Ultra-high energy neutrinos at the Pierre Auger Observatory

Autores
Pieroni, Pablo Emanuel
Año de publicación
2016
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
Neutrinos in the sub-EeV energy range and above can be detected with the Surface Detector (SD) of the Pierre Auger Observatory. They can be identified through the broad time structure of the signals induced in the SD stations. This can be efficiently done for neutrinos of all flavours interacting in the atmosphere at large zenith angles, typically above 60 deg. (downward going), as well as for ?Earth-skimming? neutrino interactions in the case of tau neutrinos (upward going). The wide angular range naturally calls for three sets of identification criteria designed to search for downward going neutrinos in the zenith angle bins (60, 75) deg. and (75, 90) deg. as well as for upward going neutrinos. In this contribution the three searches are combined into a single one, providing, in the absence of candidates in data, an updated and stringent limit to the flux of ultra-high energy neutrinos.
Fil: Pieroni, Pablo Emanuel. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria; Argentina. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina
33rd International Cosmic Ray Conference: The Astroparticle Physics Conference
Rio de Janeiro
Brasil
International Union of Pure and Applied Physics
Materia
Pierre Auger Observatory
Utra-high energy neutrinos
Inclined showers
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/161629
Acceder
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spelling Ultra-high energy neutrinos at the Pierre Auger ObservatoryPieroni, Pablo EmanuelPierre Auger ObservatoryUtra-high energy neutrinosInclined showershttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Neutrinos in the sub-EeV energy range and above can be detected with the Surface Detector (SD) of the Pierre Auger Observatory. They can be identified through the broad time structure of the signals induced in the SD stations. This can be efficiently done for neutrinos of all flavours interacting in the atmosphere at large zenith angles, typically above 60 deg. (downward going), as well as for ?Earth-skimming? neutrino interactions in the case of tau neutrinos (upward going). The wide angular range naturally calls for three sets of identification criteria designed to search for downward going neutrinos in the zenith angle bins (60, 75) deg. and (75, 90) deg. as well as for upward going neutrinos. In this contribution the three searches are combined into a single one, providing, in the absence of candidates in data, an updated and stringent limit to the flux of ultra-high energy neutrinos.Fil: Pieroni, Pablo Emanuel. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria; Argentina. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina33rd International Cosmic Ray Conference: The Astroparticle Physics ConferenceRio de JaneiroBrasilInternational Union of Pure and Applied PhysicsSociedade Brasileira de Fisica2016info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectConferenciaBookhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/161629Ultra-high energy neutrinos at the Pierre Auger Observatory; 33rd International Cosmic Ray Conference: The Astroparticle Physics Conference; Rio de Janeiro; Brasil; 2013; 538-541978-1-5108-1008-2CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://inspirehep.net/literature/1412443info:eu-repo/semantics/altIdentifier/url/http://toc.proceedings.com/27418webtoc.pdfInternacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-03T09:52:35Zoai:ri.conicet.gov.ar:11336/161629instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-03 09:52:36.206CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Ultra-high energy neutrinos at the Pierre Auger Observatory
title Ultra-high energy neutrinos at the Pierre Auger Observatory
spellingShingle Ultra-high energy neutrinos at the Pierre Auger Observatory
Pieroni, Pablo Emanuel
Pierre Auger Observatory
Utra-high energy neutrinos
Inclined showers
title_short Ultra-high energy neutrinos at the Pierre Auger Observatory
title_full Ultra-high energy neutrinos at the Pierre Auger Observatory
title_fullStr Ultra-high energy neutrinos at the Pierre Auger Observatory
title_full_unstemmed Ultra-high energy neutrinos at the Pierre Auger Observatory
title_sort Ultra-high energy neutrinos at the Pierre Auger Observatory
dc.creator.none.fl_str_mv Pieroni, Pablo Emanuel
author Pieroni, Pablo Emanuel
author_facet Pieroni, Pablo Emanuel
author_role author
dc.subject.none.fl_str_mv Pierre Auger Observatory
Utra-high energy neutrinos
Inclined showers
topic Pierre Auger Observatory
Utra-high energy neutrinos
Inclined showers
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Neutrinos in the sub-EeV energy range and above can be detected with the Surface Detector (SD) of the Pierre Auger Observatory. They can be identified through the broad time structure of the signals induced in the SD stations. This can be efficiently done for neutrinos of all flavours interacting in the atmosphere at large zenith angles, typically above 60 deg. (downward going), as well as for ?Earth-skimming? neutrino interactions in the case of tau neutrinos (upward going). The wide angular range naturally calls for three sets of identification criteria designed to search for downward going neutrinos in the zenith angle bins (60, 75) deg. and (75, 90) deg. as well as for upward going neutrinos. In this contribution the three searches are combined into a single one, providing, in the absence of candidates in data, an updated and stringent limit to the flux of ultra-high energy neutrinos.
Fil: Pieroni, Pablo Emanuel. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria; Argentina. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina
33rd International Cosmic Ray Conference: The Astroparticle Physics Conference
Rio de Janeiro
Brasil
International Union of Pure and Applied Physics
description Neutrinos in the sub-EeV energy range and above can be detected with the Surface Detector (SD) of the Pierre Auger Observatory. They can be identified through the broad time structure of the signals induced in the SD stations. This can be efficiently done for neutrinos of all flavours interacting in the atmosphere at large zenith angles, typically above 60 deg. (downward going), as well as for ?Earth-skimming? neutrino interactions in the case of tau neutrinos (upward going). The wide angular range naturally calls for three sets of identification criteria designed to search for downward going neutrinos in the zenith angle bins (60, 75) deg. and (75, 90) deg. as well as for upward going neutrinos. In this contribution the three searches are combined into a single one, providing, in the absence of candidates in data, an updated and stringent limit to the flux of ultra-high energy neutrinos.
publishDate 2016
dc.date.none.fl_str_mv 2016
dc.type.none.fl_str_mv info:eu-repo/semantics/publishedVersion
info:eu-repo/semantics/conferenceObject
Conferencia
Book
http://purl.org/coar/resource_type/c_5794
info:ar-repo/semantics/documentoDeConferencia
status_str publishedVersion
format conferenceObject
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/161629
Ultra-high energy neutrinos at the Pierre Auger Observatory; 33rd International Cosmic Ray Conference: The Astroparticle Physics Conference; Rio de Janeiro; Brasil; 2013; 538-541
978-1-5108-1008-2
CONICET Digital
CONICET
url http://hdl.handle.net/11336/161629
identifier_str_mv Ultra-high energy neutrinos at the Pierre Auger Observatory; 33rd International Cosmic Ray Conference: The Astroparticle Physics Conference; Rio de Janeiro; Brasil; 2013; 538-541
978-1-5108-1008-2
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://inspirehep.net/literature/1412443
info:eu-repo/semantics/altIdentifier/url/http://toc.proceedings.com/27418webtoc.pdf
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
application/pdf
application/pdf
dc.coverage.none.fl_str_mv Internacional
dc.publisher.none.fl_str_mv Sociedade Brasileira de Fisica
publisher.none.fl_str_mv Sociedade Brasileira de Fisica
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 13.13397

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