Calculable Corrections to Brane Black Hole Decay I: The Scalar Case
In the context of brane-world theories, the production cross-section for black holes may be greatly enhanced. Such black holes can in principle lead to detectable signals via their Hawking evaporation to brane-localized modes. We calculate, in the semiclassical approximation, the leading corrections...
| Main Authors: | , |
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| Format: | Journal article |
| Jezik: | English |
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2002
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| _version_ | 1826259598187692032 |
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| author | Kanti, P March-Russell, J |
| author_facet | Kanti, P March-Russell, J |
| author_sort | Kanti, P |
| collection | OXFORD |
| description | In the context of brane-world theories, the production cross-section for black holes may be greatly enhanced. Such black holes can in principle lead to detectable signals via their Hawking evaporation to brane-localized modes. We calculate, in the semiclassical approximation, the leading corrections to the energy spectrum (the greybody factors) for decay into scalar fields, as a function of the number of toroidally compactified extra dimensions, and partial wave number. |
| first_indexed | 2024-03-06T18:52:23Z |
| format | Journal article |
| id | oxford-uuid:10b084ef-a9a4-4924-b58c-32609fe5799b |
| institution | University of Oxford |
| language | English |
| last_indexed | 2024-03-06T18:52:23Z |
| publishDate | 2002 |
| record_format | dspace |
| spelling | oxford-uuid:10b084ef-a9a4-4924-b58c-32609fe5799b2022-03-26T09:57:48ZCalculable Corrections to Brane Black Hole Decay I: The Scalar CaseJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:10b084ef-a9a4-4924-b58c-32609fe5799bEnglishSymplectic Elements at Oxford2002Kanti, PMarch-Russell, JIn the context of brane-world theories, the production cross-section for black holes may be greatly enhanced. Such black holes can in principle lead to detectable signals via their Hawking evaporation to brane-localized modes. We calculate, in the semiclassical approximation, the leading corrections to the energy spectrum (the greybody factors) for decay into scalar fields, as a function of the number of toroidally compactified extra dimensions, and partial wave number. |
| spellingShingle | Kanti, P March-Russell, J Calculable Corrections to Brane Black Hole Decay I: The Scalar Case |
| title | Calculable Corrections to Brane Black Hole Decay I: The Scalar Case |
| title_full | Calculable Corrections to Brane Black Hole Decay I: The Scalar Case |
| title_fullStr | Calculable Corrections to Brane Black Hole Decay I: The Scalar Case |
| title_full_unstemmed | Calculable Corrections to Brane Black Hole Decay I: The Scalar Case |
| title_short | Calculable Corrections to Brane Black Hole Decay I: The Scalar Case |
| title_sort | calculable corrections to brane black hole decay i the scalar case |
| work_keys_str_mv | AT kantip calculablecorrectionstobraneblackholedecayithescalarcase AT marchrussellj calculablecorrectionstobraneblackholedecayithescalarcase |