Geometric horizons

We discuss black hole spacetimes with a geometrically defined quasi-local horizon on which the curvature tensor is algebraically special relative to the alignment classification. Based on many examples and analytical results, we conjecture that a spacetime horizon is always more algebraically specia...

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Main Authors: Alan A. Coley, David D. McNutt, Andrey A. Shoom
Format: Article
Language:English
Published: Elsevier 2017-08-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269317303544
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author Alan A. Coley
David D. McNutt
Andrey A. Shoom
author_facet Alan A. Coley
David D. McNutt
Andrey A. Shoom
author_sort Alan A. Coley
collection DOAJ
description We discuss black hole spacetimes with a geometrically defined quasi-local horizon on which the curvature tensor is algebraically special relative to the alignment classification. Based on many examples and analytical results, we conjecture that a spacetime horizon is always more algebraically special (in all of the orders of specialization) than other regions of spacetime. Using recent results in invariant theory, such geometric black hole horizons can be identified by the alignment type II or D discriminant conditions in terms of scalar curvature invariants, which are not dependent on spacetime foliations. The above conjecture is, in fact, a suite of conjectures (isolated vs dynamical horizon; four vs higher dimensions; zeroth order invariants vs higher order differential invariants). However, we are particularly interested in applications in four dimensions and especially the location of a black hole in numerical computations.
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spelling doaj.art-c8ef97ad19ef4fe79583b6fed9b80e0c2022-12-21T17:59:02ZengElsevierPhysics Letters B0370-26932017-08-01771131135Geometric horizonsAlan A. Coley0David D. McNutt1Andrey A. Shoom2Department of Mathematics and Statistics, Dalhousie University, Halifax, Nova Scotia, B3H 3J5, CanadaFaculty of Science and Technology, University of Stavanger, N-4036 Stavanger, Norway; Corresponding author.Department of Mathematics and Statistics, Memorial University, St. John's, Newfoundland and Labrador, A1C 5S7, CanadaWe discuss black hole spacetimes with a geometrically defined quasi-local horizon on which the curvature tensor is algebraically special relative to the alignment classification. Based on many examples and analytical results, we conjecture that a spacetime horizon is always more algebraically special (in all of the orders of specialization) than other regions of spacetime. Using recent results in invariant theory, such geometric black hole horizons can be identified by the alignment type II or D discriminant conditions in terms of scalar curvature invariants, which are not dependent on spacetime foliations. The above conjecture is, in fact, a suite of conjectures (isolated vs dynamical horizon; four vs higher dimensions; zeroth order invariants vs higher order differential invariants). However, we are particularly interested in applications in four dimensions and especially the location of a black hole in numerical computations.http://www.sciencedirect.com/science/article/pii/S0370269317303544
spellingShingle Alan A. Coley
David D. McNutt
Andrey A. Shoom
Geometric horizons
Physics Letters B
title Geometric horizons
title_full Geometric horizons
title_fullStr Geometric horizons
title_full_unstemmed Geometric horizons
title_short Geometric horizons
title_sort geometric horizons
url http://www.sciencedirect.com/science/article/pii/S0370269317303544
work_keys_str_mv AT alanacoley geometrichorizons
AT daviddmcnutt geometrichorizons
AT andreyashoom geometrichorizons