Black-hole formation from stellar collapse

Details Black-hole formation from stellar collapse Black-hole formation from stellar collapse

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cqgra..20s..73f&link_type=abstract

Classical and Quantum Gravity, Volume 20, Issue 10, pp. S73-S80 (2003).

Computer Science

4

Scientific paper

I review the end-state of massive stellar evolution, following the evolution of these massive stars from the onset of collapse through the formation of a compact remnant and the possible supernova or hypernova explosion. In particular, I concentrate on the formation of black holes from stellar collapse: the fraction of stars that form black holes, the black-hole mass distribution and the velocities these black-hole remnants may receive during their formation process.

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