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Ultrahigh Energy Neutrinos at the Pierre Auger Observatory

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Ultrahigh Energy Neutrinos at the Pierre Auger Observatory

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dc.contributor.author	The Pierre Auger Collaboration
dc.contributor.author	Arqueros Martínez, Fernando
dc.contributor.author	Minaya Flores, Ignacio Andrés
dc.contributor.author	Gascón Bravo, Alberto
dc.contributor.author	Lopez Agüera, Ángeles
dc.contributor.author	Pastor Carpi, Sergio
dc.contributor.author	Vázquez Peñas, José Ramón
dc.contributor.author	Zamorano García, Bruno
dc.contributor.author	Rosado Vélez, Jaime
dc.date.accessioned	2014-02-19T09:47:43Z
dc.date.available	2014-02-19T09:47:43Z
dc.date.issued	2013
dc.identifier.citation	Pastor Carpi, Sergio Arqueros Martinez, Fernando Minaya Flores, Ignacio Andrés Rosado Velez, Jaime Vázquez Peñas, José Ramón Gascón Bravo, Alberto Zamorano García, Bruno Lopez Agüera, Ángeles 2013 Ultrahigh Energy Neutrinos at the Pierre Auger Observatory Advances In High Energy Physics 2013 708680-1 708680-18
dc.identifier.uri	http://hdl.handle.net/10550/33061
dc.description.abstract	The observation of ultrahigh energy neutrinos (UHEvs) has become a priority in experimental astroparticle physics. UHEvs can be detected with a variety of techniques. In particular, neutrinos can interact in the atmosphere (downward-going nu) or in the Earth crust (Earth-skimming nu), 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 UHEvs 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 UHEvs in the EeV range and above.
dc.relation.ispartof	Advances In High Energy Physics, 2013, vol. 2013, p. 708680-1-708680-18
dc.subject	Partícules (Física nuclear)
dc.title	Ultrahigh Energy Neutrinos at the Pierre Auger Observatory
dc.type	journal article	es_ES
dc.date.updated	2014-02-19T09:47:43Z
dc.identifier.doi	10.1155/2013/708680
dc.identifier.idgrec	093580
dc.rights.accessRights	open access	es_ES
dc.identifier.url	10.1155/2013/708680