Possible explanation for the tail of the cosmic ray spectrum

Autores
Anchordoqui, Luis Alfredo; Dova, María Teresa; McCauley, T. P.; Reucroft, S.; Swain, J. D.
Año de publicación
2000
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
A re-examination of the energy cosmic ray spectrum above 1020 eV is presented. The overall data-base provides evidence, albeit still statistically limited, that non-nucleon primaries could be present at the end of the spectrum. In particular, the possible appearance of superheavy nuclei seldom discussed in the literature is analysed in detail.
Facultad de Ciencias Exactas
Materia
Ciencias Exactas
Física
cosmic ray spectrum
high energy particle interaction
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:10915/75558
Acceder
id SEDICI_3936d0159944511cce534dc4b072461e
oai_identifier_str oai:sedici.unlp.edu.ar:10915/75558
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling Possible explanation for the tail of the cosmic ray spectrumAnchordoqui, Luis AlfredoDova, María TeresaMcCauley, T. P.Reucroft, S.Swain, J. D.Ciencias ExactasFísicacosmic ray spectrumhigh energy particle interactionA re-examination of the energy cosmic ray spectrum above 10<SUP>20</SUP> eV is presented. The overall data-base provides evidence, albeit still statistically limited, that non-nucleon primaries could be present at the end of the spectrum. In particular, the possible appearance of superheavy nuclei seldom discussed in the literature is analysed in detail.Facultad de Ciencias Exactas2000-06-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf343-348http://sedici.unlp.edu.ar/handle/10915/75558enginfo:eu-repo/semantics/altIdentifier/issn/0370-2693info:eu-repo/semantics/altIdentifier/doi/10.1016/S0370-2693(00)00534-7info: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:UNLP2025-10-22T16:53:05Zoai:sedici.unlp.edu.ar:10915/75558Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 16:53:05.929SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Possible explanation for the tail of the cosmic ray spectrum
title Possible explanation for the tail of the cosmic ray spectrum
spellingShingle Possible explanation for the tail of the cosmic ray spectrum
Anchordoqui, Luis Alfredo
Ciencias Exactas
Física
cosmic ray spectrum
high energy particle interaction
title_short Possible explanation for the tail of the cosmic ray spectrum
title_full Possible explanation for the tail of the cosmic ray spectrum
title_fullStr Possible explanation for the tail of the cosmic ray spectrum
title_full_unstemmed Possible explanation for the tail of the cosmic ray spectrum
title_sort Possible explanation for the tail of the cosmic ray spectrum
dc.creator.none.fl_str_mv Anchordoqui, Luis Alfredo
Dova, María Teresa
McCauley, T. P.
Reucroft, S.
Swain, J. D.
author Anchordoqui, Luis Alfredo
author_facet Anchordoqui, Luis Alfredo
Dova, María Teresa
McCauley, T. P.
Reucroft, S.
Swain, J. D.
author_role author
author2 Dova, María Teresa
McCauley, T. P.
Reucroft, S.
Swain, J. D.
author2_role author
author
author
author
dc.subject.none.fl_str_mv Ciencias Exactas
Física
cosmic ray spectrum
high energy particle interaction
topic Ciencias Exactas
Física
cosmic ray spectrum
high energy particle interaction
dc.description.none.fl_txt_mv A re-examination of the energy cosmic ray spectrum above 10<SUP>20</SUP> eV is presented. The overall data-base provides evidence, albeit still statistically limited, that non-nucleon primaries could be present at the end of the spectrum. In particular, the possible appearance of superheavy nuclei seldom discussed in the literature is analysed in detail.
Facultad de Ciencias Exactas
description A re-examination of the energy cosmic ray spectrum above 10<SUP>20</SUP> eV is presented. The overall data-base provides evidence, albeit still statistically limited, that non-nucleon primaries could be present at the end of the spectrum. In particular, the possible appearance of superheavy nuclei seldom discussed in the literature is analysed in detail.
publishDate 2000
dc.date.none.fl_str_mv 2000-06-08
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/10915/75558
url http://sedici.unlp.edu.ar/handle/10915/75558
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/0370-2693
info:eu-repo/semantics/altIdentifier/doi/10.1016/S0370-2693(00)00534-7
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
343-348
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 12.982451

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