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https://olympias.lib.uoi.gr/jspui/handle/123456789/16066Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Kanti, P. | en |
| dc.contributor.author | Kodama, H. | en |
| dc.contributor.author | Konoplya, R. A. | en |
| dc.contributor.author | Pappas, N. | en |
| dc.contributor.author | Zhdenko, A. | en |
| dc.date.accessioned | 2015-11-24T18:27:38Z | - |
| dc.date.available | 2015-11-24T18:27:38Z | - |
| dc.identifier.issn | 1550-7998 | - |
| dc.identifier.uri | https://olympias.lib.uoi.gr/jspui/handle/123456789/16066 | - |
| dc.rights | Default Licence | - |
| dc.subject | absorption cross-section | en |
| dc.subject | hawking radiation | en |
| dc.subject | higher dimensions | en |
| dc.subject | brane | en |
| dc.subject | perturbations | en |
| dc.subject | superradiance | en |
| dc.subject | scalar | en |
| dc.subject | tev | en |
| dc.subject | millimeter | en |
| dc.subject | hierarchy | en |
| dc.title | Graviton emission in the bulk by a simply rotating black hole | en |
| heal.type | journalArticle | - |
| heal.type.en | Journal article | en |
| heal.type.el | Άρθρο Περιοδικού | el |
| heal.identifier.primary | Doi 10.1103/Physrevd.80.084016 | - |
| heal.identifier.secondary | <Go to ISI>://000271353700065 | - |
| heal.identifier.secondary | http://prd.aps.org/abstract/PRD/v80/i8/e084016 | - |
| heal.language | en | - |
| heal.access | campus | - |
| heal.recordProvider | Πανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιών | el |
| heal.publicationDate | 2009 | - |
| heal.abstract | In this work, we study the emission of tensor-type gravitational degrees of freedom from a higher-dimensional, simply rotating black hole in the bulk. The decoupled radial part of the corresponding field equation is first solved analytically in the limit of low-energy emitted particles and low-angular momentum of the black hole in order to derive the absorption probability. Both the angular and radial equations are then solved numerically, and the comparison of the analytical and numerical results shows a very good agreement in the low and intermediate energy regimes. By using our exact, numerical results we compute the energy and angular-momentum emission rates and their dependence on the spacetime parameters such as the number of additional spacelike dimensions and the angular momentum of the black hole. Particular care is given to the convergence of our results in terms of the number of modes taken into account in the calculation and the multiplicity of graviton tensor modes that correspond to the same angular-momentum numbers. | en |
| heal.journalName | Physical Review D | en |
| heal.journalType | peer reviewed | - |
| heal.fullTextAvailability | TRUE | - |
| Appears in Collections: | Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά) | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| kanti-2009-Graviton emission in the bulk by a simply rotating black hole.pdf | 489.79 kB | Adobe PDF | View/Open |
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