Ultrahigh energy neutrinos at the Pierre Auger Observatory

The observation of ultrahigh energy neutrinos (UHE s) has become a priority in experimental astroparticle physics. UHE s 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 sh...

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Detalles Bibliográficos
Autores principales:	Arganda Carreras, Ernesto, Dova, María Teresa, Gómez Albarracín, Flavia Alejandra, Hansen, Patricia María, Jarne, Cecilia Gisele, Mariazzi, Analisa Gabriela, Moreno, Juan Cruz, Sciutto, Sergio Juan, Wahlberg, Hernán Pablo, The Pierre Auger Collaboration
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2013
Materias:	Ciencias Exactas Física Altas energías Astroparticle physics Cascada atmosférica extensa
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/81561
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

id	I19-R120-10915-81561
record_format	dspace
institution	Universidad Nacional de La Plata
institution_str	I-19
repository_str	R-120
collection	SEDICI (UNLP)
language	Inglés
topic	Ciencias Exactas Física Altas energías Astroparticle physics Cascada atmosférica extensa
spellingShingle	Ciencias Exactas Física Altas energías Astroparticle physics Cascada atmosférica extensa Arganda Carreras, Ernesto Dova, María Teresa Gómez Albarracín, Flavia Alejandra Hansen, Patricia María Jarne, Cecilia Gisele Mariazzi, Analisa Gabriela Moreno, Juan Cruz Sciutto, Sergio Juan Wahlberg, Hernán Pablo The Pierre Auger Collaboration Ultrahigh energy neutrinos at the Pierre Auger Observatory
topic_facet	Ciencias Exactas Física Altas energías Astroparticle physics Cascada atmosférica extensa
description	The observation of ultrahigh energy neutrinos (UHE s) has become a priority in experimental astroparticle physics. UHE s 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 UHE s 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 UHE s in the EeV range and above.
format	Articulo Articulo
author	Arganda Carreras, Ernesto Dova, María Teresa Gómez Albarracín, Flavia Alejandra Hansen, Patricia María Jarne, Cecilia Gisele Mariazzi, Analisa Gabriela Moreno, Juan Cruz Sciutto, Sergio Juan Wahlberg, Hernán Pablo The Pierre Auger Collaboration
author_facet	Arganda Carreras, Ernesto Dova, María Teresa Gómez Albarracín, Flavia Alejandra Hansen, Patricia María Jarne, Cecilia Gisele Mariazzi, Analisa Gabriela Moreno, Juan Cruz Sciutto, Sergio Juan Wahlberg, Hernán Pablo The Pierre Auger Collaboration
author_sort	Arganda Carreras, Ernesto
title	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	http://sedici.unlp.edu.ar/handle/10915/81561
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bdutipo_str	Repositorios
_version_	1764820488212709376

Ultrahigh energy neutrinos at the Pierre Auger Observatory

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