Gravitational collapse of marginally bound spheroids - Initial conditions

Details Gravitational collapse of marginally bound spheroids - Initial conditions Gravitational collapse of marginally bound spheroids - Initial conditions

Nov 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975phrvd..12.3072e&link_type=abstract

Physical Review D - Particles and Fields, 3rd Series, vol. 12, Nov. 15, 1975, p. 3072-3076.

Astronomy and Astrophysics

Astronomy

9

Boundary Value Problems, Gravitational Collapse, Oblate Spheroids, Prolate Spheroids, Black Holes (Astronomy), Gravitational Waves, Relativity, Schwarzschild Metric, Stellar Evolution

Scientific paper

A method is given for solving the general relativistic initial-value problem in the case of some collapsing, marginally bound, nonrotating configurations. Explicit solutions are found for oblate and prolate spheroids. Maximum efficiency limits for subsequent gravitational radiation are 2.5% (oblate) and 3.4% (prolate) for spheroids so compact that they lie within an apparent horizon on the initial slice.

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