Collapse to a rotating black hole

Details Collapse to a rotating black hole Collapse to a rotating black hole

Aug 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978phrvd..18.1020k&link_type=abstract

Physical Review - Particles and Fields, 3rd Series, vol. 18, Aug. 15, 1978, p. 1020-1029. Research supported by the National Res

Astronomy and Astrophysics

Astronomy

10

Black Holes (Astronomy), Gravitational Collapse, Interstellar Gas, Rotating Matter, Adiabatic Flow, Dynamic Characteristics, Einstein Equations, Field Theory (Physics), Gravitational Effects, Perturbation Theory, Schwarzschild Metric

Scientific paper

A slowly rotating black hole is shown to form as a result of gravitational collapse of a dust cloud. The exterior vacuum region is that of the Kerr metric with small rotation parameter at all stages of the collapse; in particular, there is no gravitational radiation. A linearized perturbation of the closed Friedmann-Robertson-Walker dust cloud provides the interior region of the spacetime and matches smoothly to the Kerr exterior. The geometry is shown to be regular on the event horizon. Dragging of inertial frames during the collapse is discussed.

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