Vacuum structure and chiral symmetry breaking in strong magnetic fields for hot and dense quark matter
arXiv:1101.0498 · doi:10.1103/PhysRevD.84.014016
Abstract
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. ~
24 pages with 12 figures. three new figures, discussions added; version to appear in Phys Rev. D
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- Magnetised neutron star crust within effective relativistic mean-field model
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- QCD sum rule analysis of Heavy Quarkonium states in magnetized matter -- effects of (inverse) magnetic catalysis
- Heavy quarkonia in QGP medium in an arbitrary magnetic field
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- Dirac sea effects on Heavy Quarkonia decay widths in magnetized matter -- a field theoretic model of composite hadrons
- An NJL model analysis of a magnetised nonextensive QCD medium
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- Thermoelectric transport coefficients of quark matter