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
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/75558
Ver los metadatos del registro completo
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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:UNLP2025-09-29T11:12:12Zoai: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:13292025-09-29 11:12:13.236SEDICI (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) |
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SEDICI (UNLP) |
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Universidad Nacional de La Plata |
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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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