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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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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Black holes
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description 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.
doi_str_mv 10.1103/PhysRevD.96.044001
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source American Physical Society:Jisc Collections:APS Read and Publish 2023-2025 (reading list)
subjects Black holes
title Near horizon geometries and black hole holograph
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