Black holes in anti-de Sitter (AdS) spacetime
The space-time metric AdS will be determined and based on it the cosmological constant will be calculated as a function of the radius of the space AdS, using this cosmological constant the Einstein equations will be solved in order to find a metric based on from the radial coordinate of the event ho...
| Autores: | , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2022 |
| País: | Perú |
| Institución: | Universidad Nacional Mayor de San Marcos |
| Repositorio: | Revistas - Universidad Nacional Mayor de San Marcos |
| Idioma: | español |
| OAI Identifier: | oai:revistasinvestigacion.unmsm.edu.pe:article/21966 |
| Acceso en línea: | https://revistasinvestigacion.unmsm.edu.pe/index.php/fisica/article/view/21966 |
| Access Level: | acceso abierto |
| Palabra clave: | Black holes anti de Sitter Hawking temperature Relatividad general gravedad f(R) ecuaciones de Friedmann |
| Sumario: | The space-time metric AdS will be determined and based on it the cosmological constant will be calculated as a function of the radius of the space AdS, using this cosmological constant the Einstein equations will be solved in order to find a metric based on from the radial coordinate of the event horizon, then some thermodynamic properties of black holes in spacetime AdS such as temperature, area and entropy will be calculated. |
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