Black hole solutions in 2+1 dimensions

Details Black hole solutions in 2+1 dimensions Black hole solutions in 2+1 dimensions

1995-11-01

arxiv.org/abs/gr-qc/9511003v2

Phys.Rev. D52 (1995) 6860-6862

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

8 pages, RevTeX (to appear in Phys. Rev. D) References to Mann and Ross, and Mann, Chan and Chan added

Scientific paper

10.1103/PhysRevD.52.6860

We give circularly symmetric solutions for null fluid collapse in 2+1-dimensional Einstein gravity with a cosmological constant. The fluid pressure $P$ and energy density $\rho$ are related by $P=k\rho$ $(k\le 1)$. The long time limit of the solutions are black holes whose horizon structures depend on the value of $k$. The $k=1$ solution is the Banados-Teitelboim-Zanelli black hole metric in the long time static limit, while the $k<1$ solutions give other, `hairy' black hole metrics in this limit.

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