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https://olympias.lib.uoi.gr/jspui/handle/123456789/17203Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Creek, S. | en |
| dc.contributor.author | Efthimiou, O. | en |
| dc.contributor.author | Kanti, P. | en |
| dc.contributor.author | Tamvakis, K. | en |
| dc.date.accessioned | 2015-11-24T18:37:43Z | - |
| dc.date.available | 2015-11-24T18:37:43Z | - |
| dc.identifier.issn | 0370-2693 | - |
| dc.identifier.uri | https://olympias.lib.uoi.gr/jspui/handle/123456789/17203 | - |
| dc.rights | Default Licence | - |
| dc.subject | hawking radiation | en |
| dc.subject | absorption | en |
| dc.subject | brane | en |
| dc.subject | dimensions | en |
| dc.subject | superradiance | en |
| dc.subject | graviton | en |
| dc.subject | waves | en |
| dc.subject | space | en |
| dc.subject | tev | en |
| dc.title | Scalar emission in the bulk in a rotating black hole background | en |
| heal.type | journalArticle | - |
| heal.type.en | Journal article | en |
| heal.type.el | Άρθρο Περιοδικού | el |
| heal.identifier.primary | DOI 10.1016/j.physletb.2007.09.050 | - |
| heal.identifier.secondary | <Go to ISI>://000251292300017 | - |
| heal.identifier.secondary | http://ac.els-cdn.com/S0370269307011434/1-s2.0-S0370269307011434-main.pdf?_tid=9093d6c351fa61a6a13da26f679cac16&acdnat=1334232002_af838c9368b6f74efb0ee006eaaf8397 | - |
| heal.language | en | - |
| heal.access | campus | - |
| heal.recordProvider | Πανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιών | el |
| heal.publicationDate | 2007 | - |
| heal.abstract | We 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.journalName | Physics Letters B | en |
| heal.journalType | peer reviewed | - |
| heal.fullTextAvailability | TRUE | - |
| Appears in Collections: | Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά) - ΦΥΣ | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| Creek-2007-Scalar emission in t.pdf | 404.42 kB | Adobe PDF | View/Open |
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