A new observable in extensive air showers

Autores
García Canal, Carlos Alberto; Illana, J. I.; Masip, M.; Sciutto, Sergio Juan
Año de publicación
2016
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We find that the ratio rμe of the muon to the electromagnetic component of an extended air shower at the ground level provides an indirect measure of the depth Xmax of the shower maximum. This result, obtained with the air-shower code AIRES, is independent of the hadronic model used in the simulation. We show that the value of rμe in a particular shower discriminates its proton or iron nature with a 98% efficiency. We also show that the eventual production of forward heavy quarks inside the shower may introduce anomalous values of rμe in isolated events.
Facultad de Ciencias Exactas
Instituto de Física La Plata
Materia
Ciencias Exactas
Física
extensive air shower
cosmic-ray composition
forward charm
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/104964

id SEDICI_e12a7864f52c00b2364dc8486a8e6abf
oai_identifier_str oai:sedici.unlp.edu.ar:10915/104964
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling A new observable in extensive air showersGarcía Canal, Carlos AlbertoIllana, J. I.Masip, M.Sciutto, Sergio JuanCiencias ExactasFísicaextensive air showercosmic-ray compositionforward charmWe find that the ratio r<sub>μe</sub> of the muon to the electromagnetic component of an extended air shower at the ground level provides an indirect measure of the depth X<sub>max</sub> of the shower maximum. This result, obtained with the air-shower code AIRES, is independent of the hadronic model used in the simulation. We show that the value of r<sub>μe</sub> in a particular shower discriminates its proton or iron nature with a 98% efficiency. We also show that the eventual production of forward heavy quarks inside the shower may introduce anomalous values of r<sub>μe</sub> in isolated events.Facultad de Ciencias ExactasInstituto de Física La Plata2016info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf50-53http://sedici.unlp.edu.ar/handle/10915/104964enginfo:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/abs/pii/S092765051630144Xinfo:eu-repo/semantics/altIdentifier/issn/0927-6505info:eu-repo/semantics/altIdentifier/doi/10.1016/j.astropartphys.2016.10.001info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-22T17:03:54Zoai:sedici.unlp.edu.ar:10915/104964Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 17:03:54.518SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv A new observable in extensive air showers
title A new observable in extensive air showers
spellingShingle A new observable in extensive air showers
García Canal, Carlos Alberto
Ciencias Exactas
Física
extensive air shower
cosmic-ray composition
forward charm
title_short A new observable in extensive air showers
title_full A new observable in extensive air showers
title_fullStr A new observable in extensive air showers
title_full_unstemmed A new observable in extensive air showers
title_sort A new observable in extensive air showers
dc.creator.none.fl_str_mv García Canal, Carlos Alberto
Illana, J. I.
Masip, M.
Sciutto, Sergio Juan
author García Canal, Carlos Alberto
author_facet García Canal, Carlos Alberto
Illana, J. I.
Masip, M.
Sciutto, Sergio Juan
author_role author
author2 Illana, J. I.
Masip, M.
Sciutto, Sergio Juan
author2_role author
author
author
dc.subject.none.fl_str_mv Ciencias Exactas
Física
extensive air shower
cosmic-ray composition
forward charm
topic Ciencias Exactas
Física
extensive air shower
cosmic-ray composition
forward charm
dc.description.none.fl_txt_mv We find that the ratio r<sub>μe</sub> of the muon to the electromagnetic component of an extended air shower at the ground level provides an indirect measure of the depth X<sub>max</sub> of the shower maximum. This result, obtained with the air-shower code AIRES, is independent of the hadronic model used in the simulation. We show that the value of r<sub>μe</sub> in a particular shower discriminates its proton or iron nature with a 98% efficiency. We also show that the eventual production of forward heavy quarks inside the shower may introduce anomalous values of r<sub>μe</sub> in isolated events.
Facultad de Ciencias Exactas
Instituto de Física La Plata
description We find that the ratio r<sub>μe</sub> of the muon to the electromagnetic component of an extended air shower at the ground level provides an indirect measure of the depth X<sub>max</sub> of the shower maximum. This result, obtained with the air-shower code AIRES, is independent of the hadronic model used in the simulation. We show that the value of r<sub>μe</sub> in a particular shower discriminates its proton or iron nature with a 98% efficiency. We also show that the eventual production of forward heavy quarks inside the shower may introduce anomalous values of r<sub>μe</sub> in isolated events.
publishDate 2016
dc.date.none.fl_str_mv 2016
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/10915/104964
url http://sedici.unlp.edu.ar/handle/10915/104964
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/abs/pii/S092765051630144X
info:eu-repo/semantics/altIdentifier/issn/0927-6505
info:eu-repo/semantics/altIdentifier/doi/10.1016/j.astropartphys.2016.10.001
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.format.none.fl_str_mv application/pdf
50-53
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
_version_ 1846783308376047616
score 12.982451