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Large N limit of extremal non-supersymmetric black holes
The large N limit of extremal non-supersymmetric Type-I five-dimensional string black holes is studied from the point of view of D-branes. We find that the agreement between the D-brane and the black hole picture is due to an asymptotic restoration of supersymmetry in the large N limit in which both...
Autores principales: | , , |
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Lenguaje: | eng |
Publicado: |
1998
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/S0550-3213(98)00554-9 http://cds.cern.ch/record/355601 |
_version_ | 1780892496461561856 |
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author | Barbon, J.L.F. Manes, J.L. Vazquez-Mozo, M.A. |
author_facet | Barbon, J.L.F. Manes, J.L. Vazquez-Mozo, M.A. |
author_sort | Barbon, J.L.F. |
collection | CERN |
description | The large N limit of extremal non-supersymmetric Type-I five-dimensional string black holes is studied from the point of view of D-branes. We find that the agreement between the D-brane and the black hole picture is due to an asymptotic restoration of supersymmetry in the large N limit in which both pictures are compared. In that limit Type-I string perturbation theory is effectively embedded into a Type-IIB perturbation theory with unbroken supersymmetric charges whose presence guarantees the non-renormalization of mass and entropy as the effective couplings are increased. In this vein, we also study the near-horizon geometry of the Type-I black hole using D5-brane probes to find that the low energy effective action for the probe is identical to the corresponding one in the auxiliary Type-IIB theory in the large N limit. |
id | cern-355601 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1998 |
record_format | invenio |
spelling | cern-3556012022-06-24T03:03:00Zdoi:10.1016/S0550-3213(98)00554-9http://cds.cern.ch/record/355601engBarbon, J.L.F.Manes, J.L.Vazquez-Mozo, M.A.Large N limit of extremal non-supersymmetric black holesParticle Physics - TheoryThe large N limit of extremal non-supersymmetric Type-I five-dimensional string black holes is studied from the point of view of D-branes. We find that the agreement between the D-brane and the black hole picture is due to an asymptotic restoration of supersymmetry in the large N limit in which both pictures are compared. In that limit Type-I string perturbation theory is effectively embedded into a Type-IIB perturbation theory with unbroken supersymmetric charges whose presence guarantees the non-renormalization of mass and entropy as the effective couplings are increased. In this vein, we also study the near-horizon geometry of the Type-I black hole using D5-brane probes to find that the low energy effective action for the probe is identical to the corresponding one in the auxiliary Type-IIB theory in the large N limit.The large N limit of extremal non-supersymmetric Type-I five-dimensional string black holes is studied from the point of view of D-branes. We find that the agreement between the D-brane and the black-hole picture is due to an asymptotic restoration of supersymmetry in the large $N$ limit in which both pictures are compared. In that limit Type-I string perturbation theory is effectively embedded into a Type-IIB perturbation theory with unbroken supersymmetric charges whose presence guarantees the non-renormalization of mass and entropy as the effective couplings are increased. In this vein, we also study the near-horizon geometry of the Type-I black hole using D5-brane probes to find that the low energy effective action for the probe is identical to the corresponding one in the auxiliary Type-IIB theory in the large N limit.The large N limit of extremal non-supersymmetric Type-I five-dimensional string black holes is studied from the point of view of D-branes. We find that the agreement between the D-brane and the black-hole picture is due to an asymptotic restoration of supersymmetry in the large N limit in which both pictures are compared. In that limit Type-I string perturbation theory is effectively embedded into a Type-IIB perturbation theory with unbroken supersymmetric charges whose presence guarantees the non-renormalization of mass and entropy as the effective couplings are increased. In this vein, we also study the near-horizon geometry of the Type-I black hole using D5-brane probes to find that the low-energy effective action for the probe is identical to the corresponding one in the auxiliary Type-IIB theory in the large N limit.hep-th/9805154CERN-TH-98-158EHU-FT-9804CERN-TH-98-158EHU-FT-98-04oai:cds.cern.ch:3556011998-05-26 |
spellingShingle | Particle Physics - Theory Barbon, J.L.F. Manes, J.L. Vazquez-Mozo, M.A. Large N limit of extremal non-supersymmetric black holes |
title | Large N limit of extremal non-supersymmetric black holes |
title_full | Large N limit of extremal non-supersymmetric black holes |
title_fullStr | Large N limit of extremal non-supersymmetric black holes |
title_full_unstemmed | Large N limit of extremal non-supersymmetric black holes |
title_short | Large N limit of extremal non-supersymmetric black holes |
title_sort | large n limit of extremal non-supersymmetric black holes |
topic | Particle Physics - Theory |
url | https://dx.doi.org/10.1016/S0550-3213(98)00554-9 http://cds.cern.ch/record/355601 |
work_keys_str_mv | AT barbonjlf largenlimitofextremalnonsupersymmetricblackholes AT manesjl largenlimitofextremalnonsupersymmetricblackholes AT vazquezmozoma largenlimitofextremalnonsupersymmetricblackholes |