The pierre auger observatory and ultra-high energy neutrinos: Upper limits to the diffuse and point source fluxes

With the Surface Detector of the Pierre Auger Observatory, we can detect ultra-high energy neutrinos in the sub-EeV energy range and above. Neutrinos of all flavours can interact in the atmosphere and induce inclined showers close to the ground (down-going). The sensitivity of the Surface Detector t...

Descripción completa

Guardado en:
Detalles Bibliográficos
Publicado: 2011
Materias:
Cosmic rays
Pierre auger observatory
UHE neutrinos
Augers
Detectors
Neutrons
Observatories
Auger observatory
Differential flux
Identification criterion
Neutrino interactions
Pierre Auger observatory
Surface detectors
Ultra-high energy neutrinos
Particle detectors
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_NIS12911_v4_n_p201_Guardincerri
http://hdl.handle.net/20.500.12110/paper_NIS12911_v4_n_p201_Guardincerri
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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