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Evolution of scalar perturbations near the Cauchy horizon of a charged black hole

Yekta Gürsel and Vernon D. Sandberg

Igor D. Novikov

A. A. Starobinsky

  • W.K. Kellogg Radiation Laboratory, California Institute of Technology, Pasadena, California 91125

  • Space Research Institute Academy of Science, Profsoyuznaja 88, Moscow, 117810, Union of Soviet Socialist Republics

  • The Landau Institute for Theoretical Physics, Academy of Sciences of the USSR, Moscow, Union of Soviet Socialist Republics

Phys. Rev. D 19, 413 – Published 15 January, 1979

DOI: https://doi.org/10.1103/PhysRevD.19.413

Abstract

We describe the evolution of a scalar test field on the interior of a Reissner-Nordström black hole. For a wide variety of initial field configurations the energy density in the scalar field is shown to develop singularities in a neighborhood of the geometry's Cauchy horizon, suggesting that for a stellar collapse curvature singularities will develop prior to encountering the Cauchy horizon. The extension to the interior of stationary perturbations due to exterior sources is shown not to disrupt the Cauchy horizon.

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