Numerical evolution of secular bar-mode instability induced by the gravitational radiation reaction in rapidly rotating neutron stars

@article{Shibata2004NumericalEO,
  title={Numerical evolution of secular bar-mode instability induced by the gravitational radiation reaction in rapidly rotating neutron stars},
  author={Masaru Shibata and Sigeyuki Karino},
  journal={Physical Review D},
  year={2004},
  volume={70},
  pages={084022}
}
The evolution of a nonaxisymmetric bar-mode perturbation of rapidly rotating stars due to a secular instability induced by gravitational wave emission is studied in post-Newtonian simulations taking into account gravitational radiation reaction. A polytropic equation of state with the polytropic index n=1 is adopted. The ratio of the rotational kinetic energy to the gravitational potential energy T/|W| is chosen in the range between 0.2 and 0.26. Numerical simulations were performed until the… Expand

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