Role of magnetic interactions in neutron stars

作者: Souvik Priyam Adhya , Pradip K. Roy

DOI: 10.1051/EPJCONF/20159504001

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摘要: In this work, we present a calculation of the non-Fermi liquid correction to specific heat magnetized degenerate quark matter at core neutron star. The role corrections neutrino emissivity has been calculated beyond leading order. We extend our result evaluation pulsar kick velocity and cooling star due such anomalous comparison with simple Fermi case.

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