Near Horizon Geometries and Black Hole Holograph

Abstract

Two quasi local approaches to black holes are combined: Near Horizon Geometries (NHG) and stationary Black Hole Holographs (BHH). Necessary and sufficient conditions on BHH data for the emergence of NHGs as resulting vacuum solutions to Einstein's equations are found.

References in corpus (4)

• General Kundt spacetimes in higher dimensions
• Stationary Black Holes as Holographs
• Spacetimes foliated by non-expanding and Killing horizons: higher dimension
• When Isolated Horizons met Near Horizon Geometries

Cited by in corpus (5)

• The Near Horizon Geometry Equation on Compact 2-Manifolds Including the General Solution for g > 0
• The Petrov type D equation on genus $>0$ sections of isolated horizons
• Petrov type D equation on horizons of nontrivial bundle topology
• Spacetimes foliated by non-expanding null surfaces in the presence of a cosmological constant
• Multiple Killing Horizons: the initial value formulation for $\Lambda$-vacuum