Hawking radiation for higher dimensional Einstein-Yang-Mills linear dilaton black holes

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dc.creatorMazharimousavi, S. Habib
dc.creatorSakalli, I.
dc.creatorHalilsoy, M.
dc.date2008-08-01
dc.date.accessioned2026-07-07T12:38:43Z
dc.date.available2026-07-07T12:38:43Z
dc.descriptionRecently, Hawking radiation from a $4-$dimensional linear dilaton black hole solution to Einstein-Maxwell-Dilaton (EMD) theory, via a method of computing exactly the semi-classical radiation, has been derived by Cl\U{e9}ment, et al. Their results show that, whenever solution is available to the massless scalar wave equation, an exact computation of the radiation spectrum leads to the Hawking temperature $T_{H}$. We apply the same method to derive Hawking radiation spectrum for higher dimensional linear dilaton black holes in the Einstein-Yang-Mills-Dilaton (EYMD) and Einstein-Maxwell-Dilaton (EMD) theories. Our results show that the radiation with high frequencies for these massive black holes reveal some remarkable information about the $T_{H}$.
dc.description9 pages, 2 figures,
dc.identifierhttps://arxiv.org/abs/0808.0107
dc.identifierhttp://arxiv.org/abs/0808.0107
dc.identifierPhysics Letters B 672 (2009) 177
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/218857
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleHawking radiation for higher dimensional Einstein-Yang-Mills linear dilaton black holes
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