Rigidity dependent knee and cosmic ray induced high energy neutrino fluxes
- Autores
- Candia, Julián Marcelo; Roulet, Esteban
- Año de publicación
- 2003
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Scenarios in which the knee of the cosmic ray spectrum depends on the particle rigidities usually predict that the cosmic ray composition becomes heavier above the knee and have associated a change in the spectral slope of each individual nuclear component which is steeper than the change (Δα≃0.3) observed in the total spectrum. We show that this implies that the very high energy (Eν>1014 eV) diffuse neutrino fluxes produced by cosmic rays hitting the atmosphere or colliding with the interstellar medium in the Galaxy will be significantly suppressed, making their detection harder but also reducing the background for the search of other (more challenging) astrophysical neutrino sources.
Facultad de Ciencias Exactas - Materia
-
Física
Cosmic rays
Ultra high energy photons and neutrinos - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/129299
Ver los metadatos del registro completo
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Rigidity dependent knee and cosmic ray induced high energy neutrino fluxesCandia, Julián MarceloRoulet, EstebanFísicaCosmic raysUltra high energy photons and neutrinosScenarios in which the knee of the cosmic ray spectrum depends on the particle rigidities usually predict that the cosmic ray composition becomes heavier above the knee and have associated a change in the spectral slope of each individual nuclear component which is steeper than the change (Δα≃0.3) observed in the total spectrum. We show that this implies that the very high energy (Eν>1014 eV) diffuse neutrino fluxes produced by cosmic rays hitting the atmosphere or colliding with the interstellar medium in the Galaxy will be significantly suppressed, making their detection harder but also reducing the background for the search of other (more challenging) astrophysical neutrino sources.Facultad de Ciencias Exactas2003info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/129299enginfo:eu-repo/semantics/altIdentifier/issn/1475-7516info:eu-repo/semantics/altIdentifier/arxiv/astro-ph/0306632info:eu-repo/semantics/altIdentifier/doi/10.1088/1475-7516/2003/09/005info: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:UNLP2025-09-03T11:03:23Zoai:sedici.unlp.edu.ar:10915/129299Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-03 11:03:23.203SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
Rigidity dependent knee and cosmic ray induced high energy neutrino fluxes |
| title |
Rigidity dependent knee and cosmic ray induced high energy neutrino fluxes |
| spellingShingle |
Rigidity dependent knee and cosmic ray induced high energy neutrino fluxes Candia, Julián Marcelo Física Cosmic rays Ultra high energy photons and neutrinos |
| title_short |
Rigidity dependent knee and cosmic ray induced high energy neutrino fluxes |
| title_full |
Rigidity dependent knee and cosmic ray induced high energy neutrino fluxes |
| title_fullStr |
Rigidity dependent knee and cosmic ray induced high energy neutrino fluxes |
| title_full_unstemmed |
Rigidity dependent knee and cosmic ray induced high energy neutrino fluxes |
| title_sort |
Rigidity dependent knee and cosmic ray induced high energy neutrino fluxes |
| dc.creator.none.fl_str_mv |
Candia, Julián Marcelo Roulet, Esteban |
| author |
Candia, Julián Marcelo |
| author_facet |
Candia, Julián Marcelo Roulet, Esteban |
| author_role |
author |
| author2 |
Roulet, Esteban |
| author2_role |
author |
| dc.subject.none.fl_str_mv |
Física Cosmic rays Ultra high energy photons and neutrinos |
| topic |
Física Cosmic rays Ultra high energy photons and neutrinos |
| dc.description.none.fl_txt_mv |
Scenarios in which the knee of the cosmic ray spectrum depends on the particle rigidities usually predict that the cosmic ray composition becomes heavier above the knee and have associated a change in the spectral slope of each individual nuclear component which is steeper than the change (Δα≃0.3) observed in the total spectrum. We show that this implies that the very high energy (Eν>1014 eV) diffuse neutrino fluxes produced by cosmic rays hitting the atmosphere or colliding with the interstellar medium in the Galaxy will be significantly suppressed, making their detection harder but also reducing the background for the search of other (more challenging) astrophysical neutrino sources. Facultad de Ciencias Exactas |
| description |
Scenarios in which the knee of the cosmic ray spectrum depends on the particle rigidities usually predict that the cosmic ray composition becomes heavier above the knee and have associated a change in the spectral slope of each individual nuclear component which is steeper than the change (Δα≃0.3) observed in the total spectrum. We show that this implies that the very high energy (Eν>1014 eV) diffuse neutrino fluxes produced by cosmic rays hitting the atmosphere or colliding with the interstellar medium in the Galaxy will be significantly suppressed, making their detection harder but also reducing the background for the search of other (more challenging) astrophysical neutrino sources. |
| publishDate |
2003 |
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2003 |
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info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion Articulo http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
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article |
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publishedVersion |
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http://sedici.unlp.edu.ar/handle/10915/129299 |
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| dc.language.none.fl_str_mv |
eng |
| language |
eng |
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openAccess |
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