Neutrinos from pre-supernova star

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dc.creatorOdrzywolek, A.
dc.creatorMisiaszek, M.
dc.creatorKutschera, M.
dc.date2004-05-01
dc.date.accessioned2026-07-07T02:13:03Z
dc.date.available2026-07-07T02:13:03Z
dc.descriptionAnalysis of the massive star properties during C, Ne, O and Si burning i.e. the neutrino-cooled stage, leads to the simplified neutrino emission model. In the framework of this model we have simulated spectrum of the antineutrinos. Flux normalized according to the massive star model with explicitly given neutrino luminosity allow us to predict signal produced in water Cherenkov detectors. The results are discussed from the point of view of the possibility of the core-collapse supernova event prediction in advance of a few days.
dc.description9 pages, 1 figure, talk presented at the Epiphany Conference on Astroparticle Physics, 8-11 January 2004, Cracow, Poland
dc.identifierhttps://arxiv.org/abs/astro-ph/0405006
dc.identifierhttp://arxiv.org/abs/astro-ph/0405006
dc.identifierActa Phys.Polon. B35 (2004) 1981
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7678
dc.subjectAstrophysics
dc.titleNeutrinos from pre-supernova star
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