Detection potential of the KM3NeT detector for high-energy neutrinos from the Fermi bubbles
[EN] A recent analysis of the Fermi Large Area Telescope data provided evidence for a high-intensity emission of high-energy gamma rays with a E- 2 spectrum from two large areas, spanning 50º above and below the Galactic centre (the Fermi bubbles ). A hadronic mechanism was proposed for this gamma-r...
| Autores: | , , , , , , , , , , , , , , |
|---|---|
| Tipo de recurso: | artículo |
| Fecha de publicación: | 2013 |
| País: | España |
| Institución: | Universitat Politècnica de València (UPV) |
| Repositorio: | RiuNet. Repositorio Institucional de la Universitat Politécnica de Valéncia |
| Idioma: | inglés |
| OAI Identifier: | oai:riunet.upv.es:10251/44436 |
| Acceso en línea: | https://riunet.upv.es/handle/10251/44436 |
| Access Level: | acceso abierto |
| Palabra clave: | Neutrino telescope Fermi Bubbles KM3NeT INGENIERIA TELEMATICA |
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Detection potential of the KM3NeT detector for high-energy neutrinos from the Fermi bubblesAdrián Martínez, SilviaAgeron, M.Aguilar, J. A.Aharonian, F.Aiello, S.Albert, A.Alexandri, M.Bou Cabo, ManuelLarosa, GiuseppinaArdid, Miguel|||0000-0002-3199-594XEspinosa Roselló, Víctor|||0000-0001-8882-866XFerri García, MarcelinoLlorens Alvarez, Carlos David|||0000-0002-6675-3596Lloret, Jaime|||0000-0002-0862-0533Martínez Mora, Juan AntonioNeutrino telescopeFermi BubblesKM3NeTINGENIERIA TELEMATICA[EN] A recent analysis of the Fermi Large Area Telescope data provided evidence for a high-intensity emission of high-energy gamma rays with a E- 2 spectrum from two large areas, spanning 50º above and below the Galactic centre (the Fermi bubbles ). A hadronic mechanism was proposed for this gamma-ray emission making the Fermi bubbles promising source candidates of high-energy neutrino emission. In this work Monte Carlo simulations regarding the detectability of high-energy neutrinos from the Fermi bubbles with the future multi-km3 neutrino telescope KM3NeT in the Mediterranean Sea are presented. Under the hypothesis that the gamma-ray emission is completely due to hadronic processes, the results indicate that neutrinos from the bubbles could be discovered in about one year of operation, for a neutrino spectrum with a cutoff at 100 TeV and a detector with about 6 km3 of instrumented volume. The effect of a possible lower cutoff is also considered.The research leading to these results has received funding from the European Community's Sixth Framework Programme under Contract No. 011937 and the Seventh Framework Programme under Grant Agreement No. 212525.ElsevierDepartamento de Física AplicadaDepartamento de ComunicacionesEscuela Técnica Superior de Ingeniería Aeroespacial y Diseño IndustrialEscuela Técnica Superior de Ingeniería Geodésica, Cartográfica y TopográficaEscuela Politécnica Superior de GandiaCentro de Tecnologías Físicas: Acústica, Materiales y AstrofísicaInstituto de Investigación para la Gestión Integrada de Zonas CosterasEuropean CommissionRepositorio Institucional de la Universitat Politècnica de València Riunet20132013-02-01journal articlehttp://purl.org/coar/resource_type/c_6501VoRhttp://purl.org/coar/version/c_970fb48d4fbd8a85info:eu-repo/semantics/articleapplication/pdfapplication/pdfhttps://riunet.upv.es/handle/10251/44436reponame:RiuNet. Repositorio Institucional de la Universitat Politécnica de Valénciainstname:Universitat Politècnica de València (UPV)InglésengEuropean Commission https://doi.org/10.13039/501100000780 FP7 212525 Preparatory Phase for a Deep Sea Facility in the Mediterranean for Neutrino Astronomy and Associated SciencesEuropean Commission https://doi.org/10.13039/501100000780 FP6 011937 KM3NeT Design Studyopen accesshttp://purl.org/coar/access_right/c_abf2Reserva de todos los derechoshttp://rightsstatements.org/vocab/InC/1.0/info:eu-repo/semantics/openAccessoai:riunet.upv.es:10251/444362026-06-13T07:49:27Z |
| dc.title.none.fl_str_mv |
Detection potential of the KM3NeT detector for high-energy neutrinos from the Fermi bubbles |
| title |
Detection potential of the KM3NeT detector for high-energy neutrinos from the Fermi bubbles |
| spellingShingle |
Detection potential of the KM3NeT detector for high-energy neutrinos from the Fermi bubbles Adrián Martínez, Silvia Neutrino telescope Fermi Bubbles KM3NeT INGENIERIA TELEMATICA |
| title_short |
Detection potential of the KM3NeT detector for high-energy neutrinos from the Fermi bubbles |
| title_full |
Detection potential of the KM3NeT detector for high-energy neutrinos from the Fermi bubbles |
| title_fullStr |
Detection potential of the KM3NeT detector for high-energy neutrinos from the Fermi bubbles |
| title_full_unstemmed |
Detection potential of the KM3NeT detector for high-energy neutrinos from the Fermi bubbles |
| title_sort |
Detection potential of the KM3NeT detector for high-energy neutrinos from the Fermi bubbles |
| dc.creator.none.fl_str_mv |
