Primordial Nucleosynthesis with a Decaying Tau Neutrino

dc.creatorDodelson, S.
dc.creatorGyuk, G.
dc.creatorTurner, M. S.
dc.date1993-12-28
dc.date.accessioned2026-07-07T10:34:49Z
dc.date.available2026-07-07T10:34:49Z
dc.descriptionA comprehensive study of the effect of an unstable tau neutrino on primordial nucleosynthesis is presented. The standard code for nucleosynthesis is modified to allow for a massive decaying tau neutrino whose daughter products include neutrinos, photons, $e^\pm$ pairs, and/or noninteracting (sterile) daughter products. Tau-neutrino decays influence primordial nucleosynthesis in three distinct ways: (i) the energy density of the decaying tau neutrino and its daughter products affect the expansion rate tending to increase $^4$He, D, and $^3$He production; (ii) electromagnetic (EM) decay products heat the EM plasma and dilute the baryon-to-photon ratio tending to decrease $^4$He production and increase D and $^3$He production; and (iii) electron neutrinos and antineutrinos produced by tau-neutrino decays increase the weak rates that govern the neutron-to-proton ratio, leading to decreased $^4$He production for short lifetimes ($\la 30\sec$) and masses less than about $10\MeV$ and increased $^4$He production for long lifetimes or large masses. The precise effect of a decaying tau neutrino on the yields of primordial nucleosynthesis and the mass-lifetime limits that follow depend crucially upon decay mode. We identify four generic decay modes that serve to bracket the wider range of possibilities:
dc.description27 pages, Latex, 12 Figures avaiable on request, FNAL--Pub--93/236-A
dc.identifierhttps://arxiv.org/abs/astro-ph/9312062
dc.identifierhttp://arxiv.org/abs/astro-ph/9312062
dc.identifierPhys.Rev.D49:5068-5079,1994
dc.identifierdoi:10.1103/PhysRevD.49.5068
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179565
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titlePrimordial Nucleosynthesis with a Decaying Tau Neutrino
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