Simulation of black hole formation in stellar collapse

Details Simulation of black hole formation in stellar collapse Simulation of black hole formation in stellar collapse

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010sf2a.conf..181n&link_type=abstract

SF2A-2010: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics. Eds.: S. Boissier, M. Heydari-

Physics

1

Supernovae: General, Methods: Numerical, Black Hole Physics

Scientific paper

The collapse of massive stars leads in principle to the formation of a black hole with possible observables, from gamma-rays to neutrinos and gravitational waves. The complex physics involved in this phenomenon require the use of numerical models. We here present a starting project, based on the code CoCoNuT, to perform realistic studies in full general relativity and with detailed microphysics, of the collapse of a rotating stellar core to a black hole.

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