AREA SPECTRUM OF THE D-DIMENSIONAL DE SITTER SPACETIME
The determination of the quantum area spectrum of a black hole horizon by means of its asymptotic quasinormal frequencies has been explored recently. We believe that for D-dimensional de Sitter horizon we must study if the idea works. Thus taking into account the local description of the thermodynam...
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2009 |
| País: | México |
| Institución: | Instituto Politécnico Nacional |
| Repositorio: | Repositorio Digital del IPN |
| OAI Identifier: | oai:www.repositoriodigital.ipn.mx:123456789/11313 |
| Acceso en línea: | http://hdl.handle.net/123456789/827 http://www.repositoriodigital.ipn.mx/handle/123456789/11313 |
| Access Level: | acceso abierto |
| Palabra clave: | AREA SPECTRUM Quasinormal modes DE SITTER HORIZON BEKENSTEIN-HAWKING ENTROPY |
| Sumario: | The determination of the quantum area spectrum of a black hole horizon by means of its asymptotic quasinormal frequencies has been explored recently. We believe that for D-dimensional de Sitter horizon we must study if the idea works. Thus taking into account the local description of the thermodynamics of horizons proposed by Padmanabhan and the results of Hod, Kunstatter, and Maggiore we study the area spectrum of the D-dimensional de Sitter horizon. |
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