Local symmetries of non-expanding horizons

Abstract

Local symmetries of a non-expanding horizon has been investigated in the 1st order formulation of gravity. When applied to a spherically symmetric isolated horizon only a U(1) subgroup of the Lorentz group survives as residual local symmetry that one can make use of in constructing an effective theory on the horizon.

4 pages, revtex4, no figure. Few typos corrected

References in corpus (5)

• Black hole entropy from an SU(2)-invariant formulation of Type I isolated horizons
• The combinatorics of the SU(2) black hole entropy in loop quantum gravity
• Schwarzschild horizon dynamics and SU(2) Chern-Simons theory
• Laws of Black Hole Mechanics from Holst Action
• Generic weak isolated horizons

Cited by in corpus (8)

• Exponential corrections to black hole entropy
• The Effective Action of Superrotation Modes
• Schwarzschild horizon dynamics and SU(2) Chern-Simons theory
• Weakly Isolated Horizons: First order actions and gauge symmetries
• Reformulation of Boundary BF Theory Approach to Statistical Explanation of the Entropy of Isolated Horizons
• Quasilocal first law of black hole dynamics from local Lorentz transformations
• Hamiltonian Analysis of 3-dimensional Spacetime in Bondi-like Coordinates
• Hamiltonian Analysis of 4-dimensional Spacetime in Bondi-like Coordinates