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Gravitational wave from rotating neutron star

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arxiv 1312.5840 v1 pith:SXTK5P5P submitted 2013-12-20 astro-ph.SR nucl-th

Shailesh K. Singh , S. K. Biswal , M. Bhuyan , T. K. Jha , S. K. Patra This is my paper · ORCID
classification astro-ph.SRnucl-th
keywords gravitationalneutronrotatingwaveamplitudeequationrotationalstar
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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 $\sim 10^{-23}$.

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