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Supernova pointing with low- and high-energy neutrino detectors

A future galactic SN can be located several hours before the optical explosion through the MeV-neutrino burst, exploiting the directionality of $nu$-$e$-scattering in a water Cherenkov detector such as Super-Kamiokande. We study the statistical efficiency of different methods for extracting the SN d...

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Detalles Bibliográficos
Autores principales: Tomás, R, Semikoz, Dmitry V, Raffelt, Georg G, Kachelriess, M, Dighe, Amol S
Lenguaje:eng
Publicado: 2003
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.68.093013
http://cds.cern.ch/record/627263