Mass inflation and chaotic behaviour inside hairy black holes

Details Mass inflation and chaotic behaviour inside hairy black holes Mass inflation and chaotic behaviour inside hairy black holes

1997-03-18

arxiv.org/abs/gr-qc/9703047v1

Nucl.Phys.B524:427-443,1998

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

22 pages, Latex, 5 figures (8 eps files)

Scientific paper

10.1016/S0550-3213(98)00177-1

We analyze the interior geometry of static, spherically symmetric black holes of the Einstein-Yang-Mills-Higgs theory. Generically the solutions exhibit a behaviour that may be described as ``mass inflation'', although with a remarkable difference between the cases with and without a Higgs field. Without Higgs field the YM field induces a kind of cyclic behaviour leading to repeated cycles of mass inflation - taking the form of violent explosions - interrupted by quiescent periods and subsequent approaches to an almost Cauchy horizon. With the Higgs field no such cycles occur. In addition there are non-generic families with a Schwarzschild resp. Reissner-Nordstr{\o}m type singularity at r=0.

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