Black hole singularities: a numerical approach

Details Black hole singularities: a numerical approach Black hole singularities: a numerical approach

1995-06-28

arxiv.org/abs/gr-qc/9506067v1

Phys.Rev.Lett. 75 (1995) 1256-1259

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

4 pages Phys. Rev. style including five figures, provided as compressed postscript files. To appear in Physical Review Letters

Scientific paper

10.1103/PhysRevLett.75.1256

The singularity structure of charged spherical collapse is studied by considering the evolution of the gravity-scalar field system. A detailed examination of the geometry at late times strongly suggests the validity of the mass-inflation scenario~\cite{PI:90}. Although the area of the two-spheres remains finite at the Cauchy horizon, its generators are eventually focused to zero radius. Thus the null, mass-inflation singularity {\em generally}\/ precedes a crushing $r=0$ singularity deep inside the black hole core. This central singularity is spacelike.

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