Anisotropic scalar field emission from TeV scale black hole

dc.creatorIda, Daisuke
dc.creatorOda, Kin-ya
dc.creatorPark, Seong Chan
dc.date2005-01-24
dc.date.accessioned2026-07-07T03:54:19Z
dc.date.available2026-07-07T03:54:19Z
dc.descriptionBlack holes are predicted to be copiously produced at the CERN Large Hadron Collider in the scenarios of TeV scale gravity. We report recent progress in studying decay of such a higher dimensional black hole in D=4+n dimensions through the Hawking radiation into brane localized fields taking into account its angular momentum which is indispensable for realistic simulations. Presented is the greybody factors for a scalar field emission, which confirms our previous results in low energy approximation: (i) the existence of super-radiance modes and (ii) the non-trivial angular distribution of radiated scalar field. Phenomenological implications and future plans are discussed.
dc.description4 pages, 1 figure, Presented at the 14th Workshop on General Relativity and Gravitation,Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto, Japan, Nov.29-Dec.3 2004
dc.identifierhttps://arxiv.org/abs/hep-ph/0501210
dc.identifierhttp://arxiv.org/abs/hep-ph/0501210
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/44187
dc.subjectHigh Energy Physics - Phenomenology
dc.titleAnisotropic scalar field emission from TeV scale black hole
dc.typetext

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