Internal Instability in a Reissner-Nordström Black Hole

Details Internal Instability in a Reissner-Nordström Black Hole Internal Instability in a Reissner-Nordström Black Hole

Apr 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973ijtp....7..183s&link_type=abstract

International Journal of Theoretical Physics, Volume 7, Issue 3, pp.183-197

Physics

56

Scientific paper

The question of the effect of asynumetries in gravitational collapse is investigated by considerations of test electromagnetic fields in an extended Reissner-Nordström background. It is found, with ths aid of computer calculations, that instabilities in the test field arise at the inner (Cauchy or anti-event) horizon, though not at the ouier (event) horizon. Thus it is reasonable to infer that in the full coupled Einstein-Maxwell theory the inner horizon will not survive as a non-singular bypersurface when asymmetric perturbations are present, but will instead become a space-time curvature singularity.

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