The Giant Radio Array for Neutrino Detection

Autores: Martineau Huynh, Olivier; Bustamante, Mauricio; Carvalho, Washington; Charrier, Didier; De Jong, Sijbrand; D. de Vries, Krijn; Fang, Ke; Feng, Zhaoyang; Finley, Chad; Gou, Quanbu; Gu, Junhua; Hu, Hongbo; Kotera, Kumiko; Le Coz, Sandra; Medina, Maria Clementina; Murase, Kohta; Niess, Valentin; Oikonomou, Foteini; Timmermans, Charles; Wang, Zhen; Wu, Xiangping; Zhang, Yi; The GRAND collaboration
Año de publicación: 2017
Idioma: inglés
Tipo de recurso: documento de conferencia
Estado: versión publicada
Descripción: The Giant Radio Array for Neutrino Detection (GRAND) is a planned arrayof ~2x10^{5} radio antennas deployed over ∼ 200 000 km^2 in a mountainous site. It aims primarly at detecting high-energy neutrinos via the observation of extensive air showers induced by the decay in the atmosphere of taus produced by the interaction of cosmic neutrinos under the Earth surface. GRAND aims at reaching a neutrino sensitivity of 5 x 10^{−11}E^{−2} GeV^{−1}cm^{−2} s^{−1}{sr−1} above 3x10^{16} eV. This ensures the detection of cosmogenic neutrinos in the most pessimistic source models, and ∼50 events per year are expected for the standard models. The instrument will also detect UHECRs and possibly FRBs. Here we show how our preliminary design should enable us to reach our sensitivity goals, and discuss the steps to be taken to achieve GRAND, while the compelling science case for GRAND is discussed in more details in [1].
Fil: Martineau Huynh, Olivier. Laboratoire de Physique Nucléaire Des Hautes Énergies; Francia
Fil: Bustamante, Mauricio. Center For Cosmology And Astroparticle Physics; Estados Unidos
Fil: Carvalho, Washington. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; Brasil
Fil: Charrier, Didier. Subatech Laboratory; Francia
Fil: De Jong, Sijbrand. Nikhef/radboud University; Países Bajos
Fil: D. de Vries, Krijn. Vrije Universiteit Brussel; Bélgica
Fil: Fang, Ke. University of Maryland; Estados Unidos
Fil: Feng, Zhaoyang. Key Lab of Particle Astrophysics; China
Fil: Finley, Chad. Oskar Klein Centre And Dept. Of Physics; Suecia
Fil: Gou, Quanbu. Key Lab of Particle Astrophysics; China
Fil: Gu, Junhua. Chinese Academy of Sciences; República de China
Fil: Hu, Hongbo. Key Lab of Particle Astrophysics; China
Fil: Kotera, Kumiko. Institut Astrophysique de Paris; Francia
Fil: Le Coz, Sandra. Chinese Academy of Sciences; República de China
Fil: Medina, Maria Clementina. 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
Fil: Murase, Kohta. Penn State University; Estados Unidos
Fil: Niess, Valentin. Universite Blaise Pascal; Francia
Fil: Oikonomou, Foteini. Penn State University; Estados Unidos
Fil: Timmermans, Charles. Nikhef/Radboud University; Países Bajos
Fil: Wang, Zhen. Key Lab of Particle Astrophysics; China
Fil: Wu, Xiangping. National Astronomical Observatory; China
Fil: Zhang, Yi. Key Lab of Particle Astrophysics; China
Fil: The GRAND collaboration. No especifíca;
7th International Conference on Acoustic and Radio EeV Neutrino Detection Activities
Groningen
Países Bajos
GRAND Collaboration
Materia: Astrophysics
Instrumentation and Methods for Astrophysics
High Energy Astrophysical Phenomena
Neutrinos
Nivel de accesibilidad: acceso abierto
Condiciones de uso: https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
Institución: Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador: oai:ri.conicet.gov.ar:11336/138587

Acceder

