Scalar emission in the bulk in a rotating black hole background

dc.contributor.authorCreek, S.en
dc.contributor.authorEfthimiou, O.en
dc.contributor.authorKanti, P.en
dc.contributor.authorTamvakis, K.en
dc.date.accessioned2015-11-24T18:37:43Z
dc.date.available2015-11-24T18:37:43Z
dc.identifier.issn0370-2693-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/17203
dc.rightsDefault Licence-
dc.subjecthawking radiationen
dc.subjectabsorptionen
dc.subjectbraneen
dc.subjectdimensionsen
dc.subjectsuperradianceen
dc.subjectgravitonen
dc.subjectwavesen
dc.subjectspaceen
dc.subjectteven
dc.titleScalar emission in the bulk in a rotating black hole backgrounden
heal.abstractWe study the emission of scalars into the bulk from a higher-dimensional rotating black hole. We obtain an analytic solution to the field equation by employing matching techniques on expressions valid in the near-horizon and far-field regimes. Both analytic and numerical results for the absorption probability, in the low-energy and low-angular momentum limit, are derived and found to be in excellent agreement. We also compute the energy emission rate, and show that the brane-to-bulk ratio of the energy emission rates for scalar fields remains always larger than unity in the aforementioned regime. (c) 2007 Elsevier B.V. All rights reserved.en
heal.accesscampus-
heal.fullTextAvailabilityTRUE-
heal.identifier.primaryDOI 10.1016/j.physletb.2007.09.050-
heal.identifier.secondary<Go to ISI>://000251292300017-
heal.identifier.secondaryhttp://ac.els-cdn.com/S0370269307011434/1-s2.0-S0370269307011434-main.pdf?_tid=9093d6c351fa61a6a13da26f679cac16&acdnat=1334232002_af838c9368b6f74efb0ee006eaaf8397-
heal.journalNamePhysics Letters Ben
heal.journalTypepeer reviewed-
heal.languageen-
heal.publicationDate2007-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.typejournalArticle-
heal.type.elΆρθρο Περιοδικούel
heal.type.enJournal articleen

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