Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory

Neutrinos with energies above 10¹⁷ eV are detectable with the Surface Detector Array of the Pierre Auger Observatory. The identification is efficiently performed for neutrinos of all flavors interacting in the atmosphere at large zenith angles, as well as for Earth-skimming tau neutrinos with nearly...

Descripción completa

Detalles Bibliográficos
Autores principales:	Calcagni, Laura Randa, Dova, María Teresa, Hansen, Patricia María, Mariazzi, Analisa Gabriela, Sciutto, Sergio Juan, Tueros, Matías Jorge, Vergara Quispe, Indira Dajhana, Wahlberg, Hernán Pablo, The Pierre Auger Collaboration
Formato:	Articulo Preprint
Lenguaje:	Inglés
Publicado:	2019
Materias:	Física Ultra-high-energy cosmic rays and neutrinos Extensive air showers Surface detector arrays Pierre Auger Observatory
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/125464
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

id	I19-R120-10915-125464
record_format	dspace
institution	Universidad Nacional de La Plata
institution_str	I-19
repository_str	R-120
collection	SEDICI (UNLP)
language	Inglés
topic	Física Ultra-high-energy cosmic rays and neutrinos Extensive air showers Surface detector arrays Pierre Auger Observatory
spellingShingle	Física Ultra-high-energy cosmic rays and neutrinos Extensive air showers Surface detector arrays Pierre Auger Observatory Calcagni, Laura Randa Dova, María Teresa Hansen, Patricia María Mariazzi, Analisa Gabriela Sciutto, Sergio Juan Tueros, Matías Jorge Vergara Quispe, Indira Dajhana Wahlberg, Hernán Pablo The Pierre Auger Collaboration Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory
topic_facet	Física Ultra-high-energy cosmic rays and neutrinos Extensive air showers Surface detector arrays Pierre Auger Observatory
description	Neutrinos with energies above 10¹⁷ eV are detectable with the Surface Detector Array of the Pierre Auger Observatory. The identification is efficiently performed for neutrinos of all flavors interacting in the atmosphere at large zenith angles, as well as for Earth-skimming tau neutrinos with nearly tangential trajectories relative to the Earth. No neutrino candidates were found in similar to 14.7 years of data taken up to 31 August 2018. This leads to restrictive upper bounds on their flux. The 90% C.L. single-flavor limit to the diffuse flux of ultra-high-energy neutrinos with an E-nu(⁻²) spectrum in the energy range 1.0 x 10¹⁷ eV-2.5 x 10¹⁹ eV is E(²)dN(nu)/dE(nu) <4.4 x 10(⁻⁹) GeV cm(⁻²) s(⁻¹) sr(⁻¹), placing strong constraints on several models of neutrino production at EeV energies and on the properties of the sources of ultra-high-energy cosmic rays.
format	Articulo Preprint
author	Calcagni, Laura Randa Dova, María Teresa Hansen, Patricia María Mariazzi, Analisa Gabriela Sciutto, Sergio Juan Tueros, Matías Jorge Vergara Quispe, Indira Dajhana Wahlberg, Hernán Pablo The Pierre Auger Collaboration
author_facet	Calcagni, Laura Randa Dova, María Teresa Hansen, Patricia María Mariazzi, Analisa Gabriela Sciutto, Sergio Juan Tueros, Matías Jorge Vergara Quispe, Indira Dajhana Wahlberg, Hernán Pablo The Pierre Auger Collaboration
author_sort	Calcagni, Laura Randa
title	Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory
title_short	Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory
title_full	Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory
title_fullStr	Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory
title_full_unstemmed	Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory
title_sort	probing the origin of ultra-high-energy cosmic rays with neutrinos in the eev energy range using the pierre auger observatory
publishDate	2019
url	http://sedici.unlp.edu.ar/handle/10915/125464
work_keys_str_mv	AT calcagnilauraranda probingtheoriginofultrahighenergycosmicrayswithneutrinosintheeevenergyrangeusingthepierreaugerobservatory AT dovamariateresa probingtheoriginofultrahighenergycosmicrayswithneutrinosintheeevenergyrangeusingthepierreaugerobservatory AT hansenpatriciamaria probingtheoriginofultrahighenergycosmicrayswithneutrinosintheeevenergyrangeusingthepierreaugerobservatory AT mariazzianalisagabriela probingtheoriginofultrahighenergycosmicrayswithneutrinosintheeevenergyrangeusingthepierreaugerobservatory AT sciuttosergiojuan probingtheoriginofultrahighenergycosmicrayswithneutrinosintheeevenergyrangeusingthepierreaugerobservatory AT tuerosmatiasjorge probingtheoriginofultrahighenergycosmicrayswithneutrinosintheeevenergyrangeusingthepierreaugerobservatory AT vergaraquispeindiradajhana probingtheoriginofultrahighenergycosmicrayswithneutrinosintheeevenergyrangeusingthepierreaugerobservatory AT wahlberghernanpablo probingtheoriginofultrahighenergycosmicrayswithneutrinosintheeevenergyrangeusingthepierreaugerobservatory AT thepierreaugercollaboration probingtheoriginofultrahighenergycosmicrayswithneutrinosintheeevenergyrangeusingthepierreaugerobservatory
bdutipo_str	Repositorios
_version_	1764820451709681667

Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory

Ejemplares similares