Graviton Cosmology in Universal Extra Dimensions

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dc.creatorFeng, Jonathan L.
dc.creatorRajaraman, Arvind
dc.creatorTakayama, Fumihiro
dc.date2003-07-31
dc.date.accessioned2026-07-07T11:09:25Z
dc.date.available2026-07-07T11:09:25Z
dc.descriptionIn models of universal extra dimensions, gravity and all standard model fields propagate in the extra dimensions. Previous studies of such models have concentrated on the Kaluza-Klein (KK) partners of standard model particles. Here we determine the properties of the KK gravitons and explore their cosmological implications. We find the lifetimes of decays to KK gravitons, of relevance for the viability of KK gravitons as dark matter. We then discuss the primordial production of KK gravitons after reheating. The existence of a tower of KK graviton states makes such production extremely efficient: for reheat temperature T_RH and d extra dimensions, the energy density stored in gravitons scales as T_RH^{2+3d/2}. Overclosure and Big Bang nucleosynthesis therefore stringently constrain T_RH in all universal extra dimension scenarios. At the same time, there is a window of reheat temperatures low enough to avoid these constraints and high enough to generate the desired thermal relic density for KK WIMP and superWIMP dark matter.
dc.description19 pages, 1 figure
dc.identifierhttps://arxiv.org/abs/hep-ph/0307375
dc.identifierhttp://arxiv.org/abs/hep-ph/0307375
dc.identifierPhys.Rev.D68:085018,2003
dc.identifierdoi:10.1103/PhysRevD.68.085018
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/190462
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleGraviton Cosmology in Universal Extra Dimensions
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