Properties of Rotating Neutron Star

  • Shailesh K. Singh Institute of Physics, Bhubaneswar 751005, India.
  • S.K. Biswal Institute of Physics, Bhubaneswar 751005, India.
  • M. Bhuyan Institute of Physics, Bhubaneswar 751005, India.
  • T.K.Jha Department of Physics, BITS Pilani, K. K. Birla goa Campus, India.
  • S.K. Patra Institute of Physics, Bhubaneswar 751005, India.
Keywords: Relativistic and Non-relativistic mean field formalisms, equation of state, static and rotating neutron star, gravitational waves

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 evaluate the properties of rotating neutron stars, such as rotational frequencies, moment of inertia, quadrupole deformation parameter, rotational ellipticity 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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References

Shailesh K. Singh, S. K. Biswal, M. Bhuyan, T. K. Jha and S. K. Patra, arXiv:1312.5840.

P. Danielewicz et al., Science 298, 1592 (2002). http://dx.doi.org/10.1126/science.1078070

Published
2015-08-03
How to Cite
Shailesh K. Singh, S.K. Biswal, M. Bhuyan, T.K.Jha, & S.K. Patra. (2015). Properties of Rotating Neutron Star . Journal of Nuclear Physics, Material Sciences, Radiation and Applications, 3(1), 93-96. https://doi.org/10.15415/jnp.2015.31011
Section
Articles