Radio-detection of neutrino-induced air showers: The influence of topography

Autores
Decoene, V.; Renault-Tinacci, N.; Martineau Huynh, O.; Charrier, D.; Kotera, K.; Le Coz, S.; Niess, V.; Tueros, Matias Jorge; Zilles, A.
Año de publicación
2021
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Neutrinos of astrophysical origin could be detected through the electromagnetic radiation of the particle showers induced in the atmosphere by their interaction in the Earth. This applies in particular for tau neutrinos of energies E>1016eV following Earth-skimming trajectories. The ∼1° beaming of the radio emission in the forward direction however implies that the radio signal will likely fly above a detector deployed over a flat site and would therefore not be detected. We study here how a non-flat detector topography can improve the detection probability of these neutrino-induced air showers. We do this by computing with three distinct tools the neutrino detection efficiency for a radio array deployed over a toy-model mountainous terrain, also taking into account experimental and topographic constraints. We show in particular that ground topographies inclined by few degrees only induce detection efficiencies typically three times larger than those obtained for flat areas for favorable trajectories. We conclude that the topography of the area where the detector is deployed will be a key factor for an experiment like GRAND.
Fil: Decoene, V.. Université Pierre et Marie Curie; Francia
Fil: Renault-Tinacci, N.. Université Pierre et Marie Curie; Francia
Fil: Martineau Huynh, O.. Université Pierre et Marie Curie; Francia
Fil: Charrier, D.. Universite de Nantes; Francia
Fil: Kotera, K.. Université Pierre et Marie Curie; Francia
Fil: Le Coz, S.. Chinese Academy of Sciences; República de China
Fil: Niess, V.. Université Clermont Auvergne; Francia
Fil: Tueros, Matias Jorge. 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
Fil: Zilles, A.. Université Pierre et Marie Curie; Francia
Materia
AIR-SHOWERS
RADIO-DETECTION
ULTRA-HIGH-ENERGY COSMIC-RAYS
ULTRA-HIGH-ENERGY NEUTRINOS
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-nd/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/181059
Acceder
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network_name_str CONICET Digital (CONICET)
spelling Radio-detection of neutrino-induced air showers: The influence of topographyDecoene, V.Renault-Tinacci, N.Martineau Huynh, O.Charrier, D.Kotera, K.Le Coz, S.Niess, V.Tueros, Matias JorgeZilles, A.AIR-SHOWERSRADIO-DETECTIONULTRA-HIGH-ENERGY COSMIC-RAYSULTRA-HIGH-ENERGY NEUTRINOShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Neutrinos of astrophysical origin could be detected through the electromagnetic radiation of the particle showers induced in the atmosphere by their interaction in the Earth. This applies in particular for tau neutrinos of energies E>1016eV following Earth-skimming trajectories. The ∼1° beaming of the radio emission in the forward direction however implies that the radio signal will likely fly above a detector deployed over a flat site and would therefore not be detected. We study here how a non-flat detector topography can improve the detection probability of these neutrino-induced air showers. We do this by computing with three distinct tools the neutrino detection efficiency for a radio array deployed over a toy-model mountainous terrain, also taking into account experimental and topographic constraints. We show in particular that ground topographies inclined by few degrees only induce detection efficiencies typically three times larger than those obtained for flat areas for favorable trajectories. We conclude that the topography of the area where the detector is deployed will be a key factor for an experiment like GRAND.Fil: Decoene, V.. Université Pierre et Marie Curie; FranciaFil: Renault-Tinacci, N.. Université Pierre et Marie Curie; FranciaFil: Martineau Huynh, O.. Université Pierre et Marie Curie; FranciaFil: Charrier, D.. Universite de Nantes; FranciaFil: Kotera, K.. Université Pierre et Marie Curie; FranciaFil: Le Coz, S.. Chinese Academy of Sciences; República de ChinaFil: Niess, V.. Université Clermont Auvergne; FranciaFil: Tueros, Matias Jorge. 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; ArgentinaFil: Zilles, A.. Université Pierre et Marie Curie; FranciaElsevier Science2021-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/181059Decoene, V.; Renault-Tinacci, N.; Martineau Huynh, O.; Charrier, D.; Kotera, K.; et al.; Radio-detection of neutrino-induced air showers: The influence of topography; Elsevier Science; Nuclear Instruments and Methods in Physics Research A: Accelerators, Spectrometers, Detectors and Associated Equipament; 986; 1-2021; 1-300168-9002CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/abs/pii/S0168900220312006info:eu-repo/semantics/altIdentifier/doi/10.1016/j.nima.2020.164803info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-nd/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:33:03Zoai:ri.conicet.gov.ar:11336/181059instacron: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 10:33:03.439CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Radio-detection of neutrino-induced air showers: The influence of topography
title Radio-detection of neutrino-induced air showers: The influence of topography
spellingShingle Radio-detection of neutrino-induced air showers: The influence of topography
Decoene, V.
