Nuclear thermodynamics and the in-medium chiral condensate
arXiv:1204.4318 · doi:10.1016/j.physletb.2012.06.070
Abstract
The temperature dependence of the chiral condensate in isospin-symmetric nuclear matter at varying baryon density is investigated using thermal in-medium chiral effective field theory. This framework provides a realistic approach to the thermodynamics of the correlated nuclear many-body system and permits calculating systematically the pion-mass dependence of the free energy per particle. One- and two-pion exchange processes, -isobar excitations, Pauli blocking corrections and three-body correlations are treated up to and including three loops in the expansion of the free energy density. It is found that nuclear matter remains in the Nambu-Goldstone phase with spontaneously broken chiral symmetry in the temperature range MeV and at baryon densities at least up to about twice the density of normal nuclear matter, fm. Effects of the nuclear liquid-gas phase transition on the chiral condensate at low temperatures are also discussed.
9 pages, 4 figures. arXiv admin note: substantial text overlap with arXiv:1104.2819
References in corpus (9)
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Cited by in corpus (9)
- Roy-Steiner-equation analysis of pion-nucleon scattering
- Nuclear chiral dynamics and thermodynamics
- Dense baryonic matter: constraints from recent neutron star observations
- Chiral Mirror-Baryon-Meson Model and Nuclear Matter beyond Mean-Field
- Thermodynamic phases and mesonic fluctuations in a chiral nucleon-meson model
- Emergent Hadrons and Diquarks
- Dilepton Radiation from Strongly Interacting Systems
- Partial restoration of chiral symmetry in hot and dense neutron matter
- Functional renormalization group study of nuclear and neutron matter