ar X iv : g r-qc / 0 50 30 16 v 1 4 M ar 2 00 5 Gravitational-Wave Emission from Rotating Gravitational Collapse in three Dimensions

@inproceedings{Baiotti2005arXI,
  title={ar X iv : g r-qc / 0 50 30 16 v 1 4 M ar 2 00 5 Gravitational-Wave Emission from Rotating Gravitational Collapse in three Dimensions},
  author={Luca Baiotti and Ian Hawke and Luciano Rezzolla and Erik Schnetter},
  year={2005}
}
We present the first calculation of gravitational wave emiss ion produced in the gravitational collapse of uniformly rotating neutron stars to black holes in fully threedimensional simulations. The initial stellar models are relativistic polytropes which are dynamically unstable an d with angular velocities ranging from slow rotation to the mass-shedding… CONTINUE READING