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| DOI | 10.1007/S10509-012-1333-X | ||||
| Año | 2013 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
In this work we study the null geodesics in the background of Reissner-Nordstrom Anti de Sitter black hole. We compute the exact trajectories in terms of Weierstrass elliptic functions, obtaining a detailed description of the orbits in terms of the charge, mass and the cosmological constant. The trajectories of the photon are classified using the impact parameter.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | VILLANUEVA-LOBOS, JOSE RICARDO | Hombre |
Universidad de Tarapacá - Chile
|
| 2 | SAAVEDRA-ALVEAR, JOEL FRANCISCO | Hombre |
Pontificia Universidad Católica de Valparaíso - Chile
|
| 3 | Olivares, Marco | Hombre |
Pontificia Universidad Católica de Valparaíso - Chile
|
| 4 | Cruz, Norman | Hombre |
Universidad de Santiago de Chile - Chile
|
| Fuente |
|---|
| CONICYT |
| Universidad de Tarapacá |
| PUCV |
| Fondo Nacional de Desarrollo Científico y Tecnológico |
| Comisión Nacional de Investigación Científica y Tecnológica |
| Pontificia Universidad Católica de Valparaíso |
| Comision Nacional de Ciencias y Tecnologia through FONDECYT |
| PUCV through Proyecto DI Postdoctorado |
| COMISION NA-CIONAL DE CIENCIAS Y TECNOLOGIA |
| Agradecimiento |
|---|
| We are grateful to Prof. Gary Gibbons for his enlightening comments. J.S. was supported by COMISION NACIONAL DE CIENCIAS Y TECNOLOGIA through FONDECYT Grant 1110076, 1090613 and 1110230. Also J.S. work was partially supported by PUCV DI-123.713/2011. N.C. acknowledges the support to this research by CONICYT through Grant No. 1110840. M.O. and J.V. acknowledge the hospitality of the Physics Department of Universidad de Santiago de Chile. M.O. was supported by PUCV through Proyecto DI Postdoctorado 2011. J.V. was supported by Universidad de Tarapaca Grant 4720-11. |
| Acknowledgements We are grateful to Prof. Gary Gibbons for his enlightening comments. J.S. was supported by COMISION NA-CIONAL DE CIENCIAS Y TECNOLOGIA through FONDECYT Grant 1110076, 1090613 and 1110230. Also J.S. work was partially supported by PUCV DI-123.713/2011. N.C. acknowledges the support to this research by CONICYT through Grant No. 1110840. M.O. and J.V. acknowledge the hospitality of the Physics Department of Univer-sidad de Santiago de Chile. M.O. was supported by PUCV through Proyecto DI Postdoctorado 2011. J.V. was supported by Universidad de Tarapacá Grant 4720-11. |