Detection of neutrinos from micro-quasars II
- Autores
- Mosquera, Mercedes Elisa; Civitarese, Enrique Osvaldo
- Año de publicación
- 2012
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Considering a system composed of a compact object and a star subrounded by wind, and using models for high-energy proton emission from micro-quasars, we calculate the neutrino flux resulting from protonproton collisions, with and without including neutrino oscillations. It is found that the flux of neutrinos from a windy micro-quasar is affected by neutrino oscillations, and that it reflects upon the increase in the time of observation, by a factor of the order 23. © 2012 World Scientific Publishing Company.
Fil: Mosquera, Mercedes Elisa. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Civitarese, Enrique Osvaldo. 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 - Materia
-
Cosmic Rays
Astronomial Observations
Windy Quasar
Neutrino Oscillation - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/74682
Ver los metadatos del registro completo
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Detection of neutrinos from micro-quasars IIMosquera, Mercedes ElisaCivitarese, Enrique OsvaldoCosmic RaysAstronomial ObservationsWindy QuasarNeutrino Oscillationhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Considering a system composed of a compact object and a star subrounded by wind, and using models for high-energy proton emission from micro-quasars, we calculate the neutrino flux resulting from protonproton collisions, with and without including neutrino oscillations. It is found that the flux of neutrinos from a windy micro-quasar is affected by neutrino oscillations, and that it reflects upon the increase in the time of observation, by a factor of the order 23. © 2012 World Scientific Publishing Company.Fil: Mosquera, Mercedes Elisa. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Civitarese, Enrique Osvaldo. 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; ArgentinaWorld Scientific2012-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/74682Mosquera, Mercedes Elisa; Civitarese, Enrique Osvaldo; Detection of neutrinos from micro-quasars II; World Scientific; International Journal of Modern Physics E - Nuclear Physics; 21; 10; 10-2012; 1250086-12500990218-3013CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1142/S0218301312500863info:eu-repo/semantics/altIdentifier/url/https://www.worldscientific.com/doi/abs/10.1142/S0218301312500863info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:27:16Zoai:ri.conicet.gov.ar:11336/74682instacron: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:34982025-10-22 11:27:16.436CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
Detection of neutrinos from micro-quasars II |
| title |
Detection of neutrinos from micro-quasars II |
| spellingShingle |
Detection of neutrinos from micro-quasars II Mosquera, Mercedes Elisa Cosmic Rays Astronomial Observations Windy Quasar Neutrino Oscillation |
| title_short |
Detection of neutrinos from micro-quasars II |
| title_full |
Detection of neutrinos from micro-quasars II |
| title_fullStr |
Detection of neutrinos from micro-quasars II |
| title_full_unstemmed |
Detection of neutrinos from micro-quasars II |
| title_sort |
Detection of neutrinos from micro-quasars II |
| dc.creator.none.fl_str_mv |
Mosquera, Mercedes Elisa Civitarese, Enrique Osvaldo |
| author |
Mosquera, Mercedes Elisa |
| author_facet |
Mosquera, Mercedes Elisa Civitarese, Enrique Osvaldo |
| author_role |
author |
| author2 |
Civitarese, Enrique Osvaldo |
| author2_role |
author |
| dc.subject.none.fl_str_mv |
Cosmic Rays Astronomial Observations Windy Quasar Neutrino Oscillation |
| topic |
Cosmic Rays Astronomial Observations Windy Quasar Neutrino Oscillation |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
Considering a system composed of a compact object and a star subrounded by wind, and using models for high-energy proton emission from micro-quasars, we calculate the neutrino flux resulting from protonproton collisions, with and without including neutrino oscillations. It is found that the flux of neutrinos from a windy micro-quasar is affected by neutrino oscillations, and that it reflects upon the increase in the time of observation, by a factor of the order 23. © 2012 World Scientific Publishing Company. Fil: Mosquera, Mercedes Elisa. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Civitarese, Enrique Osvaldo. 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 |
| description |
Considering a system composed of a compact object and a star subrounded by wind, and using models for high-energy proton emission from micro-quasars, we calculate the neutrino flux resulting from protonproton collisions, with and without including neutrino oscillations. It is found that the flux of neutrinos from a windy micro-quasar is affected by neutrino oscillations, and that it reflects upon the increase in the time of observation, by a factor of the order 23. © 2012 World Scientific Publishing Company. |
| publishDate |
2012 |
| dc.date.none.fl_str_mv |
2012-10 |
| 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 |
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article |
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publishedVersion |
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http://hdl.handle.net/11336/74682 Mosquera, Mercedes Elisa; Civitarese, Enrique Osvaldo; Detection of neutrinos from micro-quasars II; World Scientific; International Journal of Modern Physics E - Nuclear Physics; 21; 10; 10-2012; 1250086-1250099 0218-3013 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/74682 |
| identifier_str_mv |
Mosquera, Mercedes Elisa; Civitarese, Enrique Osvaldo; Detection of neutrinos from micro-quasars II; World Scientific; International Journal of Modern Physics E - Nuclear Physics; 21; 10; 10-2012; 1250086-1250099 0218-3013 CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
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eng |
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World Scientific |
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World Scientific |
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