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dc.contributor | Universitat de Barcelona |
---|---|
dc.contributor.author | Emparan García de Salazar, Roberto A. |
dc.contributor.author | Tanabe, Kentaro |
dc.date | 2019-04-05T13:54:13Z |
dc.date | 2019-04-05T13:54:13Z |
dc.date | 2014-03-11 |
dc.date | 2019-04-05T13:54:13Z |
dc.identifier.citation | 1550-7998 |
dc.identifier.citation | 636236 |
dc.identifier.uri | http://hdl.handle.net/2445/131681 |
dc.description.abstract | We show that in the limit where the number of spacetime dimensions D grows to infinity a very large class of black holes (including nonextremal, static, asymptotically flat ones, with any number of gauge-field charges, possibly coupled to dilatons) possess a universal set of quasinormal modes whose complex frequencies depend only on the horizon radius and no other black hole parameters. The damping ratio of these modes vanishes like D − 2 / 3 , so they are almost normal modes, or "quasiparticle" excitations of the black hole. The structure responsible for the existence of these modes at large D is also present very generally in other black holes. |
dc.format | 4 p. |
dc.format | application/pdf |
dc.language.iso | eng |
dc.publisher | American Physical Society |
dc.relation | Reproducció del document publicat a: https://doi.org/10.1103/PhysRevD.89.064028 |
dc.relation | Physical Review D, 2014, vol. 89, num. 6, p. 064028 |
dc.relation | https://doi.org/10.1103/PhysRevD.89.064028 |
dc.rights | (c) American Physical Society, 2014 |
dc.rights | info:eu-repo/semantics/openAccess |
dc.subject | Forats negres (Astronomia) |
dc.subject | Cosmologia |
dc.subject | Espai i temps |
dc.subject | Black holes (Astronomy) |
dc.subject | Cosmology |
dc.subject | Space and time |
dc.title | Universal quasinormal modes of black holes in the limit of large number of dimensions |
dc.type | info:eu-repo/semantics/article |
dc.type | info:eu-repo/semantics/publishedVersion |