Relic neutrino clustering and implications for their detection

dc.creatorRingwald, Andreas
dc.creatorWong, Yvonne Y. Y.
dc.date2004-12-17
dc.date.accessioned2026-07-07T03:54:07Z
dc.date.available2026-07-07T03:54:07Z
dc.descriptionWe study the gravitational clustering of big bang relic neutrinos onto existing cold dark matter and baryonic structures within the flat $Λ$CDM model. We then discuss the implications of clustering for scattering-based relic neutrino detection methods, ranging from flux detection via Cavendish-type torsion balances, to target detection using accelerator beams and cosmic rays.
dc.description15 pages, 5 figures, talk given at DARK2004, College Station TX, Oct 2004
dc.identifierhttps://arxiv.org/abs/hep-ph/0412256
dc.identifierhttp://arxiv.org/abs/hep-ph/0412256
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/44108
dc.subjectHigh Energy Physics - Phenomenology
dc.titleRelic neutrino clustering and implications for their detection
dc.typetext

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