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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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Published in: | Physical review. D 2017-08, Vol.96 (4), p.044001, Article 044001 |
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Main Authors: | , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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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. |
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ISSN: | 2470-0010 2470-0029 |
DOI: | 10.1103/PhysRevD.96.044001 |