General relativistic collapse of rotating stars

Details General relativistic collapse of rotating stars General relativistic collapse of rotating stars

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981phla...86..318n&link_type=abstract

Physics Letters A, Volume 86, Issue 5, p. 318-320.

Physics

12

Scientific paper

Numerical calculations have been made for the formation process of
rotating black holes. It is suggested that Kerr black holes may be
formed for wide ranges of initial conditions if q (= total angular
momentum M2) is smaller than unity. For q > 1, an
expanding disk or a jet appears.

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