Phenomenology of cosmic ray air showers

Autores
Dova, María Teresa
Año de publicación
2005
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
The properties of cosmic rays with energies above 106 GeV have to be deduced from the spacetime structure and particle content of the air showers which they initiate. In this review, a summary of the phenomenology of these giant air showers is presented. We describe the hadronic interaction models used to extrapolate results from collider data to ultra high energies, an also the main electromagnetic processes that govern the longitudinal shower evolution as well as the lateral spread of particles.
Facultad de Ciencias Exactas
Materia
Ciencias Exactas
Física
Radiación Cósmica
Fenomenología
Cascada atmosférica extensa
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:10915/81602
Acceder
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oai_identifier_str oai:sedici.unlp.edu.ar:10915/81602
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling Phenomenology of cosmic ray air showersDova, María TeresaCiencias ExactasFísicaRadiación CósmicaFenomenologíaCascada atmosférica extensaThe properties of cosmic rays with energies above 10<sup>6</sup> GeV have to be deduced from the spacetime structure and particle content of the air showers which they initiate. In this review, a summary of the phenomenology of these giant air showers is presented. We describe the hadronic interaction models used to extrapolate results from collider data to ultra high energies, an also the main electromagnetic processes that govern the longitudinal shower evolution as well as the lateral spread of particles.Facultad de Ciencias Exactas2005-01info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionObjeto de conferenciahttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/81602enginfo:eu-repo/semantics/altIdentifier/isbn/978-981-256-625-6info:eu-repo/semantics/altIdentifier/doi/10.1142/9789812774439_0005info: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:UNLP2025-09-29T11:15:12Zoai:sedici.unlp.edu.ar:10915/81602Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:15:12.474SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Phenomenology of cosmic ray air showers
title Phenomenology of cosmic ray air showers
spellingShingle Phenomenology of cosmic ray air showers
Dova, María Teresa
Ciencias Exactas
Física
Radiación Cósmica
Fenomenología
Cascada atmosférica extensa
title_short Phenomenology of cosmic ray air showers
title_full Phenomenology of cosmic ray air showers
title_fullStr Phenomenology of cosmic ray air showers
title_full_unstemmed Phenomenology of cosmic ray air showers
title_sort Phenomenology of cosmic ray air showers
dc.creator.none.fl_str_mv Dova, María Teresa
author Dova, María Teresa
author_facet Dova, María Teresa
author_role author
dc.subject.none.fl_str_mv Ciencias Exactas
Física
Radiación Cósmica
Fenomenología
Cascada atmosférica extensa
topic Ciencias Exactas
Física
Radiación Cósmica
Fenomenología
Cascada atmosférica extensa
dc.description.none.fl_txt_mv The properties of cosmic rays with energies above 10<sup>6</sup> GeV have to be deduced from the spacetime structure and particle content of the air showers which they initiate. In this review, a summary of the phenomenology of these giant air showers is presented. We describe the hadronic interaction models used to extrapolate results from collider data to ultra high energies, an also the main electromagnetic processes that govern the longitudinal shower evolution as well as the lateral spread of particles.
Facultad de Ciencias Exactas
description The properties of cosmic rays with energies above 10<sup>6</sup> GeV have to be deduced from the spacetime structure and particle content of the air showers which they initiate. In this review, a summary of the phenomenology of these giant air showers is presented. We describe the hadronic interaction models used to extrapolate results from collider data to ultra high energies, an also the main electromagnetic processes that govern the longitudinal shower evolution as well as the lateral spread of particles.
publishDate 2005
dc.date.none.fl_str_mv 2005-01
dc.type.none.fl_str_mv info:eu-repo/semantics/conferenceObject
info:eu-repo/semantics/publishedVersion
Objeto de conferencia
http://purl.org/coar/resource_type/c_5794
info:ar-repo/semantics/documentoDeConferencia
format conferenceObject
status_str publishedVersion
dc.identifier.none.fl_str_mv http://sedici.unlp.edu.ar/handle/10915/81602
url http://sedici.unlp.edu.ar/handle/10915/81602
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/isbn/978-981-256-625-6
info:eu-repo/semantics/altIdentifier/doi/10.1142/9789812774439_0005
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
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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score 13.070432

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