plasma hadrons coexistent ρ 35 Finite density simulation with the canonical ensemble Anyi Li - Lattice 2008 Williamsburg
Baryon Chemical Potential (mπ ~ 1 GeV) 36 Finite density simulation with the canonical ensemble Anyi Li - Lattice 2008 Williamsburg
Summary • Canonical Ensemble Approach overcomes the overlap problem and alleviates the fluctuation problem. No sign problem for T > 0.8 Tc. • Exact algorithm which can discern a first order phase transition from finite volumes. • Wilson fermion on 63 x 4 lattice with mπ ~ 1 GeV shows NF = 2 is 2nd order (?) down to 0.83 Tc, NF = 4 is first order. • Iwasaki + Clover fermion on 63 x 4 lattice with mπ ~ 0.8 GeV results for NF = 3 shows an unambiguous first order phase transition at finite density.
Future • Smaller masses • Larger volume HNMC (A. Alexandru, et al. arXiv:0711.2678) • Chiral fermion action • Lower temperature (sign problem)
Phase Boundaries Ph. Forcrand,S.Kratochvila, Nucl. Phys. B (Proc. Suppl.) 153 (2006) 62 4 flavor (taste) staggered fermion
Winding number expansion (IV) The parameters of Winding number expansion---Fourier series The recursion of Bessel function Winding number expansion in canonical approach to finite density Xiangfei Meng - Lattice 2008 Williamsburg
Phase Boundary (Preliminary) Nf = 4 This work Ph. Forcrand,S.Kratochvila, Nucl. Phys. B (Proc. Suppl.) 153 (2006) 62 48 Finite density simulation with the canonical ensemble Anyi Li - Lattice 2008 Williamsburg