The interior structure of rotating black holes 1. Concise derivation

Details The interior structure of rotating black holes 1. Concise derivation The interior structure of rotating black holes 1. Concise derivation

2010-10-03

arxiv.org/abs/1010.1269v3

Phys. Rev. D 84, 124055 (2011)

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Version 1: 8 pages, 3 figures. Version 2: Extensively revised to emphasize the derivation of the solution rather than the solu

Scientific paper

10.1103/PhysRevD.84.124055

This paper presents a concise derivation of a new set of solutions for the interior structure of accreting, rotating black holes. The solutions are conformally stationary, axisymmetric, and conformally separable. Hyper-relativistic counter-streaming between freely-falling collisionless ingoing and outgoing streams leads to mass inflation at the inner horizon, followed by collapse. The solutions fail at an exponentially tiny radius, where the rotational motion of the streams becomes comparable to their radial motion. The papers provide a fully nonlinear, dynamical solution for the interior structure of a rotating black hole from just above the inner horizon inward, down to a tiny scale.

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