Growing neutrino cosmology

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dc.creatorWetterich, Christof
dc.creatorPettorino, Valeria
dc.date2009-05-05
dc.date.accessioned2026-07-07T13:12:08Z
dc.date.available2026-07-07T13:12:08Z
dc.descriptionIn growing neutrino models, the neutrino mass increases in time and stops the dynamical evolution of a dark energy scalar field, thus explaining the 'why now' problem. A new attractive force, mediated by the 'cosmon' scalar field, makes non relativistic neutrino form lumps on the scales of superclusters and beyond. Nonlinear neutrino lumps are predicted to form at redshift z ~ 1 and, if observed, could be an indication for a new attractive force stronger than gravity.
dc.descriptionTo appear in the proceedings of the XIII International Workshop on Neutrino Telescopes, Venice 2009
dc.identifierhttps://arxiv.org/abs/0905.0715
dc.identifierhttp://arxiv.org/abs/0905.0715
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/229496
dc.subjectCosmology and Nongalactic Astrophysics
dc.titleGrowing neutrino cosmology
dc.typetext

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