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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...
Autores principales: | , |
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Lenguaje: | eng |
Publicado: |
1999
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1088/0264-9381/17/7/302 http://cds.cern.ch/record/398717 |
_version_ | 1780894028184682496 |
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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. |
id | cern-398717 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1999 |
record_format | invenio |
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 |