The Giant Radio Array for Neutrino Detection

Olivier Martineau-Huynh; Mauricio Bustamante; Washington Carvalho; Didier Charrier; Sijbrand De Jong; Krijn D. de Vries; Ke Fang; Zhaoyang Feng; Chad Finley; Quanbu Gou; Junhua Gu; Hongbo Hu; Kumiko Kotera; Sandra Le Coz; Clementina Medina; Kohta Murase; Valentin Niess; Foteini Oikonomou; Charles Timmermans; Zhen Wang; Xiangping Wu; Yi Zhang

doi:10.1051/epjconf/201713502001

The Giant Radio Array for Neutrino Detection

Olivier Martineau-Huynh, Mauricio Bustamante, Washington Carvalho, Didier Charrier, Sijbrand De Jong, Krijn D. de Vries, Ke Fang, Zhaoyang Feng, Chad Finley, Quanbu Gou, Junhua Gu, Hongbo Hu, Kumiko Kotera, Sandra Le Coz, Clementina Medina, Kohta Murase, Valentin Niess, Foteini Oikonomou, Charles Timmermans, Zhen WangXiangping Wu, Yi Zhang

Teoretisk højenergi, astropartikel og gravitationel fysik

12 Citationer (Scopus)

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Abstract

The Giant Radio Array for Neutrino Detection (GRAND) is a planned array of ∼ 2·10⁵ radio antennas deployed over ∼ 200 000 km² 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 · 10^-11 E^-2 GeV^-1 cm^-2 s^-1 sr^-1 above 3 · 10¹⁶ 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].

Originalsprog	Engelsk
Artikelnummer	02001
Tidsskrift	E P J Web of Conferences
Vol/bind	135
ISSN	2100-014X
DOI	https://doi.org/10.1051/epjconf/201713502001
Status	Udgivet - 15 mar. 2017

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10.1051/epjconf/201713502001

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Martineau-Huynh, O., Bustamante, M., Carvalho, W., Charrier, D., Jong, S. D., Vries, K. D. D., Fang, K., Feng, Z., Finley, C., Gou, Q., Gu, J., Hu, H., Kotera, K., Coz, S. L., Medina, C., Murase, K., Niess, V., Oikonomou, F., Timmermans, C., ... Zhang, Y. (2017). The Giant Radio Array for Neutrino Detection. E P J Web of Conferences, 135, [02001]. https://doi.org/10.1051/epjconf/201713502001

Martineau-Huynh, O, Bustamante, M, Carvalho, W, Charrier, D, Jong, SD, Vries, KDD, Fang, K, Feng, Z, Finley, C, Gou, Q, Gu, J, Hu, H, Kotera, K, Coz, SL, Medina, C, Murase, K, Niess, V, Oikonomou, F, Timmermans, C, Wang, Z, Wu, X & Zhang, Y 2017, 'The Giant Radio Array for Neutrino Detection', E P J Web of Conferences, bind 135, 02001. https://doi.org/10.1051/epjconf/201713502001

@inproceedings{19ca9f168019446baf0c37727a50d7a0,

title = "The Giant Radio Array for Neutrino Detection",

abstract = "The Giant Radio Array for Neutrino Detection (GRAND) is a planned array of ∼ 2·105 radio antennas deployed over ∼ 200 000 km2 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 · 10-11 E-2 GeV-1 cm-2 s-1 sr-1 above 3 · 1016 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].",

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author = "Olivier Martineau-Huynh and Mauricio Bustamante and Washington Carvalho and Didier Charrier and Jong, {Sijbrand De} and Vries, {Krijn D. de} and Ke Fang and Zhaoyang Feng and Chad Finley and Quanbu Gou and Junhua Gu and Hongbo Hu and Kumiko Kotera and Coz, {Sandra Le} and Clementina Medina and Kohta Murase and Valentin Niess and Foteini Oikonomou and Charles Timmermans and Zhen Wang and Xiangping Wu and Yi Zhang",

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AU - Martineau-Huynh, Olivier

AU - Bustamante, Mauricio

AU - Carvalho, Washington

AU - Charrier, Didier

AU - Jong, Sijbrand De

AU - Vries, Krijn D. de

AU - Fang, Ke

AU - Feng, Zhaoyang

AU - Finley, Chad

AU - Gou, Quanbu

AU - Gu, Junhua

AU - Hu, Hongbo

AU - Kotera, Kumiko

AU - Coz, Sandra Le

AU - Medina, Clementina

AU - Murase, Kohta

AU - Niess, Valentin

AU - Oikonomou, Foteini

AU - Timmermans, Charles

AU - Wang, Zhen

AU - Wu, Xiangping

AU - Zhang, Yi

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PY - 2017/3/15

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N2 - The Giant Radio Array for Neutrino Detection (GRAND) is a planned array of ∼ 2·105 radio antennas deployed over ∼ 200 000 km2 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 · 10-11 E-2 GeV-1 cm-2 s-1 sr-1 above 3 · 1016 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].

AB - The Giant Radio Array for Neutrino Detection (GRAND) is a planned array of ∼ 2·105 radio antennas deployed over ∼ 200 000 km2 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 · 10-11 E-2 GeV-1 cm-2 s-1 sr-1 above 3 · 1016 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].

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KW - astro-ph.HE

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JO - EPJ Web of Conferences

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ER -

The Giant Radio Array for Neutrino Detection

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