Spacetime Topology and the Laws of Black Hole-Soliton Mechanics

The domain of outer communication of an asymptotically flat spactime must be simply connected. In five dimensions, this still allows for the possibility of an arbitrary number of 2-cycles supported by magnetic flux carried by Maxwell fields. As a result, stationary, asymptotically flat, horizonless...

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Main Author: Hari K. Kunduri
Format: Article
Language:English
Published: MDPI AG 2017-01-01
Series:Entropy
Subjects:
Online Access:http://www.mdpi.com/1099-4300/19/1/35
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author Hari K. Kunduri
author_facet Hari K. Kunduri
author_sort Hari K. Kunduri
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description The domain of outer communication of an asymptotically flat spactime must be simply connected. In five dimensions, this still allows for the possibility of an arbitrary number of 2-cycles supported by magnetic flux carried by Maxwell fields. As a result, stationary, asymptotically flat, horizonless solutions—“gravitational solitons”—may exist with non-vanishing mass, charge, and angular momenta. These gravitational solutions satisfy a Smarr-like relation, as well as a first law of mechanics. Furthermore, the presence of solitons leads to new terms in the well-known first law of black hole mechanics for spacetimes containing black hole horizons and non-trivial topology in the exterior region. I outline the derivation of these results and consider an explicit example in five-dimensional supergravity.
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spelling doaj.art-13aa5c8fd0bc4777b3b2466a84fbedc32022-12-22T02:55:02ZengMDPI AGEntropy1099-43002017-01-011913510.3390/e19010035e19010035Spacetime Topology and the Laws of Black Hole-Soliton MechanicsHari K. Kunduri0Department of Mathematics and Statistics, Memorial University of Newfoundland, St. John’s, NL A1C 2S6, CanadaThe domain of outer communication of an asymptotically flat spactime must be simply connected. In five dimensions, this still allows for the possibility of an arbitrary number of 2-cycles supported by magnetic flux carried by Maxwell fields. As a result, stationary, asymptotically flat, horizonless solutions—“gravitational solitons”—may exist with non-vanishing mass, charge, and angular momenta. These gravitational solutions satisfy a Smarr-like relation, as well as a first law of mechanics. Furthermore, the presence of solitons leads to new terms in the well-known first law of black hole mechanics for spacetimes containing black hole horizons and non-trivial topology in the exterior region. I outline the derivation of these results and consider an explicit example in five-dimensional supergravity.http://www.mdpi.com/1099-4300/19/1/35black holes in higher dimensionssupergravityblack hole thermodynamicsgravitational aspects of string theory
spellingShingle Hari K. Kunduri
Spacetime Topology and the Laws of Black Hole-Soliton Mechanics
Entropy
black holes in higher dimensions
supergravity
black hole thermodynamics
gravitational aspects of string theory
title Spacetime Topology and the Laws of Black Hole-Soliton Mechanics
title_full Spacetime Topology and the Laws of Black Hole-Soliton Mechanics
title_fullStr Spacetime Topology and the Laws of Black Hole-Soliton Mechanics
title_full_unstemmed Spacetime Topology and the Laws of Black Hole-Soliton Mechanics
title_short Spacetime Topology and the Laws of Black Hole-Soliton Mechanics
title_sort spacetime topology and the laws of black hole soliton mechanics
topic black holes in higher dimensions
supergravity
black hole thermodynamics
gravitational aspects of string theory
url http://www.mdpi.com/1099-4300/19/1/35
work_keys_str_mv AT harikkunduri spacetimetopologyandthelawsofblackholesolitonmechanics