Vacuum structure and chiral symmetry breaking in strong magnetic fields for hot and dense quark matter

Details Vacuum structure and chiral symmetry breaking in strong magnetic fields for hot and dense quark matter Vacuum structure and chiral symmetry breaking in strong magnetic fields for hot and dense quark matter

2011-01-03

arxiv.org/abs/1101.0498v2

Phys.Rev.D84:014016,2011

Physics

High Energy Physics

High Energy Physics - Phenomenology

24 pages with 12 figures. three new figures, discussions added; version to appear in Phys Rev. D

Scientific paper

10.1103/PhysRevD.84.014016

We investigate chiral symmetry breaking in strong magnetic fields at finite temperature and densities in a 3 flavor Nambu Jona Lasinio (NJL) model including the Kobayashi Maskawa t-Hooft (KMT) determinant term, using an explicit structure for the ground state in terms of quark antiquark condensates. The mass gap equations are solved self consistently and are used to compute the thermodynamic potential. We also derive the equation of state for strange quark matter in the presence of strong magnetic fields which could be relevant for proto-neutron stars. ~

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