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| 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 | 2015-11-24T18:27:37Z | - |
| dc.date.available | 2015-11-24T18:27:37Z | - |
| dc.identifier.issn | 1550-7998 | - |
| dc.identifier.uri | https://olympias.lib.uoi.gr/jspui/handle/123456789/16060 | - |
| dc.rights | Default Licence | - |
| dc.subject | absorption cross-section | en |
| dc.subject | large extra dimensions | en |
| dc.subject | hawking radiation | en |
| dc.subject | emission-spectra | en |
| dc.subject | angular-momentum | en |
| dc.subject | tev-gravity | en |
| dc.subject | lhc | en |
| dc.subject | waves | en |
| dc.subject | superradiance | en |
| dc.subject | scattering | en |
| dc.title | Greybody factors for brane scalar fields 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 10.1103/Physrevd.75.084043 | - |
| heal.identifier.secondary | <Go to ISI>://000246076900085 | - |
| heal.identifier.secondary | http://prd.aps.org/abstract/PRD/v75/i8/e084043 | - |
| 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 evaporation of (4 + n)-dimensional rotating black holes into scalar degrees of freedom on the brane. We calculate the corresponding absorption probabilities and cross sections obtaining analytic solutions in the low-energy regime and compare the derived analytic expressions to numerical results, with very good agreement. We then consider the high-energy regime, construct an analytic high-energy solution to the scalar-field equation by employing a new method, and calculate the absorption probability and cross section for this energy regime, finding again a very good agreement with the exact numerical results. We also determine the high-energy asymptotic value of the total cross section and compare it to the analytic results derived from the application of the geometrical optics limit. | en |
| heal.journalName | Physical Review D | en |
| heal.journalType | peer reviewed | - |
| heal.fullTextAvailability | TRUE | - |
| Appears in Collections: | Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά) | |
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