Adrián Martínez, Silvia Ageron, M. Aguilar, J. A. Aharonian, F. Aiello, S. Albert, A. Alexandri, M. Bou Cabo, Manuel Larosa, Giuseppina Ardid, Miguel|||0000-0002-3199-594X Espinosa Roselló, Víctor|||0000-0001-8882-866X Ferri García, Marcelino Llorens Alvarez, Carlos David|||0000-0002-6675-3596 Lloret, Jaime|||0000-0002-0862-0533 Martínez Mora, Juan Antonio |
| author |
Adrián Martínez, Silvia |
| author_facet |
Adrián Martínez, Silvia Ageron, M. Aguilar, J. A. Aharonian, F. Aiello, S. Albert, A. Alexandri, M. Bou Cabo, Manuel Larosa, Giuseppina Ardid, Miguel|||0000-0002-3199-594X Espinosa Roselló, Víctor|||0000-0001-8882-866X Ferri García, Marcelino Llorens Alvarez, Carlos David|||0000-0002-6675-3596 Lloret, Jaime|||0000-0002-0862-0533 Martínez Mora, Juan Antonio |
| author_role |
author |
| author2 |
Ageron, M. Aguilar, J. A. Aharonian, F. Aiello, S. Albert, A. Alexandri, M. Bou Cabo, Manuel Larosa, Giuseppina Ardid, Miguel|||0000-0002-3199-594X Espinosa Roselló, Víctor|||0000-0001-8882-866X Ferri García, Marcelino Llorens Alvarez, Carlos David|||0000-0002-6675-3596 Lloret, Jaime|||0000-0002-0862-0533 Martínez Mora, Juan Antonio |
| author2_role |
author author author author author author author author author author author author author author |
| dc.contributor.none.fl_str_mv |
Departamento de Física Aplicada Departamento de Comunicaciones Escuela Técnica Superior de Ingeniería Aeroespacial y Diseño Industrial Escuela Técnica Superior de Ingeniería Geodésica, Cartográfica y Topográfica Escuela Politécnica Superior de Gandia Centro de Tecnologías Físicas: Acústica, Materiales y Astrofísica Instituto de Investigación para la Gestión Integrada de Zonas Costeras European Commission Repositorio Institucional de la Universitat Politècnica de València Riunet |
| dc.subject.none.fl_str_mv |
Neutrino telescope Fermi Bubbles KM3NeT INGENIERIA TELEMATICA |
| topic |
Neutrino telescope Fermi Bubbles KM3NeT INGENIERIA TELEMATICA |
| description |
[EN] A recent analysis of the Fermi Large Area Telescope data provided evidence for a high-intensity emission of high-energy gamma rays with a E- 2 spectrum from two large areas, spanning 50º above and below the Galactic centre (the Fermi bubbles ). A hadronic mechanism was proposed for this gamma-ray emission making the Fermi bubbles promising source candidates of high-energy neutrino emission. In this work Monte Carlo simulations regarding the detectability of high-energy neutrinos from the Fermi bubbles with the future multi-km3 neutrino telescope KM3NeT in the Mediterranean Sea are presented. Under the hypothesis that the gamma-ray emission is completely due to hadronic processes, the results indicate that neutrinos from the bubbles could be discovered in about one year of operation, for a neutrino spectrum with a cutoff at 100 TeV and a detector with about 6 km3 of instrumented volume. The effect of a possible lower cutoff is also considered. |
| publishDate |
2013 |
| dc.date.none.fl_str_mv |
2013 2013-02-01 |
| dc.type.none.fl_str_mv |
journal article http://purl.org/coar/resource_type/c_6501 VoR http://purl.org/coar/version/c_970fb48d4fbd8a85 |
| dc.type.openaire.fl_str_mv |
info:eu-repo/semantics/article |
| format |
article |
| dc.identifier.none.fl_str_mv |
https://riunet.upv.es/handle/10251/44436 |
| url |
https://riunet.upv.es/handle/10251/44436 |
| dc.language.none.fl_str_mv |
Inglés eng |
| language_invalid_str_mv |
Inglés |
| language |
eng |
| dc.relation.none.fl_str_mv |
European Commission https://doi.org/10.13039/501100000780 FP7 212525 Preparatory Phase for a Deep Sea Facility in the Mediterranean for Neutrino Astronomy and Associated Sciences European Commission https://doi.org/10.13039/501100000780 FP6 011937 KM3NeT Design Study |
| dc.rights.none.fl_str_mv |
open access http://purl.org/coar/access_right/c_abf2 Reserva de todos los derechos http://rightsstatements.org/vocab/InC/1.0/ |
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info:eu-repo/semantics/openAccess |
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open access http://purl.org/coar/access_right/c_abf2 Reserva de todos los derechos http://rightsstatements.org/vocab/InC/1.0/ |
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openAccess |
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application/pdf application/pdf |
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Elsevier |
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Elsevier |
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reponame:RiuNet. Repositorio Institucional de la Universitat Politécnica de Valéncia instname:Universitat Politècnica de València (UPV) |
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Universitat Politècnica de València (UPV) |
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RiuNet. Repositorio Institucional de la Universitat Politécnica de Valéncia |
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RiuNet. Repositorio Institucional de la Universitat Politécnica de Valéncia |
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