Are Bulk Axions in Models with Extra, Large, Compact Dimensions Observable?

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dc.creatorNussinov, Shmuel
dc.date2004-06-22
dc.date.accessioned2026-07-07T03:52:43Z
dc.date.available2026-07-07T03:52:43Z
dc.descriptionThe high degeneracy of KK modes in models which have bulk axions moving in some extra, compact dimensions which are larger than O (Angstrom)strongly tightens the supernova upper bounds on the axion photon coupling making axions practically unobservable. Conversely, discovering axions directly or indirectly will exclude such models. These drastic conclusions are avoided if the supernova and bounds from solar axion searches are relaxed.
dc.description7 pages; cross-reference with Astrophysics
dc.identifierhttps://arxiv.org/abs/hep-ph/0406244
dc.identifierhttp://arxiv.org/abs/hep-ph/0406244
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/43570
dc.subjectHigh Energy Physics - Phenomenology
dc.titleAre Bulk Axions in Models with Extra, Large, Compact Dimensions Observable?
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