Nonexistence of degenerate horizons in static vacua and black hole uniqueness

We show that in any spacetime dimension D≥4, degenerate components of the event horizon do not exist in static vacuum configurations with positive cosmological constant. We also show that without a cosmological constant asymptotically flat solutions cannot possess a degenerate horizon component. Sev...

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Main Authors: Marcus Khuri, Eric Woolgar
Format: Article
Language:English
Published: Elsevier 2018-02-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269317310298
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author Marcus Khuri
Eric Woolgar
author_facet Marcus Khuri
Eric Woolgar
author_sort Marcus Khuri
collection DOAJ
description We show that in any spacetime dimension D≥4, degenerate components of the event horizon do not exist in static vacuum configurations with positive cosmological constant. We also show that without a cosmological constant asymptotically flat solutions cannot possess a degenerate horizon component. Several independent proofs are presented. One proof follows easily from differential geometry in the near-horizon limit, while others use Bakry–Émery–Ricci bounds for static Einstein manifolds.
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spelling doaj.art-d45c87b628c349d29f98477db6e76ac42022-12-22T01:14:40ZengElsevierPhysics Letters B0370-26932018-02-01777235239Nonexistence of degenerate horizons in static vacua and black hole uniquenessMarcus Khuri0Eric Woolgar1Department of Mathematics, Stony Brook University, Stony Brook, NY 11794, USADepartment of Mathematical and Statistical Sciences, University of Alberta, Edmonton, AB T6G 2G1, CanadaWe show that in any spacetime dimension D≥4, degenerate components of the event horizon do not exist in static vacuum configurations with positive cosmological constant. We also show that without a cosmological constant asymptotically flat solutions cannot possess a degenerate horizon component. Several independent proofs are presented. One proof follows easily from differential geometry in the near-horizon limit, while others use Bakry–Émery–Ricci bounds for static Einstein manifolds.http://www.sciencedirect.com/science/article/pii/S0370269317310298
spellingShingle Marcus Khuri
Eric Woolgar
Nonexistence of degenerate horizons in static vacua and black hole uniqueness
Physics Letters B
title Nonexistence of degenerate horizons in static vacua and black hole uniqueness
title_full Nonexistence of degenerate horizons in static vacua and black hole uniqueness
title_fullStr Nonexistence of degenerate horizons in static vacua and black hole uniqueness
title_full_unstemmed Nonexistence of degenerate horizons in static vacua and black hole uniqueness
title_short Nonexistence of degenerate horizons in static vacua and black hole uniqueness
title_sort nonexistence of degenerate horizons in static vacua and black hole uniqueness
url http://www.sciencedirect.com/science/article/pii/S0370269317310298
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AT ericwoolgar nonexistenceofdegeneratehorizonsinstaticvacuaandblackholeuniqueness