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spelling	The Giant Radio Array for Neutrino DetectionMartineau Huynh, OlivierBustamante, MauricioCarvalho, WashingtonCharrier, DidierDe Jong, SijbrandD. de Vries, KrijnFang, KeFeng, ZhaoyangFinley, ChadGou, QuanbuGu, JunhuaHu, HongboKotera, KumikoLe Coz, SandraMedina, Maria ClementinaMurase, KohtaNiess, ValentinOikonomou, FoteiniTimmermans, CharlesWang, ZhenWu, XiangpingZhang, YiThe GRAND collaborationAstrophysicsInstrumentation and Methods for AstrophysicsHigh Energy Astrophysical PhenomenaNeutrinoshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The Giant Radio Array for Neutrino Detection (GRAND) is a planned arrayof ~2x10^{5} radio antennas deployed over ∼ 200 000 km^2 in a mountainous site. It aims primarly at detecting high-energy neutrinos via the observation of extensive air showers induced by the decay in the atmosphere of taus produced by the interaction of cosmic neutrinos under the Earth surface. GRAND aims at reaching a neutrino sensitivity of 5 x 10^{−11}E^{−2} GeV^{−1}cm^{−2} s^{−1}{sr−1} above 3x10^{16} eV. This ensures the detection of cosmogenic neutrinos in the most pessimistic source models, and ∼50 events per year are expected for the standard models. The instrument will also detect UHECRs and possibly FRBs. Here we show how our preliminary design should enable us to reach our sensitivity goals, and discuss the steps to be taken to achieve GRAND, while the compelling science case for GRAND is discussed in more details in [1].Fil: Martineau Huynh, Olivier. Laboratoire de Physique Nucléaire Des Hautes Énergies; FranciaFil: Bustamante, Mauricio. Center For Cosmology And Astroparticle Physics; Estados UnidosFil: Carvalho, Washington. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; BrasilFil: Charrier, Didier. Subatech Laboratory; FranciaFil: De Jong, Sijbrand. Nikhef/radboud University; Países BajosFil: D. de Vries, Krijn. Vrije Universiteit Brussel; BélgicaFil: Fang, Ke. University of Maryland; Estados UnidosFil: Feng, Zhaoyang. Key Lab of Particle Astrophysics; ChinaFil: Finley, Chad. Oskar Klein Centre And Dept. Of Physics; SueciaFil: Gou, Quanbu. Key Lab of Particle Astrophysics; ChinaFil: Gu, Junhua. Chinese Academy of Sciences; República de ChinaFil: Hu, Hongbo. Key Lab of Particle Astrophysics; ChinaFil: Kotera, Kumiko. Institut Astrophysique de Paris; FranciaFil: Le Coz, Sandra. Chinese Academy of Sciences; República de ChinaFil: Medina, Maria Clementina. 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; ArgentinaFil: Murase, Kohta. Penn State University; Estados UnidosFil: Niess, Valentin. Universite Blaise Pascal; FranciaFil: Oikonomou, Foteini. Penn State University; Estados UnidosFil: Timmermans, Charles. Nikhef/Radboud University; Países BajosFil: Wang, Zhen. Key Lab of Particle Astrophysics; ChinaFil: Wu, Xiangping. National Astronomical Observatory; ChinaFil: Zhang, Yi. Key Lab of Particle Astrophysics; ChinaFil: The GRAND collaboration. No especifíca;7th International Conference on Acoustic and Radio EeV Neutrino Detection ActivitiesGroningenPaíses BajosGRAND CollaborationEDP SciencesBuitink, S.2017info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectConferenciaJournalhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/138587The Giant Radio Array for Neutrino Detection; 7th International Conference on Acoustic and Radio EeV Neutrino Detection Activities; Groningen; Países Bajos; 2016; 02001, 1-4978-2-7598-9015-62100-014XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.epj-conferences.org/articles/epjconf/abs/2017/04/epjconf_arena2017_02001/epjconf_arena2017_02001.htmlinfo:eu-repo/semantics/altIdentifier/doi/10.1051/epjconf/201713502001Internacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:22:22Zoai:ri.conicet.gov.ar:11336/138587instacron: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 11:22:23.17CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv	The Giant Radio Array for Neutrino Detection
