Response to Comments on "Neutrino Flavor Evolution Near a Supernova's Core"

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dc.creatorPantaleone, J.
dc.date1994-08-01
dc.date.accessioned2026-07-07T02:19:20Z
dc.date.available2026-07-07T02:19:20Z
dc.descriptionIn a recent paper I concluded that the neutrino background is important for calculating neutrino flavor evolution in supernovae, and including it weakens the connection between r-process nucleosynthesis and cosmologically relevant neutrino masses. Comments on this paper have been posted to this bulletin board; one by J. Cline and the other by Y.Z. Qian and G.M. Fuller. Here I briefly discuss these Comments and demonstrate that they are inaccurate and ill-considered. No corrections to my paper are necessary.
dc.description4 pages, LATEX, IUHET-282
dc.identifierhttps://arxiv.org/abs/astro-ph/9408006
dc.identifierhttp://arxiv.org/abs/astro-ph/9408006
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9822
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleResponse to Comments on "Neutrino Flavor Evolution Near a Supernova's Core"
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