Enhancement of Dark Matter Abundance in Scalar-Tensor Dark Energy

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dc.creatorCatena, R.
dc.creatorFornengo, N.
dc.creatorMasiero, A.
dc.creatorPietroni, M.
dc.creatorRosati, F.
dc.date2004-06-07
dc.date.accessioned2026-07-07T02:13:26Z
dc.date.available2026-07-07T02:13:26Z
dc.descriptionIn Scalar-Tensor theories of gravity, the expansion rate of the universe in the past may differ considerably from the standard one. After imposing the constraints coming from nucleosynthesis, CMB, type Ia supernovae, and solar system tests of General Relativity, we consider the expansion rate of the universe at WIMP decoupling, showing that it can lead to an enhancement of the dark matter relic density of some orders of magnitude with respect to the standard case. This effect may have a deep impact on most popular candidates for dark matter, as the supersymmetric neutralino.
dc.description4 pages, 2 figures, Talk presented at 39th Rencontres de Moriond, "Exploring the Universe," La Thuile, Italy, March 28 - April 4, 2004
dc.identifierhttps://arxiv.org/abs/astro-ph/0406152
dc.identifierhttp://arxiv.org/abs/astro-ph/0406152
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7815
dc.subjectAstrophysics
dc.titleEnhancement of Dark Matter Abundance in Scalar-Tensor Dark Energy
dc.typetext

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