Testing a stability conjecture of Cauchy horizons in three-dimensional black holes

Details Testing a stability conjecture of Cauchy horizons in three-dimensional black holes Testing a stability conjecture of Cauchy horizons in three-dimensional black holes

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996phrvd..53.1950w&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 53, Issue 4, 15 February 1996, pp.1950-1954

Physics

8

Classical Black Holes, Singularities And Cosmic Censorship, Exact Solutions

Scientific paper

The stability conjecture of Cauchy horizons of black holes suggested by Helliwell and Konkowski is used to investigate the (2+1)-dimensional (3D) black holes under perturbations of infalling null dust and of both outgoing and infalling null dust. The results given by this conjecture agree with that from the mass inflation scenario for 3D black holes. For 3D black holes, we show that the Cauchy horizon is unstable and the corresponding singularities exist.

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