Phenomenology of the relic dilaton background

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dc.creatorGasperini, M.
dc.date2003-01-09
dc.date.accessioned2026-07-07T03:27:31Z
dc.date.available2026-07-07T03:27:31Z
dc.descriptionWe discuss the expected amplitude of a cosmic background of massive, non-relativistic dilatons, and we report recent results about its possible detection. This paper is a contracted version of a talk given at the 15th SIGRAV Conference on "General Relativity and Gravitational Physics" (Villa Mondragone, Roma, September 2002).
dc.description6 pages, latex, IOP style ecssm.sty included, to appear in Proc. of the 15th SIGRAV Conference on General Relativity and Gravitational Physics
dc.identifierhttps://arxiv.org/abs/gr-qc/0301032
dc.identifierhttp://arxiv.org/abs/gr-qc/0301032
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34459
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titlePhenomenology of the relic dilaton background
dc.typetext

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