English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT

Released

Journal Article

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;

/persons/resource/persons20670

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;

External Resource
No external resources are shared
Fulltext (restricted access)
There are currently no full texts shared for your IP range.
Fulltext (public)

0403029.pdf
(Preprint), 2MB

Supplementary Material (public)
There is no public supplementary material available
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: https://hdl.handle.net/11858/00-001M-0000-0013-4F15-3
Abstract
There is no abstract available