Gravitational energy and radiation of a charged black hole
We analyze the energy configuration of a charged black hole in the TeleparallelFramework of General Relativity. We obtain the energy-momentum tensor of the gravitationalfield in a stationary frame, and we calculate its contribution to the total energyof the system. We study the same gravitational fi...
| Autores: | , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2017 |
| País: | Argentina |
| Institución: | Consejo Nacional de Investigaciones Científicas y Técnicas |
| Repositorio: | CONICET Digital (CONICET) |
| Idioma: | inglés |
| OAI Identifier: | oai:ri.conicet.gov.ar:11336/35353 |
| Acceso en línea: | http://hdl.handle.net/11336/35353 |
| Access Level: | acceso abierto |
| Palabra clave: | Gravitational fields General Relativity Blacks holes https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| Sumario: | We analyze the energy configuration of a charged black hole in the TeleparallelFramework of General Relativity. We obtain the energy-momentum tensor of the gravitationalfield in a stationary frame, and we calculate its contribution to the total energyof the system. We study the same gravitational field measured by an accelerated frameand we analyze how the energy-momentum tensor is transformed. We found that in theaccelerated frame, a Poyinting-like flux appears for the gravitational field but not for theelectromagnetic field. |
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