The Giant Radio Array for Neutrino Detection

Research output: Contribution to journal › Conference article › peer-review

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

In: E P J Web of Conferences, Vol. 135, 02001, 05.02.2017.

Research output: Contribution to journal › Conference article › peer-review

Harvard

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, vol. 135, 02001. https://doi.org/10.1051/epjconf/201713502001

APA

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

Vancouver

Martineau-Huynh O, Bustamante M, Carvalho W, Charrier D, Jong SD, Vries KDD et al. The Giant Radio Array for Neutrino Detection. E P J Web of Conferences. 2017 Feb 5;135. 02001. https://doi.org/10.1051/epjconf/201713502001

Author

Martineau-Huynh, Olivier ; Bustamante, Mauricio ; Carvalho, Washington ; Charrier, Didier ; Jong, Sijbrand De ; Vries, Krijn D. de ; Fang, Ke ; Feng, Zhaoyang ; Finley, Chad ; Gou, Quanbu ; Gu, Junhua ; Hu, Hongbo ; Kotera, Kumiko ; Coz, Sandra Le ; Medina, Clementina ; Murase, Kohta ; Niess, Valentin ; Oikonomou, Foteini ; Timmermans, Charles ; Wang, Zhen ; Wu, Xiangping ; Zhang, Yi. / The Giant Radio Array for Neutrino Detection. In: E P J Web of Conferences. 2017 ; Vol. 135.

Bibtex

@inproceedings{19ca9f168019446baf0c37727a50d7a0,
title = "The Giant Radio Array for Neutrino Detection",
abstract = "The Giant Radio Array for Neutrino Detection (GRAND) is a planned array of ~200 000 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 3.10$^{16}$ 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.",
keywords = "astro-ph.IM, astro-ph.HE",
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",
note = "4 pages, 2 figures, proceedings of the ARENA2016 conference",
year = "2017",
month = feb,
day = "5",
doi = "10.1051/epjconf/201713502001",
language = "English",
volume = "135",
journal = "EPJ Web of Conferences",
issn = "2101-6275",
publisher = "E D P Sciences",

}

RIS

TY - GEN

T1 - The Giant Radio Array for Neutrino Detection

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

N1 - 4 pages, 2 figures, proceedings of the ARENA2016 conference

PY - 2017/2/5

Y1 - 2017/2/5

N2 - The Giant Radio Array for Neutrino Detection (GRAND) is a planned array of ~200 000 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 3.10$^{16}$ 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.

AB - The Giant Radio Array for Neutrino Detection (GRAND) is a planned array of ~200 000 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 3.10$^{16}$ 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.

KW - astro-ph.IM

KW - astro-ph.HE

U2 - 10.1051/epjconf/201713502001

DO - 10.1051/epjconf/201713502001

M3 - Conference article

VL - 135

JO - EPJ Web of Conferences

JF - EPJ Web of Conferences

SN - 2101-6275

M1 - 02001

ER -

ID: 184745855