Mechanics of Rotating Isolated Horizons

Details Mechanics of Rotating Isolated Horizons Mechanics of Rotating Isolated Horizons

2001-03-09

arxiv.org/abs/gr-qc/0103026v2

Phys.Rev. D64 (2001) 044016

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

31 pages REVTeX, 1 eps figure; Minor typos corrected and a footnote added

Scientific paper

10.1103/PhysRevD.64.044016

Black hole mechanics was recently extended by replacing the more commonly used event horizons in stationary space-times with isolated horizons in more general space-times (which may admit radiation arbitrarily close to black holes). However, so far the detailed analysis has been restricted to non-rotating black holes (although it incorporated arbitrary distortion, as well as electromagnetic, Yang-Mills and dilatonic charges). We now fill this gap by first introducing the notion of isolated horizon angular momentum and then extending the first law to the rotating case.

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