Inner-horizon instability and mass inflation in black holes

Details Inner-horizon instability and mass inflation in black holes Inner-horizon instability and mass inflation in black holes

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phrvl..63.1663p&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 63, Oct. 16, 1989, p. 1663-1666. Research supported by the University of Alberta,

Statistics

Computation

72

Black Holes (Astronomy), Computational Astrophysics, Gravitational Collapse, Stability, Doppler Effect, Relativity, Universe

Scientific paper

Gravitational collapse with rotation leaves a slowly decaying radiative tail which becomes infinitely blueshifted at the inner horizon of the resulting black hole. The gravitational effects of this on the inner structure of the hole are studied using a simple spherical model. In the presence of outflow from the collapsing star, the gravitational-mass parameter and the curvature are inflated at and within the inner horizon to values which, classically, are unlimited. Implications of this result are briefly discussed.

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