Role of magnetic interactions in neutron stars
EPJ Web Conf. 95 (2015) 04001 In this work, we present a calculation of the non-Fermi liquid correction to the specific heat of magnetized degenerate quark matter present at the core of the neutron star. The role of non-Fermi liquid corrections to the neutrino emissivity has been calculated beyond l...
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| Zusammenfassung: | EPJ Web Conf. 95 (2015) 04001 In this work, we present a calculation of the non-Fermi liquid correction to
the specific heat of magnetized degenerate quark matter present at the core of
the neutron star. The role of non-Fermi liquid corrections to the neutrino
emissivity has been calculated beyond leading order. We extend our result to
the evaluation of the pulsar kick velocity and cooling of the star due to such
anomalous corrections and present a comparison with the simple Fermi liquid
case. |
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| DOI: | 10.48550/arxiv.1604.07573 |