Generic weak isolated horizons

Abstract

Weak isolated horizon boundary conditions have been relaxed supposedly to their weakest form such that both zeroth and the first law of black hole mechanics still emerge, thus making the formulation more amenable for applications in both analytic and numerical Relativity. As an additional gain it explicitly brings the non-extremal and extremal black holes at the same footing.

4 pages, 1 figure

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Cited by in corpus (8)

• Laws of Black Hole Mechanics from Holst Action
• Local symmetries of non-expanding horizons
• Quasilocal conformal Killing horizons: Classical phase space and the first law
• Quasilocal rotating conformal Killing horizons
• Horizon Mechanics and Asymptotic Symmetries with a Immirzi-like Parameter in 2+1 Dimensions
• Note on Kerr/CFT correspondence in a first order formalism
• Non- minimally Coupled Scalar Fields, Holst Action and Black Hole Mechanics
• Entropy of Black Holes in N=2 Supergravity