Modifications to the pulsar kick velocity due to magnetic interactions in dense plasma
High Energy Physics - Phenomenology
2016-06-01 v2 High Energy Astrophysical Phenomena
Abstract
In this work we calculate pulsar kick velocity of magnetized neutron star composed of degenerate quark matter core with non-Fermi liquid (NFL) correction. Both the leading order (LO) and next to leading order (NLO) corrections to the kick velocity have been incorporated. In addition, the NFL corrections to the specific heat of magnetized quark matter have been presented. This has been taken into account to calculate the kick velocity of the neutron star. Results show significant departure from the normal Fermi liquid estimates. The relation between radius and temperature has been shown with kick velocity of with and without NFL corrections.
Keywords
Cite
@article{arxiv.1303.6126,
title = {Modifications to the pulsar kick velocity due to magnetic interactions in dense plasma},
author = {Souvik Priyam Adhya and Pradip K. Roy and Abhee K. Dutt-Mazumder},
journal= {arXiv preprint arXiv:1303.6126},
year = {2016}
}
Comments
15 pages, 8 figures, version accepted for publication in J. Phys. G