Producción y propagación de neutrones en jets de microcuásares

Autores
Escobar, Gastón Javier
Año de publicación
2018
Idioma
español castellano
Tipo de recurso
artículo
Estado
versión publicada
Descripción
A usual investigation line to address the study of jets nature and composition is to determine the energetics of the relativistic particles populations which are present in the jet, and the electromagnetic radiation emitted by them. The neutron component, originated in situ through interactions of relativistic protons with matter or radiation, has not been studied in microquasars. The neutrons, when decaying or interacting with matter or radiation fields, introduce new relativistic electron and proton sources, distributing the latter populations along the jet. Since neutrons do not interact with magnetic fields, their dynamics are distinct to that of charged particles. This allows neutrons to escape from the acceleration region easier than other particles, taking an energy fraction away of the system. In this work we introduce the relativistic neutron component in the study of energetics of relativistic particles of microquasar jets. We model the spectral energy distributions with a One-Zone approximation to solve the appropriate transport equations.
Fil: Escobar, Gastón Javier. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
Materia
X-ray binaries
Radiation mechanisms
Relativistic processes
Stars
Non thermal mechanisms
Jets
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:11336/93353
Acceder
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network_name_str CONICET Digital (CONICET)
spelling Producción y propagación de neutrones en jets de microcuásaresEscobar, Gastón JavierX-ray binariesRadiation mechanismsRelativistic processesStarsNon thermal mechanismsJetshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1A usual investigation line to address the study of jets nature and composition is to determine the energetics of the relativistic particles populations which are present in the jet, and the electromagnetic radiation emitted by them. The neutron component, originated in situ through interactions of relativistic protons with matter or radiation, has not been studied in microquasars. The neutrons, when decaying or interacting with matter or radiation fields, introduce new relativistic electron and proton sources, distributing the latter populations along the jet. Since neutrons do not interact with magnetic fields, their dynamics are distinct to that of charged particles. This allows neutrons to escape from the acceleration region easier than other particles, taking an energy fraction away of the system. In this work we introduce the relativistic neutron component in the study of energetics of relativistic particles of microquasar jets. We model the spectral energy distributions with a One-Zone approximation to solve the appropriate transport equations.Fil: Escobar, Gastón Javier. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; ArgentinaAsociación Argentina de Astronomía2018-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/93353Escobar, Gastón Javier; Producción y propagación de neutrones en jets de microcuásares; Asociación Argentina de Astronomía; Boletín de la Asociación Argentina de Astronomía; 60; 8-2018; 95-971669-9521CONICET DigitalCONICETspainfo:eu-repo/semantics/altIdentifier/url/http://articles.adsabs.harvard.edu/pdf/2018BAAA...60...95Einfo:eu-repo/semantics/altIdentifier/url/http://www.astronomiaargentina.org.ar/uploads/docs/baaa_60.pdfinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:45:52Zoai:ri.conicet.gov.ar:11336/93353instacron: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 10:45:53.116CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Producción y propagación de neutrones en jets de microcuásares
title Producción y propagación de neutrones en jets de microcuásares
spellingShingle Producción y propagación de neutrones en jets de microcuásares
Escobar, Gastón Javier
X-ray binaries
Radiation mechanisms
Relativistic processes
Stars
Non thermal mechanisms
Jets
title_short Producción y propagación de neutrones en jets de microcuásares
title_full Producción y propagación de neutrones en jets de microcuásares
title_fullStr Producción y propagación de neutrones en jets de microcuásares
title_full_unstemmed Producción y propagación de neutrones en jets de microcuásares
title_sort Producción y propagación de neutrones en jets de microcuásares
dc.creator.none.fl_str_mv Escobar, Gastón Javier
author Escobar, Gastón Javier
author_facet Escobar, Gastón Javier
author_role author
dc.subject.none.fl_str_mv X-ray binaries
Radiation mechanisms
Relativistic processes
Stars
Non thermal mechanisms
Jets
topic X-ray binaries
Radiation mechanisms
Relativistic processes
Stars
Non thermal mechanisms
Jets
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 usual investigation line to address the study of jets nature and composition is to determine the energetics of the relativistic particles populations which are present in the jet, and the electromagnetic radiation emitted by them. The neutron component, originated in situ through interactions of relativistic protons with matter or radiation, has not been studied in microquasars. The neutrons, when decaying or interacting with matter or radiation fields, introduce new relativistic electron and proton sources, distributing the latter populations along the jet. Since neutrons do not interact with magnetic fields, their dynamics are distinct to that of charged particles. This allows neutrons to escape from the acceleration region easier than other particles, taking an energy fraction away of the system. In this work we introduce the relativistic neutron component in the study of energetics of relativistic particles of microquasar jets. We model the spectral energy distributions with a One-Zone approximation to solve the appropriate transport equations.
Fil: Escobar, Gastón Javier. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina
description A usual investigation line to address the study of jets nature and composition is to determine the energetics of the relativistic particles populations which are present in the jet, and the electromagnetic radiation emitted by them. The neutron component, originated in situ through interactions of relativistic protons with matter or radiation, has not been studied in microquasars. The neutrons, when decaying or interacting with matter or radiation fields, introduce new relativistic electron and proton sources, distributing the latter populations along the jet. Since neutrons do not interact with magnetic fields, their dynamics are distinct to that of charged particles. This allows neutrons to escape from the acceleration region easier than other particles, taking an energy fraction away of the system. In this work we introduce the relativistic neutron component in the study of energetics of relativistic particles of microquasar jets. We model the spectral energy distributions with a One-Zone approximation to solve the appropriate transport equations.
publishDate 2018
dc.date.none.fl_str_mv 2018-08
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/11336/93353
Escobar, Gastón Javier; Producción y propagación de neutrones en jets de microcuásares; Asociación Argentina de Astronomía; Boletín de la Asociación Argentina de Astronomía; 60; 8-2018; 95-97
1669-9521
CONICET Digital
CONICET
url http://hdl.handle.net/11336/93353
identifier_str_mv Escobar, Gastón Javier; Producción y propagación de neutrones en jets de microcuásares; Asociación Argentina de Astronomía; Boletín de la Asociación Argentina de Astronomía; 60; 8-2018; 95-97
1669-9521
CONICET Digital
CONICET
dc.language.none.fl_str_mv spa
language spa
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://articles.adsabs.harvard.edu/pdf/2018BAAA...60...95E
info:eu-repo/semantics/altIdentifier/url/http://www.astronomiaargentina.org.ar/uploads/docs/baaa_60.pdf
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 Asociación Argentina de Astronomía
publisher.none.fl_str_mv Asociación Argentina de Astronomía
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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