Structure of the singularity inside a realistic rotating black hole

Details Structure of the singularity inside a realistic rotating black hole Structure of the singularity inside a realistic rotating black hole

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phrvl..68.2117o&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 68, April 6, 1992, p. 2117-2120.

Astronomy and Astrophysics

Astronomy

97

Asymptotic Properties, Black Holes (Astronomy), Perturbation Theory, Relativity, Singularity (Mathematics), Space-Time Functions, Einstein Equations, Gravitation Theory, Reissner-Nordstrom Solution, Schwarzschild Metric, Stellar Rotation

Scientific paper

The structure and results of an analysis of the asymptotic behavior of nonlinear, asymmetric, metric perturbations near the Cauchy horizon inside a Kerr black hole are presented. This analysis suggests that metric perturbations, to all orders in the perturbation expansion, are finite and small at the Cauchy horizon, even though their gradients (and the curvature) diverge there. Accordingly, objects which fall into a realistic rotating blackhole a longtime after the collapse will not be crushed by a tidal gravitational deformations as they approach the curvature singularity.

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