AIR-SHOWERS
RADIO-DETECTION
ULTRA-HIGH-ENERGY COSMIC-RAYS
ULTRA-HIGH-ENERGY NEUTRINOS
title_short Radio-detection of neutrino-induced air showers: The influence of topography
title_full Radio-detection of neutrino-induced air showers: The influence of topography
title_fullStr Radio-detection of neutrino-induced air showers: The influence of topography
title_full_unstemmed Radio-detection of neutrino-induced air showers: The influence of topography
title_sort Radio-detection of neutrino-induced air showers: The influence of topography
dc.creator.none.fl_str_mv Decoene, V.
Renault-Tinacci, N.
Martineau Huynh, O.
Charrier, D.
Kotera, K.
Le Coz, S.
Niess, V.
Tueros, Matias Jorge
Zilles, A.
author Decoene, V.
author_facet Decoene, V.
Renault-Tinacci, N.
Martineau Huynh, O.
Charrier, D.
Kotera, K.
Le Coz, S.
Niess, V.
Tueros, Matias Jorge
Zilles, A.
author_role author
author2 Renault-Tinacci, N.
Martineau Huynh, O.
Charrier, D.
Kotera, K.
Le Coz, S.
Niess, V.
Tueros, Matias Jorge
Zilles, A.
author2_role author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv AIR-SHOWERS
RADIO-DETECTION
ULTRA-HIGH-ENERGY COSMIC-RAYS
ULTRA-HIGH-ENERGY NEUTRINOS
topic AIR-SHOWERS
RADIO-DETECTION
ULTRA-HIGH-ENERGY COSMIC-RAYS
ULTRA-HIGH-ENERGY NEUTRINOS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Neutrinos of astrophysical origin could be detected through the electromagnetic radiation of the particle showers induced in the atmosphere by their interaction in the Earth. This applies in particular for tau neutrinos of energies E>1016eV following Earth-skimming trajectories. The ∼1° beaming of the radio emission in the forward direction however implies that the radio signal will likely fly above a detector deployed over a flat site and would therefore not be detected. We study here how a non-flat detector topography can improve the detection probability of these neutrino-induced air showers. We do this by computing with three distinct tools the neutrino detection efficiency for a radio array deployed over a toy-model mountainous terrain, also taking into account experimental and topographic constraints. We show in particular that ground topographies inclined by few degrees only induce detection efficiencies typically three times larger than those obtained for flat areas for favorable trajectories. We conclude that the topography of the area where the detector is deployed will be a key factor for an experiment like GRAND.
Fil: Decoene, V.. Université Pierre et Marie Curie; Francia
Fil: Renault-Tinacci, N.. Université Pierre et Marie Curie; Francia
Fil: Martineau Huynh, O.. Université Pierre et Marie Curie; Francia
Fil: Charrier, D.. Universite de Nantes; Francia
Fil: Kotera, K.. Université Pierre et Marie Curie; Francia
Fil: Le Coz, S.. Chinese Academy of Sciences; República de China
Fil: Niess, V.. Université Clermont Auvergne; Francia
Fil: Tueros, Matias Jorge. 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
Fil: Zilles, A.. Université Pierre et Marie Curie; Francia
description Neutrinos of astrophysical origin could be detected through the electromagnetic radiation of the particle showers induced in the atmosphere by their interaction in the Earth. This applies in particular for tau neutrinos of energies E>1016eV following Earth-skimming trajectories. The ∼1° beaming of the radio emission in the forward direction however implies that the radio signal will likely fly above a detector deployed over a flat site and would therefore not be detected. We study here how a non-flat detector topography can improve the detection probability of these neutrino-induced air showers. We do this by computing with three distinct tools the neutrino detection efficiency for a radio array deployed over a toy-model mountainous terrain, also taking into account experimental and topographic constraints. We show in particular that ground topographies inclined by few degrees only induce detection efficiencies typically three times larger than those obtained for flat areas for favorable trajectories. We conclude that the topography of the area where the detector is deployed will be a key factor for an experiment like GRAND.
publishDate 2021
dc.date.none.fl_str_mv 2021-01
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/11336/181059
Decoene, V.; Renault-Tinacci, N.; Martineau Huynh, O.; Charrier, D.; Kotera, K.; et al.; Radio-detection of neutrino-induced air showers: The influence of topography; Elsevier Science; Nuclear Instruments and Methods in Physics Research A: Accelerators, Spectrometers, Detectors and Associated Equipament; 986; 1-2021; 1-30
0168-9002
CONICET Digital
CONICET
url http://hdl.handle.net/11336/181059
identifier_str_mv Decoene, V.; Renault-Tinacci, N.; Martineau Huynh, O.; Charrier, D.; Kotera, K.; et al.; Radio-detection of neutrino-induced air showers: The influence of topography; Elsevier Science; Nuclear Instruments and Methods in Physics Research A: Accelerators, Spectrometers, Detectors and Associated Equipament; 986; 1-2021; 1-30
0168-9002
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/abs/pii/S0168900220312006
info:eu-repo/semantics/altIdentifier/doi/10.1016/j.nima.2020.164803
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-nd/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-nd/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Elsevier Science
publisher.none.fl_str_mv Elsevier Science
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
_version_ 1844614345474965504
score 13.070432

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