Possible explanation for the tail of the cosmic ray spectrum

Autores
Anchordoqui, Luis A.; Dova, Maria Teresa; Thomas P. McCauley; Reucroft, Stephen; Swain, John
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.
Fil: Anchordoqui, Luis A.. Northeastern University; Estados Unidos
Fil: Dova, Maria Teresa. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina
Fil: Thomas P. McCauley. Northeastern University; Estados Unidos
Fil: Reucroft, Stephen. Northeastern University; Estados Unidos
Fil: Swain, John. Northeastern University; Estados Unidos
Materia
COSMIC RAYS
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/98577
Acceder
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network_name_str CONICET Digital (CONICET)
spelling Possible explanation for the tail of the cosmic ray spectrumAnchordoqui, Luis A.Dova, Maria TeresaThomas P. McCauleyReucroft, StephenSwain, JohnCOSMIC RAYShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1A 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.Fil: Anchordoqui, Luis A.. Northeastern University; Estados UnidosFil: Dova, Maria Teresa. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; ArgentinaFil: Thomas P. McCauley. Northeastern University; Estados UnidosFil: Reucroft, Stephen. Northeastern University; Estados UnidosFil: Swain, John. Northeastern University; Estados UnidosElsevier Science2000-05info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/98577Anchordoqui, Luis A.; Dova, Maria Teresa; Thomas P. McCauley; Reucroft, Stephen ; Swain, John ; Possible explanation for the tail of the cosmic ray spectrum; Elsevier Science; Physics Letters B; 482; 5-2000; 343-3480370-2693CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1016/S0370-2693(00)00534-7info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S0370269300005347?via%3Dihubinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:09:53Zoai:ri.conicet.gov.ar:11336/98577instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:09:53.63CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
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 A.
COSMIC RAYS
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 A.
Dova, Maria Teresa
Thomas P. McCauley
Reucroft, Stephen
Swain, John
author Anchordoqui, Luis A.
author_facet Anchordoqui, Luis A.
Dova, Maria Teresa
Thomas P. McCauley
Reucroft, Stephen
Swain, John
author_role author
author2 Dova, Maria Teresa
Thomas P. McCauley
Reucroft, Stephen
Swain, John
author2_role author
author
author
author
dc.subject.none.fl_str_mv COSMIC RAYS
topic COSMIC RAYS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv 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.
Fil: Anchordoqui, Luis A.. Northeastern University; Estados Unidos
Fil: Dova, Maria Teresa. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina
Fil: Thomas P. McCauley. Northeastern University; Estados Unidos
Fil: Reucroft, Stephen. Northeastern University; Estados Unidos
Fil: Swain, John. Northeastern University; Estados Unidos
description 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.
publishDate 2000
dc.date.none.fl_str_mv 2000-05
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
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://hdl.handle.net/11336/98577
Anchordoqui, Luis A.; Dova, Maria Teresa; Thomas P. McCauley; Reucroft, Stephen ; Swain, John ; Possible explanation for the tail of the cosmic ray spectrum; Elsevier Science; Physics Letters B; 482; 5-2000; 343-348
0370-2693
CONICET Digital
CONICET
url http://hdl.handle.net/11336/98577
identifier_str_mv Anchordoqui, Luis A.; Dova, Maria Teresa; Thomas P. McCauley; Reucroft, Stephen ; Swain, John ; Possible explanation for the tail of the cosmic ray spectrum; Elsevier Science; Physics Letters B; 482; 5-2000; 343-348
0370-2693
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1016/S0370-2693(00)00534-7
info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S0370269300005347?via%3Dihub
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Elsevier Science
publisher.none.fl_str_mv Elsevier Science
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 13.070432

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