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Near horizon geometries and black hole holograph

Two quasilocal 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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Bibliographic Details
Published in:Physical review. D 2017-08, Vol.96 (4), p.044001, Article 044001
Main Authors: Lewandowski, Jerzy, Racz, Istvan, Szereszewski, Adam
Format: Article
Language:English
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Summary:Two quasilocal 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.
ISSN:2470-0010
2470-0029
DOI:10.1103/PhysRevD.96.044001