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Three-dimensional relativistic simulations of rotating neutron star collapse to a Kerr black hole

MPS-Authors

Hawke,  Ian
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

Seidel,  Edward
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

Löffler,  Frank
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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Rezzolla,  Luciano
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

Stergioulas,  Nikolaos
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

Font,  Jose A.
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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Fulltext (public)

0403029.pdf
(Preprint), 2MB

Supplementary Material (public)
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Citation

Baiotti, L., Hawke, I., Seidel, E., Montero, P. J., Löffler, F., Rezzolla, L., et al. (2005). Three-dimensional relativistic simulations of rotating neutron star collapse to a Kerr black hole. Physical Review D, 71: 024035.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0013-4F15-3
Abstract
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