Gravitational Collapse with Asymmetries

Details Gravitational Collapse with Asymmetries Gravitational Collapse with Asymmetries

Feb 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970phrvl..24..423d&link_type=abstract

Physical Review Letters, vol. 24, Issue 8, pp. 423-426

Astronomy and Astrophysics

Astrophysics

54

Scientific paper

Two idealized collapse models, involving a magnetic dipole and a gravitational quadrupole, are analyzed, treating departures from sphericity as small perturbations. Radiative leakage (largely downwards through the Schwarzschild radius) causes externally observable asymmetries to decay to zero in an oscillatory fashion, with a period of the order of the Schwarzschild characteristic time 2Gmc3. These results have significant consequences for astrophysics; they imply in particular that a "black hole" cannot be a source of synchrotron radiation.

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