Supernova neutrino detection

Simple item page
dc.creatorScholberg, K.
dc.date2007-01-04
dc.date.accessioned2026-07-07T07:38:25Z
dc.date.available2026-07-07T07:38:25Z
dc.descriptionThe gravitational core collapse of a star produces a huge burst of neutrinos of all flavors. A number of detectors worldwide are sensitive to such a burst; its detection would yield information about both particle physics and astrophysics. Sensitivity to all flavors, and ability to tag different interactions, will be key for extraction of information. Here I will survey the capabilities of current and future detectors for detection of supernova neutrinos from the Milky Way and beyond.
dc.descriptionSubmitted to the Proceedings of Neutrino 2006, Santa Fe, with minor updates and extended list of experiment references. 7 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0701081
dc.identifierhttp://arxiv.org/abs/astro-ph/0701081
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/121077
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Experiment
dc.subjectNuclear Experiment
dc.titleSupernova neutrino detection
dc.typetext

Files

Collections

arXiv