Time like geodesics for five-dimensional Schwarzschild and Reissner-Nordstrom anti-de Sitter black holes

dc.contributor.authorGonzalez P. A.
dc.contributor.authorOlivares Marco
dc.contributor.authorVasquez Yerko
dc.contributor.authorVillanueva J. R.
dc.date.accessioned2025-05-19T16:37:49Z
dc.date.available2025-05-19T16:37:49Z
dc.date.issued2023/09/23
dc.description.abstractThe time like structure of the five-dimensional Schwarzschild and Reissner-Nordstrom anti-de Sitter black holes is studied in detail. Different kinds of motion are allowed and studied by using an adequate effective potential. Then, by solving the corresponding equations of motion, several trajectories and orbits are described in terms of Weierstra ss elliptic functions and elementary functions for neutral particles.
dc.identifier.doihttp://dx.doi.org/10.1140/epjc/s10052-023-12018-4
dc.identifier.issn1434-6044
dc.identifier.urihttps://publicacionesabiertas.userena.cl/handle/123456789/210
dc.languageEnglish
dc.publisherSPRINGER
dc.subjectNULL GEODESICS, MOTION, FIELD, SPACE
dc.titleTime like geodesics for five-dimensional Schwarzschild and Reissner-Nordstrom anti-de Sitter black holes
dc.typeArticle

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