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Infinitely Coloured Black Holes

We formulate the field equations for $SU(\infty)$ Einstein-Yang-Mills theory, and find spherically symmetric black-hole solutions. This model may be motivated by string theory considerations, given the enormous gauge symmetries which characterize string theory. The solutions simplify considerably in...

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Detalles Bibliográficos
Autores principales: Mavromatos, Nick E., Winstanley, Elizabeth
Lenguaje:eng
Publicado: 1999
Materias:
Acceso en línea:https://dx.doi.org/10.1088/0264-9381/17/7/302
http://cds.cern.ch/record/398717
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author Mavromatos, Nick E.
Winstanley, Elizabeth
author_facet Mavromatos, Nick E.
Winstanley, Elizabeth
author_sort Mavromatos, Nick E.
collection CERN
description We formulate the field equations for $SU(\infty)$ Einstein-Yang-Mills theory, and find spherically symmetric black-hole solutions. This model may be motivated by string theory considerations, given the enormous gauge symmetries which characterize string theory. The solutions simplify considerably in the presence of a negative cosmological constant, particularly for the limiting cases of a very large cosmological constant or very small gauge field. The situation of an arbitrarily small gauge field is relevant for holography and we comment on the AdS/CFT conjecture in this light. The black holes possess infinite amounts of gauge field hair, and we speculate on possible consequences of this for quantum decoherence, which, however, we do not tackle here.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1999
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spelling cern-3987172021-10-08T02:23:27Zdoi:10.1088/0264-9381/17/7/302http://cds.cern.ch/record/398717engMavromatos, Nick E.Winstanley, ElizabethInfinitely Coloured Black HolesParticle Physics - TheoryWe formulate the field equations for $SU(\infty)$ Einstein-Yang-Mills theory, and find spherically symmetric black-hole solutions. This model may be motivated by string theory considerations, given the enormous gauge symmetries which characterize string theory. The solutions simplify considerably in the presence of a negative cosmological constant, particularly for the limiting cases of a very large cosmological constant or very small gauge field. The situation of an arbitrarily small gauge field is relevant for holography and we comment on the AdS/CFT conjecture in this light. The black holes possess infinite amounts of gauge field hair, and we speculate on possible consequences of this for quantum decoherence, which, however, we do not tackle here.We formulate the field equations for $SU(\infty)$ Einstein-Yang-Mills theory, and find spherically symmetric black-hole solutions. This model may be motivated by string theory considerations, given the enormous gauge symmetries which characterize string theory. The solutions simplify considerably in the presence of a negative cosmological constant, particularly for the limiting cases of a very large cosmological constant or very small gauge field. The situation of an arbitrarily small gauge field is relevant for holography and we comment on the AdS/CFT conjecture in this light. The black holes possess infinite amounts of gauge field hair, and we speculate on possible consequences of this for quantum decoherence, which, however, we do not tackle here.hep-th/9909018OUTP-99-41POUTP-99-41-Poai:cds.cern.ch:3987171999-09-06
spellingShingle Particle Physics - Theory
Mavromatos, Nick E.
Winstanley, Elizabeth
Infinitely Coloured Black Holes
title Infinitely Coloured Black Holes
title_full Infinitely Coloured Black Holes
title_fullStr Infinitely Coloured Black Holes
title_full_unstemmed Infinitely Coloured Black Holes
title_short Infinitely Coloured Black Holes
title_sort infinitely coloured black holes
topic Particle Physics - Theory
url https://dx.doi.org/10.1088/0264-9381/17/7/302
http://cds.cern.ch/record/398717
work_keys_str_mv AT mavromatosnicke infinitelycolouredblackholes
AT winstanleyelizabeth infinitelycolouredblackholes