Ultra high energy cosmic rays as a probe of black strings
- Autores
- Anjos, Rita C.; Coimbra-Araújo, Carlos H.
- Año de publicación
- 2015
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- Ultrahigh energy cosmic rays (UHECRs) are problably originated in extragalactic sources as, e.g., Active Galactic Nuclei (AGNs). In the present work it is proposed an approach to calculate bounds on the AGN luminosity fraction that can be converted in such UHECRs. This result comes from two separated points of view: (i) the intrinsic mechanism powered by central black holes to produce the AGN luminosity and (ii) the observation of UHECRs and gamma-rays from ground experiments to reconstruct proton luminosities of a given AGN source.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
Ultrahigh energy cosmic rays
black strings - 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:10915/168051
Ver los metadatos del registro completo
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Ultra high energy cosmic rays as a probe of black stringsAnjos, Rita C.Coimbra-Araújo, Carlos H.Ciencias AstronómicasUltrahigh energy cosmic raysblack stringsUltrahigh energy cosmic rays (UHECRs) are problably originated in extragalactic sources as, e.g., Active Galactic Nuclei (AGNs). In the present work it is proposed an approach to calculate bounds on the AGN luminosity fraction that can be converted in such UHECRs. This result comes from two separated points of view: (i) the intrinsic mechanism powered by central black holes to produce the AGN luminosity and (ii) the observation of UHECRs and gamma-rays from ground experiments to reconstruct proton luminosities of a given AGN source.Facultad de Ciencias Astronómicas y Geofísicas2015-10info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionObjeto de conferenciahttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdf125-128http://sedici.unlp.edu.ar/handle/10915/168051enginfo:eu-repo/semantics/altIdentifier/isbn/978-987-24948-3-4info:eu-repo/semantics/reference/url/https://sedici.unlp.edu.ar/handle/10915/167830info: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:UNLP2025-09-29T11:44:46Zoai:sedici.unlp.edu.ar:10915/168051Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-29 11:44:47.161SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
Ultra high energy cosmic rays as a probe of black strings |
| title |
Ultra high energy cosmic rays as a probe of black strings |
| spellingShingle |
Ultra high energy cosmic rays as a probe of black strings Anjos, Rita C. Ciencias Astronómicas Ultrahigh energy cosmic rays black strings |
| title_short |
Ultra high energy cosmic rays as a probe of black strings |
| title_full |
Ultra high energy cosmic rays as a probe of black strings |
| title_fullStr |
Ultra high energy cosmic rays as a probe of black strings |
| title_full_unstemmed |
Ultra high energy cosmic rays as a probe of black strings |
| title_sort |
Ultra high energy cosmic rays as a probe of black strings |
| dc.creator.none.fl_str_mv |
Anjos, Rita C. Coimbra-Araújo, Carlos H. |
| author |
Anjos, Rita C. |
| author_facet |
Anjos, Rita C. Coimbra-Araújo, Carlos H. |
| author_role |
author |
| author2 |
Coimbra-Araújo, Carlos H. |
| author2_role |
author |
| dc.subject.none.fl_str_mv |
Ciencias Astronómicas Ultrahigh energy cosmic rays black strings |
| topic |
Ciencias Astronómicas Ultrahigh energy cosmic rays black strings |
| dc.description.none.fl_txt_mv |
Ultrahigh energy cosmic rays (UHECRs) are problably originated in extragalactic sources as, e.g., Active Galactic Nuclei (AGNs). In the present work it is proposed an approach to calculate bounds on the AGN luminosity fraction that can be converted in such UHECRs. This result comes from two separated points of view: (i) the intrinsic mechanism powered by central black holes to produce the AGN luminosity and (ii) the observation of UHECRs and gamma-rays from ground experiments to reconstruct proton luminosities of a given AGN source. Facultad de Ciencias Astronómicas y Geofísicas |
| description |
Ultrahigh energy cosmic rays (UHECRs) are problably originated in extragalactic sources as, e.g., Active Galactic Nuclei (AGNs). In the present work it is proposed an approach to calculate bounds on the AGN luminosity fraction that can be converted in such UHECRs. This result comes from two separated points of view: (i) the intrinsic mechanism powered by central black holes to produce the AGN luminosity and (ii) the observation of UHECRs and gamma-rays from ground experiments to reconstruct proton luminosities of a given AGN source. |
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2015 |
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2015-10 |
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eng |
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