Inner-structure instability of the Reissner-Nordstrom black hole

Details Inner-structure instability of the Reissner-Nordstrom black hole Inner-structure instability of the Reissner-Nordstrom black hole

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992azh....69..584g&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 69, no. 3, May-June 1992, p. 584-592. In Russian.

Statistics

Computation

Black Holes (Astronomy), Computational Astrophysics, Stability, Einstein Equations, Scalars

Scientific paper

The instability of the inner horizon of Reissner-Nordstrom black hole with respect to scalar perturbations arising on the outer horizon is simulated numerically. It is shown that perturbations incident on the black hole change the black hole structure and create a singularity. If the mass of perturbations is large enough, the singularity consists of two isotropic parts and a spacelike one, in agreement with the strong Cosmic Censor Conjecture. The march null slicing method is used for numerical solution of the Einstein equations.

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