Gravitational wave from rotating neutron star
Solar and Stellar Astrophysics
2013-12-23 v1 Nuclear Theory
Abstract
Using the nuclear equation of states for a large variety of relativistic and non-relativistic force parameters, we calculate the static and rotating masses and radii of neutron stars. From these equation of states, we also evaluate the properties of rotating neutron stars, such as rotational and gravitational frequencies, moment of inertia, quadrupole deformation parameter, rotational ellipcity and gravitational wave strain amplitude. The estimated gravitational wave strain amplitude of the star is found to be .
Cite
@article{arxiv.1312.5840,
title = {Gravitational wave from rotating neutron star},
author = {Shailesh K. Singh and S. K. Biswal and M. Bhuyan and T. K. Jha and S. K. Patra},
journal= {arXiv preprint arXiv:1312.5840},
year = {2013}
}
Comments
11 pages, 11 figures. arXiv admin note: text overlap with arXiv:nucl-th/0310075 by other authors