Souvik Priyam Adhya, Pradip K. Roy, Abhee K. Dutt-Mazumder
In this work we have studied the non-Fermi liquid (NFL) behavior that enters into the expression of the pulsar kick velocity of the neutron star composed of degenerate quark matter core. We have incorporated leading order (LO) and next to leading order (NLO) corrections to the velocity and compared the results with the Fermi liquid case. Results for large magnetic field case persistent in neutron stars are also presented. The relation between radius and temperature has been shown with different values of the kick velocity with and without NFL corrections.
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http://arxiv.org/abs/1303.6126
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