Near Horizon Geometries and Black Hole Holograph

Published 6 Jan 2017 in gr-qc | (1701.01704v1)

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.

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