Finite temperature effects on anisotropic pressure and equation of state of dense neutron matter in an ultrastrong magnetic field

Physics

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Asymmetric Matter, Neutron Matter, Nuclear Matter Aspects Of Neutron Stars, Neutron Stars, Forces In Hadronic Systems And Effective Interactions

Scientific paper

Spin-polarized states in dense neutron matter with the recently developed Skyrme effective interaction (BSk20 parametrization) are considered in the magnetic fields H up to 1020 G at finite temperature. In a strong magnetic field, the total pressure in neutron matter is anisotropic, and the difference between the pressures parallel and perpendicular to the field direction becomes significant at H>Hth˜1018 G. The longitudinal pressure decreases with the magnetic field and vanishes in the critical field 1018

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