Published August 1, 2011 | Version v1
Journal article

Phase diagrams in the hadron-Polyakov-Nambu-Jona-Lasinio model

  • 1. INFN-Laboratori Nazionali del Sud, Via S. Sofia 62, I-95123 Catania (Italy)
  • 2. Physics and Astronomy Department, University of Catania (Italy)
  • 3. Theoretical Physics Center for Scientific Facilities, Chinese Academy of Sciences, Beijing (China)
  • 4. IHEP, Chinese Academy of Sciences, Beijing (China)
  • 5. Center of Theoretical Nuclear Physics, National Laboratory of Heavy-Ion Accelerator, Lanzhou 730000 (China)
  • 6. Department of Physics and State Key Laboratory of Nuclear Physics and Technology, Peking University, Beijing 100871 (China)

Description

The two-equation of state model is used to describe the hadron-quark phase transition in dense-hot matter formed in heavy-ion collisions. The nonlinear Walecka model is used to describe the hadronic phase. For the quark phase, the Nambu-Jona-Lasinio (NJL) model coupled to Polyakov-loop fields is used to include both the chiral and (de)confinement dynamics. The phase diagrams are derived from the Gibbs conditions and compared with the results obtained in the hadron-NJL model without confinement. As in the hadron-NJL case a first order transition is observed, but with a critical end point at much higher temperatures, a consequence of the confinement mechanism that reduces the degrees of freedom of the quark matter in proximity to the phase transition. Particular attention is devoted to the phase transition in isospin asymmetric matter. Interesting isospin effects are found at high baryon density and reduced temperatures, which are in fact also common to other quark models, like the MIT bag model and the NJL model. Some possible observational signals are suggested to probe in heavy-ion collision experiments at intermediate energies.

Additional details

Publishing Information

Journal Title
Physical Review. D, Particles Fields
Journal Volume
84
Journal Issue
3
Journal Page Range
p. 034028-034028.11
ISSN
0556-2821
CODEN
PRVDAQ

Optional Information

Notes
(c) 2011 American Institute of Physics