Ultrahigh energy neutrinos at the pierre auger observatory

The observation of ultrahigh energy neutrinos (UHEs) has become a priority in experimental astroparticle physics. UHEs can be detected with a variety of techniques. In particular, neutrinos can interact in the atmosphere (downward-going ) or in the Earth crust (Earth-skimming ), producing air shower...

Descripción completa

Guardado en:
Detalles Bibliográficos
Publicado: 2013
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_16877357_v2013_n_p_Multitudinario
http://hdl.handle.net/20.500.12110/paper_16877357_v2013_n_p_Multitudinario
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id paper:paper_16877357_v2013_n_p_Multitudinario
record_format dspace
spelling paper:paper_16877357_v2013_n_p_Multitudinario2023-06-08T16:26:42Z Ultrahigh energy neutrinos at the pierre auger observatory The observation of ultrahigh energy neutrinos (UHEs) has become a priority in experimental astroparticle physics. UHEs can be detected with a variety of techniques. In particular, neutrinos can interact in the atmosphere (downward-going ) or in the Earth crust (Earth-skimming ), producing air showers that can be observed with arrays of detectors at the ground. With the surface detector array of the Pierre Auger Observatory we can detect these types of cascades. The distinguishing signature for neutrino events is the presence of very inclined showers produced close to the ground (i.e., after having traversed a large amount of atmosphere). In this work we review the procedure and criteria established to search for UHEs in the data collected with the ground array of the Pierre Auger Observatory. This includes Earth-skimming as well as downward-going neutrinos. No neutrino candidates have been found, which allows us to place competitive limits to the diffuse flux of UHEs in the EeV range and above. © 2013 P. Abreu et al. 2013 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_16877357_v2013_n_p_Multitudinario http://hdl.handle.net/20.500.12110/paper_16877357_v2013_n_p_Multitudinario
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
description The observation of ultrahigh energy neutrinos (UHEs) has become a priority in experimental astroparticle physics. UHEs can be detected with a variety of techniques. In particular, neutrinos can interact in the atmosphere (downward-going ) or in the Earth crust (Earth-skimming ), producing air showers that can be observed with arrays of detectors at the ground. With the surface detector array of the Pierre Auger Observatory we can detect these types of cascades. The distinguishing signature for neutrino events is the presence of very inclined showers produced close to the ground (i.e., after having traversed a large amount of atmosphere). In this work we review the procedure and criteria established to search for UHEs in the data collected with the ground array of the Pierre Auger Observatory. This includes Earth-skimming as well as downward-going neutrinos. No neutrino candidates have been found, which allows us to place competitive limits to the diffuse flux of UHEs in the EeV range and above. © 2013 P. Abreu et al.
title Ultrahigh energy neutrinos at the pierre auger observatory
spellingShingle Ultrahigh energy neutrinos at the pierre auger observatory
title_short Ultrahigh energy neutrinos at the pierre auger observatory
title_full Ultrahigh energy neutrinos at the pierre auger observatory
title_fullStr Ultrahigh energy neutrinos at the pierre auger observatory
title_full_unstemmed Ultrahigh energy neutrinos at the pierre auger observatory
title_sort ultrahigh energy neutrinos at the pierre auger observatory
publishDate 2013
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_16877357_v2013_n_p_Multitudinario
http://hdl.handle.net/20.500.12110/paper_16877357_v2013_n_p_Multitudinario
_version_ 1768544567677681664

Ejemplares similares