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Quantizing magnetic field and quark-hadron phase transition in a neutron star
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Quantizing magnetic field and quark-hadron phase transition in a neutron star
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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.
Forward citations
Cited by 2 Pith papers
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New phenomenological anisotropy profiles in hybrid stars, driven by superconductivity and magnetic fields, lead to enhanced masses and continuous gravitational wave emission.
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