title	The Giant Radio Array for Neutrino Detection
spellingShingle	The Giant Radio Array for Neutrino Detection Martineau Huynh, Olivier Astrophysics Instrumentation and Methods for Astrophysics High Energy Astrophysical Phenomena Neutrinos
title_short	The Giant Radio Array for Neutrino Detection
title_full	The Giant Radio Array for Neutrino Detection
title_fullStr	The Giant Radio Array for Neutrino Detection
title_full_unstemmed	The Giant Radio Array for Neutrino Detection
title_sort	The Giant Radio Array for Neutrino Detection
dc.creator.none.fl_str_mv	Martineau Huynh, Olivier Bustamante, Mauricio Carvalho, Washington Charrier, Didier De Jong, Sijbrand D. de Vries, Krijn Fang, Ke Feng, Zhaoyang Finley, Chad Gou, Quanbu Gu, Junhua Hu, Hongbo Kotera, Kumiko Le Coz, Sandra Medina, Maria Clementina Murase, Kohta Niess, Valentin Oikonomou, Foteini Timmermans, Charles Wang, Zhen Wu, Xiangping Zhang, Yi The GRAND collaboration
author	Martineau Huynh, Olivier
author_facet	Martineau Huynh, Olivier Bustamante, Mauricio Carvalho, Washington Charrier, Didier De Jong, Sijbrand D. de Vries, Krijn Fang, Ke Feng, Zhaoyang Finley, Chad Gou, Quanbu Gu, Junhua Hu, Hongbo Kotera, Kumiko Le Coz, Sandra Medina, Maria Clementina Murase, Kohta Niess, Valentin Oikonomou, Foteini Timmermans, Charles Wang, Zhen Wu, Xiangping Zhang, Yi The GRAND collaboration
author_role	author
author2	Bustamante, Mauricio Carvalho, Washington Charrier, Didier De Jong, Sijbrand D. de Vries, Krijn Fang, Ke Feng, Zhaoyang Finley, Chad Gou, Quanbu Gu, Junhua Hu, Hongbo Kotera, Kumiko Le Coz, Sandra Medina, Maria Clementina Murase, Kohta Niess, Valentin Oikonomou, Foteini Timmermans, Charles Wang, Zhen Wu, Xiangping Zhang, Yi The GRAND collaboration
author2_role	author author author author author author author author author author author author author author author author author author author author author author
dc.contributor.none.fl_str_mv	Buitink, S.
dc.subject.none.fl_str_mv	Astrophysics Instrumentation and Methods for Astrophysics High Energy Astrophysical Phenomena Neutrinos
topic	Astrophysics Instrumentation and Methods for Astrophysics High Energy Astrophysical Phenomena 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	The Giant Radio Array for Neutrino Detection (GRAND) is a planned arrayof ~2x10^{5} radio antennas deployed over ∼ 200 000 km^2 in a mountainous site. It aims primarly at detecting high-energy neutrinos via the observation of extensive air showers induced by the decay in the atmosphere of taus produced by the interaction of cosmic neutrinos under the Earth surface. GRAND aims at reaching a neutrino sensitivity of 5 x 10^{−11}E^{−2} GeV^{−1}cm^{−2} s^{−1}{sr−1} above 3x10^{16} eV. This ensures the detection of cosmogenic neutrinos in the most pessimistic source models, and ∼50 events per year are expected for the standard models. The instrument will also detect UHECRs and possibly FRBs. Here we show how our preliminary design should enable us to reach our sensitivity goals, and discuss the steps to be taken to achieve GRAND, while the compelling science case for GRAND is discussed in more details in [1]. Fil: Martineau Huynh, Olivier. Laboratoire de Physique Nucléaire Des Hautes Énergies; Francia Fil: Bustamante, Mauricio. Center For Cosmology And Astroparticle Physics; Estados Unidos Fil: Carvalho, Washington. