Direct measurement of the muonic content of extensive air showers between 2 × 10¹⁷ and 2 × 10¹⁸ eV at the Pierre Auger Observatory

Autores
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
Año de publicación
2020
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The hybrid design of the Pierre Auger Observatory allows for the measurement of the properties of extensive air showers initiated by ultra-high energy cosmic rays with unprecedented precision. By using an array of prototype underground muon detectors, we have performed the first direct measurement, by the Auger Collaboration, of the muon content of air showers between 2 × 10¹⁷ and 2 × 10¹⁸ eV. We have studied the energy evolution of the attenuation-corrected muon density, and compared it to predictions from air shower simulations. The observed densities are found to be larger than those predicted by models. We quantify this discrepancy by combining the measurements from the muon detector with those from the Auger fluorescence detector at 1017.5 eV and 10¹⁸ eV. We find that, for the models to explain the data, an increase in the muon density of 38% ± 4%(12%) ± 21%18% for EPOS- LHC, and of 50%(53%) ± 4%(13%) ± 23%20% for QGSJetII- 04, is respectively needed.
La lista completa de autores que integran el documento puede consultarse en el archivo.
Facultad de Ciencias Exactas
Instituto de Física La Plata
Materia
Ciencias Exactas
Física
Cosmic ray
Physics
Air shower
Energy
Muon
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/125559

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network_name_str SEDICI (UNLP)
spelling Direct measurement of the muonic content of extensive air showers between 2 × 10¹⁷ and 2 × 10¹⁸ eV at the Pierre Auger ObservatoryCalcagni, Laura RandaDova, María TeresaHansen, Patricia MaríaMariazzi, Analisa GabrielaSciutto, Sergio JuanTueros, Matías JorgeVergara Quispe, Indira DajhanaWahlberg, Hernán PabloThe Pierre Auger CollaborationCiencias ExactasFísicaCosmic rayPhysicsAir showerEnergyMuonThe hybrid design of the Pierre Auger Observatory allows for the measurement of the properties of extensive air showers initiated by ultra-high energy cosmic rays with unprecedented precision. By using an array of prototype underground muon detectors, we have performed the first direct measurement, by the Auger Collaboration, of the muon content of air showers between 2 × 10¹⁷ and 2 × 10¹⁸ eV. We have studied the energy evolution of the attenuation-corrected muon density, and compared it to predictions from air shower simulations. The observed densities are found to be larger than those predicted by models. We quantify this discrepancy by combining the measurements from the muon detector with those from the Auger fluorescence detector at 10<sup>17.5</sup> eV and 10¹⁸ eV. We find that, for the models to explain the data, an increase in the muon density of 38% ± 4%(12%) ± <sup>21%</sup><sub>18%</sub> for EPOS- LHC, and of 50%(53%) ± 4%(13%) ± <sup>23%</sup><sub>20%</sub> for QGSJetII- 04, is respectively needed.La lista completa de autores que integran el documento puede consultarse en el archivo.Facultad de Ciencias ExactasInstituto de Física La Plata2020-08-18info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/125559enginfo:eu-repo/semantics/altIdentifier/issn/1434-6044info:eu-repo/semantics/altIdentifier/issn/1434-6052info:eu-repo/semantics/altIdentifier/doi/10.1140/epjc/s10052-020-8055-yinfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/4.0/Creative Commons Attribution 4.0 International (CC BY 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-29T11:29:49Zoai:sedici.unlp.edu.ar:10915/125559Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:29:49.387SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Direct measurement of the muonic content of extensive air showers between 2 × 10¹⁷ and 2 × 10¹⁸ eV at the Pierre Auger Observatory
title Direct measurement of the muonic content of extensive air showers between 2 × 10¹⁷ and 2 × 10¹⁸ eV at the Pierre Auger Observatory
spellingShingle Direct measurement of the muonic content of extensive air showers between 2 × 10¹⁷ and 2 × 10¹⁸ eV at the Pierre Auger Observatory
Calcagni, Laura Randa
Ciencias Exactas
Física
Cosmic ray
Physics
