Gravitational collapse of a rotating star. 2: Exterior field of a slowly rotating collapsing star

Details Gravitational collapse of a rotating star. 2: Exterior field of a slowly rotating collapsing star Gravitational collapse of a rotating star. 2: Exterior field of a slowly rotating collapsing star

May 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973stin...7517260t&link_type=abstract

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Gravitational Collapse, Stellar Rotation, Kerr Effects, Metric Space

Scientific paper

The gravitational exterior field outside a slowly rotating collapsing
star is examined. The final field in the course of the collapse is shown
to be expressed by a stationary metric which is exactly Kerr's metric,
and the other nonstationary parts of the metric damp away in a power law
at large time. The case of rapid rotation is also discussed.

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