Transcript Kapusta
Phase Fluctuations near the Chiral Critical Point Joe Kapusta University of Minnesota Winter Workshop on Nuclear Dynamics Ocho Rios, Jamaica, January 2010 Phase Structure of QCD: Chiral Symmetry and Deconfinement • If the up and down quark masses are zero and the strange quark mass is not, the transition may be first or second order at zero baryon chemical potential. • If the up and down quark masses are small enough there may exist a phase transition for large enough chemical potential. This chiral phase transition would be in the same universality class as liquid-gas phase transitions and the 3D Ising model. Phase Structure of QCD: Diverse Studies Suggest a Critical Point • • • • • • • Nambu Jona-Lasinio model composite operator model random matrix model linear sigma model effective potential model hadronic bootstrap model lattice QCD Goal: To understand the equation of state of QCD near the chiral critical point and its implications for high energy heavy ion collisions. Requirements: Incorporate critical exponents and amplitudes and to match on to lattice QCD at µ = 0 and to nuclear matter at T = 0. Model: Parameterize the Helmholtz free energy density as a function of temperature and baryon density to incorporate the above requirements. T / T0 / 0 2 2 1 lattice QCD nuclear matter P A4T 4 A2T 2 2 A0 4 B2T02T 2 B0T04 Coefficients are adjusted to: (i) free gas of 2.5 flavors of massless quarks (ii) lattice results near the crossover when µ=0 (iii) pressure = constant along critical curve. Cold Dense Nuclear Matter 2 Kn Model I : E0 (n) E0 (n0 ) 1 18 n0 n Kn (n) mN E0 (n0 ) 1 3 1 18 n0 n0 Stiff 2 2 K n Model II : E0 (n) E0 (n0 ) 1 9 n0 2 K n n (n) mN E0 (n0 ) 1 2 1 9 n0 n0 Soft n0 0.153 fm 3 E0 (n0 ) 16.3 MeV K 250 30 MeV (4n0 ) 1230 150 MeV Parameterize the Helmhotz free energy density to incorporate critical exponents and amplitudes and to match on to lattice QCD at µ = 0 and to nuclear matter at T = 0. f ( , t ) f 0 (t ) f1 (t ) f 2 (t ) f (t ) 2 (n nc ) / nc and t (T Tc ) / Tc f 0 (t ) a (t ) 2 if t 0 f 0 (t ) f 0 (t ) a t 2 if t 0 2 c 2 0 T f1 (t ) 0 nc 1 (1 t ) 2 T Parameterize the Helmhotz free energy density to incorporate critical exponents and amplitudes and to match on to lattice QCD at µ = 0 and to nuclear matter at T = 0. f ( , t ) f 0 (t ) f1 (t ) f 2 (t ) f (t ) 2 (n nc ) / nc and t (T Tc ) / Tc f 2 (t ) b (t ) if t 0 f 2 (t ) f 2 (t ) b t if t 0 f 5Pc 512 MeV/fm 3 along critical curve Critical exponents and amplitudes c ( t ) when t 0 s (n, T ) cV T T c t whe n t 0 1 ( t ) when t 0 B P ( n , T ) n T 2 n n t whe n t 0 l g ~ (t ) along coexistenc e curve P Pc ~| | sign ( ) along critical isotherm exponents are related : 2 2 and ( 1) / 5 and c / c 0.5 are universal term | | in free energy has 1 0.11 0.325 1.24 4.815 phase coexistence spinodal 1.24 0.11 Expansion away from equilibrium states using Landau theory ( , T ; ) 0 ( , T ) [( f1 nc ) f 2 2 f | | ]V f 0 nc V 0 along coexistence curve The relative probability to be at a density other than the equilibrium one is P( ) exp / T P(l ) f 2 2 l2 f | | | l | V Volume = 400 fm3 Volume = 400 fm3 Future Work • A more accurate parameterization of the equation of state for a wider range of T and µ. • Incorporate these results into a dynamical simulation of high energy heavy ion collisions. • What is the appropriate way to describe the transition in a small dynamically evolving system? Spinodal decomposition? Nucleation? • What are the best experimental observables and can they be measured at RHIC, FAIR or somewhere else? Supported by the U.S. Department of Energy under Grant No. DE-FG02-87ER40328.