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; Brasil Fil: Charrier, Didier. Subatech Laboratory; Francia Fil: De Jong, Sijbrand. Nikhef/radboud University; Países Bajos Fil: D. de Vries, Krijn. Vrije Universiteit Brussel; Bélgica Fil: Fang, Ke. University of Maryland; Estados Unidos Fil: Feng, Zhaoyang. Key Lab of Particle Astrophysics; China Fil: Finley, Chad. Oskar Klein Centre And Dept. Of Physics; Suecia Fil: Gou, Quanbu. Key Lab of Particle Astrophysics; China Fil: Gu, Junhua. Chinese Academy of Sciences; República de China Fil: Hu, Hongbo. Key Lab of Particle Astrophysics; China Fil: Kotera, Kumiko. Institut Astrophysique de Paris; Francia Fil: Le Coz, Sandra. Chinese Academy of Sciences; República de China Fil: Medina, Maria Clementina. 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 Fil: Murase, Kohta. Penn State University; Estados Unidos Fil: Niess, Valentin. Universite Blaise Pascal; Francia Fil: Oikonomou, Foteini. Penn State University; Estados Unidos Fil: Timmermans, Charles. Nikhef/Radboud University; Países Bajos Fil: Wang, Zhen. Key Lab of Particle Astrophysics; China Fil: Wu, Xiangping. National Astronomical Observatory; China Fil: Zhang, Yi. Key Lab of Particle Astrophysics; China Fil: The GRAND collaboration. No especifíca; 7th International Conference on Acoustic and Radio EeV Neutrino Detection Activities Groningen Países Bajos GRAND Collaboration
description	The Giant Radio Array for Neutrino Detection (GRAND) is a planned arrayof ~2x10^{5} radio antennas deployed over ∼ 200 000 km^2 in a mountainous site. It aims primarly at detecting high-energy neutrinos via the observation of extensive air showers induced by the decay in the atmosphere of taus produced by the interaction of cosmic neutrinos under the Earth surface. GRAND aims at reaching a neutrino sensitivity of 5 x 10^{−11}E^{−2} GeV^{−1}cm^{−2} s^{−1}{sr−1} above 3x10^{16} eV. This ensures the detection of cosmogenic neutrinos in the most pessimistic source models, and ∼50 events per year are expected for the standard models. The instrument will also detect UHECRs and possibly FRBs. Here we show how our preliminary design should enable us to reach our sensitivity goals, and discuss the steps to be taken to achieve GRAND, while the compelling science case for GRAND is discussed in more details in [1].
publishDate	2017
dc.date.none.fl_str_mv	2017
dc.type.none.fl_str_mv	info:eu-repo/semantics/publishedVersion info:eu-repo/semantics/conferenceObject Conferencia Journal http://purl.org/coar/resource_type/c_5794 info:ar-repo/semantics/documentoDeConferencia
status_str	publishedVersion
format	conferenceObject
dc.identifier.none.fl_str_mv	http://hdl.handle.net/11336/138587 The Giant Radio Array for Neutrino Detection; 7th International Conference on Acoustic and Radio EeV Neutrino Detection Activities; Groningen; Países Bajos; 2016; 02001, 1-4 978-2-7598-9015-6 2100-014X CONICET Digital CONICET
url	http://hdl.handle.net/11336/138587
identifier_str_mv	The Giant Radio Array for Neutrino Detection; 7th International Conference on Acoustic and Radio EeV Neutrino Detection Activities; Groningen; Países Bajos; 2016; 02001, 1-4 978-2-7598-9015-6 2100-014X 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.epj-conferences.org/articles/epjconf/abs/2017/04/epjconf_arena2017_02001/epjconf_arena2017_02001.html info:eu-repo/semantics/altIdentifier/doi/10.1051/epjconf/201713502001
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dc.coverage.none.fl_str_mv	Internacional
dc.publisher.none.fl_str_mv	EDP Sciences
publisher.none.fl_str_mv	EDP Sciences
dc.source.none.fl_str_mv	reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str	CONICET Digital (CONICET)
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repository.mail.fl_str_mv	dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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The Giant Radio Array for Neutrino Detection

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