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Quantizing magnetic field and quark-hadron phase transition in a neutron star

Debades Bandyopadhyay·Somenath Chakrabarty·Subrata Pal
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Abstract

We investigate the influence of a strong magnetic field on various properties of neutron stars with quark-hadron phase transition. The one-gluon exchange contribution in a magnetic field is calculated in a relativistic Dirac-Hartree-Fock approach. In a magnetic field of $5\times 10^{18}$G in the center of the star, the overall equation of state is softer in comparison to the field-free case resulting in the reduction of maximum mass of the neutron star.

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Debades Bandyopadhyay, Somenath Chakrabarty, Subrata Pal. 1997-07-31. Quantizing magnetic field and quark-hadron phase transition in a neutron star. https://doi.org/10.1103/physrevlett.79.2176

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