Air shower
Energy
Muon
title_short Direct measurement of the muonic content of extensive air showers between 2 × 10¹⁷ and 2 × 10¹⁸ eV at the Pierre Auger Observatory
title_full Direct measurement of the muonic content of extensive air showers between 2 × 10¹⁷ and 2 × 10¹⁸ eV at the Pierre Auger Observatory
title_fullStr Direct measurement of the muonic content of extensive air showers between 2 × 10¹⁷ and 2 × 10¹⁸ eV at the Pierre Auger Observatory
title_full_unstemmed Direct measurement of the muonic content of extensive air showers between 2 × 10¹⁷ and 2 × 10¹⁸ eV at the Pierre Auger Observatory
title_sort Direct measurement of the muonic content of extensive air showers between 2 × 10¹⁷ and 2 × 10¹⁸ eV at the Pierre Auger Observatory
dc.creator.none.fl_str_mv 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 Calcagni, Laura Randa
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_role author
author2 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
author2_role author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Ciencias Exactas
Física
Cosmic ray
Physics
Air shower
Energy
Muon
topic Ciencias Exactas
Física
Cosmic ray
Physics
Air shower
Energy
Muon
dc.description.none.fl_txt_mv The hybrid design of the Pierre Auger Observatory allows for the measurement of the properties of extensive air showers initiated by ultra-high energy cosmic rays with unprecedented precision. By using an array of prototype underground muon detectors, we have performed the first direct measurement, by the Auger Collaboration, of the muon content of air showers between 2 × 10¹⁷ and 2 × 10¹⁸ eV. We have studied the energy evolution of the attenuation-corrected muon density, and compared it to predictions from air shower simulations. The observed densities are found to be larger than those predicted by models. We quantify this discrepancy by combining the measurements from the muon detector with those from the Auger fluorescence detector at 10<sup>17.5</sup> eV and 10¹⁸ eV. We find that, for the models to explain the data, an increase in the muon density of 38% ± 4%(12%) ± <sup>21%</sup><sub>18%</sub> for EPOS- LHC, and of 50%(53%) ± 4%(13%) ± <sup>23%</sup><sub>20%</sub> for QGSJetII- 04, is respectively needed.
La lista completa de autores que integran el documento puede consultarse en el archivo.
Facultad de Ciencias Exactas
Instituto de Física La Plata
description The hybrid design of the Pierre Auger Observatory allows for the measurement of the properties of extensive air showers initiated by ultra-high energy cosmic rays with unprecedented precision. By using an array of prototype underground muon detectors, we have performed the first direct measurement, by the Auger Collaboration, of the muon content of air showers between 2 × 10¹⁷ and 2 × 10¹⁸ eV. We have studied the energy evolution of the attenuation-corrected muon density, and compared it to predictions from air shower simulations. The observed densities are found to be larger than those predicted by models. We quantify this discrepancy by combining the measurements from the muon detector with those from the Auger fluorescence detector at 10<sup>17.5</sup> eV and 10¹⁸ eV. We find that, for the models to explain the data, an increase in the muon density of 38% ± 4%(12%) ± <sup>21%</sup><sub>18%</sub> for EPOS- LHC, and of 50%(53%) ± 4%(13%) ± <sup>23%</sup><sub>20%</sub> for QGSJetII- 04, is respectively needed.
publishDate 2020
dc.date.none.fl_str_mv 2020-08-18
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Articulo
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://sedici.unlp.edu.ar/handle/10915/125559
url http://sedici.unlp.edu.ar/handle/10915/125559
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/1434-6044
info:eu-repo/semantics/altIdentifier/issn/1434-6052
info:eu-repo/semantics/altIdentifier/doi/10.1140/epjc/s10052-020-8055-y
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by/4.0/
Creative Commons Attribution 4.0 International (CC BY 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by/4.0/
Creative Commons Attribution 4.0 International (CC BY 4.0)
dc.format.none.fl_str_mv application/pdf
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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