Non Thermal Features in the Cosmic Neutrino Background

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dc.creatorMangano, G.
dc.date2006-03-22
dc.date.accessioned2026-07-07T07:01:14Z
dc.date.available2026-07-07T07:01:14Z
dc.descriptionI review some of the basic information on the Cosmic Neutrino Background momentum distribution. In particular, I discuss how present data from several cosmological observables such as Big Bang Nucleosynthesis, Cosmic Microwave Background and Large Scale Structure power spectrum constrain possible deviations from a standard Fermi-Dirac thermal distribution.
dc.descriptionTalk given at "Neutrino Oscillations in Venice" Conference, Venice, February 7-10 2006
dc.identifierhttps://arxiv.org/abs/astro-ph/0603603
dc.identifierhttp://arxiv.org/abs/astro-ph/0603603
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/108214
dc.subjectAstrophysics
dc.titleNon Thermal Features in the Cosmic Neutrino Background
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