Composition studies of Ultra High Energy Cosmic Rays at the Pierre Auger Observatory

Autores
Jarne, Cecilia Gisele; Pierre Auger Collaboration
Año de publicación
2015
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
To understand the origin and nature of Ultra High Energy Cosmic Rays their mass composition must be known. The Pierre Auger Observatory is an instrument which provides valuable information for the determination of the primary mass. Different parameters that describe various characteristics of the shower development and at the same time are sensitive to the primary mass are discussed. Their energy dependence and a comparison with predictions from different models are also presented.
Facultad de Ciencias Exactas
Materia
Física
Composition
Pierre Auger Observatory
UHECR
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-nd/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/85936
Acceder
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oai_identifier_str oai:sedici.unlp.edu.ar:10915/85936
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network_name_str SEDICI (UNLP)
spelling Composition studies of Ultra High Energy Cosmic Rays at the Pierre Auger ObservatoryJarne, Cecilia GiselePierre Auger CollaborationFísicaCompositionPierre Auger ObservatoryUHECRTo understand the origin and nature of Ultra High Energy Cosmic Rays their mass composition must be known. The Pierre Auger Observatory is an instrument which provides valuable information for the determination of the primary mass. Different parameters that describe various characteristics of the shower development and at the same time are sensitive to the primary mass are discussed. Their energy dependence and a comparison with predictions from different models are also presented.Facultad de Ciencias Exactas2015info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf399-402http://sedici.unlp.edu.ar/handle/10915/85936enginfo:eu-repo/semantics/altIdentifier/issn/2405-6014info:eu-repo/semantics/altIdentifier/doi/10.1016/j.nuclphysbps.2015.10.136info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-nd/4.0/Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-03T10:49:17Zoai:sedici.unlp.edu.ar:10915/85936Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-03 10:49:17.681SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Composition studies of Ultra High Energy Cosmic Rays at the Pierre Auger Observatory
title Composition studies of Ultra High Energy Cosmic Rays at the Pierre Auger Observatory
spellingShingle Composition studies of Ultra High Energy Cosmic Rays at the Pierre Auger Observatory
Jarne, Cecilia Gisele
Física
Composition
Pierre Auger Observatory
UHECR
title_short Composition studies of Ultra High Energy Cosmic Rays at the Pierre Auger Observatory
title_full Composition studies of Ultra High Energy Cosmic Rays at the Pierre Auger Observatory
title_fullStr Composition studies of Ultra High Energy Cosmic Rays at the Pierre Auger Observatory
title_full_unstemmed Composition studies of Ultra High Energy Cosmic Rays at the Pierre Auger Observatory
title_sort Composition studies of Ultra High Energy Cosmic Rays at the Pierre Auger Observatory
dc.creator.none.fl_str_mv Jarne, Cecilia Gisele
Pierre Auger Collaboration
author Jarne, Cecilia Gisele
author_facet Jarne, Cecilia Gisele
Pierre Auger Collaboration
author_role author
author2 Pierre Auger Collaboration
author2_role author
dc.subject.none.fl_str_mv Física
Composition
Pierre Auger Observatory
UHECR
topic Física
Composition
Pierre Auger Observatory
UHECR
dc.description.none.fl_txt_mv To understand the origin and nature of Ultra High Energy Cosmic Rays their mass composition must be known. The Pierre Auger Observatory is an instrument which provides valuable information for the determination of the primary mass. Different parameters that describe various characteristics of the shower development and at the same time are sensitive to the primary mass are discussed. Their energy dependence and a comparison with predictions from different models are also presented.
Facultad de Ciencias Exactas
description To understand the origin and nature of Ultra High Energy Cosmic Rays their mass composition must be known. The Pierre Auger Observatory is an instrument which provides valuable information for the determination of the primary mass. Different parameters that describe various characteristics of the shower development and at the same time are sensitive to the primary mass are discussed. Their energy dependence and a comparison with predictions from different models are also presented.
publishDate 2015
dc.date.none.fl_str_mv 2015
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/10915/85936
url http://sedici.unlp.edu.ar/handle/10915/85936
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/2405-6014
info:eu-repo/semantics/altIdentifier/doi/10.1016/j.nuclphysbps.2015.10.136
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-nd/4.0/
Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-nd/4.0/
Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)
dc.format.none.fl_str_mv application/pdf
399-402
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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 13.13397

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