Neutrinos from Gamma Ray Bursts

Simple item page
dc.creatorHalzen, F.
dc.creatorJaczko, G.
dc.date1996-02-07
dc.date.accessioned2026-07-07T02:20:53Z
dc.date.available2026-07-07T02:20:53Z
dc.descriptionWe show that the detection of neutrinos from a typical gamma ray burst requires a kilometer-scale detector. We argue that large bursts should be visible with the neutrino telescopes under construction. We emphasize the 3 techniques by which neutrino telescopes can perform this search: by triggering on i) bursts of muons from muon neutrinos, ii) muons from air cascades initiated by high energy gamma rays and iii) showers made by relatively low energy ($\simeq 100\,\mev$) electron neutrinos. Timing of neutrino-photon coincidences may yield a measurement of the neutrino mass to order $10^{-5}$~eV, an interesting range in light of the solar neutrino anomaly.
dc.description12 pages, Latex 2.09, no figures. Postscript version available at http://phenom.physics.wisc.edu/pub/preprints/1996/madph-96-929.ps.Z or ftp://phenom.physics.wisc.edu/pub/preprints/1996/madph-96-929.ps.Z
dc.identifierhttps://arxiv.org/abs/astro-ph/9602038
dc.identifierhttp://arxiv.org/abs/astro-ph/9602038
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10360
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleNeutrinos from Gamma Ray Bursts
dc.typetext

Files

Collections

arXiv