The Giant Radio Array for Neutrino Detection

Olivier Martineau-Huynh; Kumiko Kotera; Mauricio Bustamente; Didier Charrier; Sijbrand De Jong; Krijn D. De Vries; Ke Fang; Zhaoyang Feng; Chad Finley; Quanbu Gou; Junhua Gu; Jordan C. Hanson; Hongbo Hu; Kohta Murase; Valentin Niess; Foteini Oikonomou; Nicolas Renault-Tinacci; Julia Schmid; Charles Timmermans; Zhen Wang; Xiangping Wu; Jianli Zhang; Yi Zhang

doi:10.1051/epjconf/201611603005

The Giant Radio Array for Neutrino Detection

Olivier Martineau-Huynh, Kumiko Kotera, Mauricio Bustamente, Didier Charrier, Sijbrand De Jong, Krijn D. De Vries, Ke Fang, Zhaoyang Feng, Chad Finley, Quanbu Gou, Junhua Gu, Jordan C. Hanson, Hongbo Hu, Kohta Murase, Valentin Niess, Foteini Oikonomou, Nicolas Renault-Tinacci, Julia Schmid, Charles Timmermans, Zhen WangXiangping Wu, Jianli Zhang, Yi Zhang

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

24 Scopus citations

Abstract

High-energy neutrino astronomy will probe the working of the most violent phenomena in the Universe. The Giant Radio Array for Neutrino Detection (GRAND) project consists of an array of ∼ 10⁵ radio antennas deployed over ∼ 200 000 km² in a mountainous site. It aims at detecting high-energy neutrinos via the measurement of air showers induced by the decay in the atmosphere of τ leptons produced by the interaction of cosmic neutrinos under the Earth surface. Our objective with GRAND is to reach a neutrino sensitivity of 5 × 10^-11E^-2 GeV^-1 cm^-2 s^-1 sr^-1 above 3 × 10¹⁶ eV. This sensitivity ensures the detection of cosmogenic neutrinos in the most pessimistic source models, and up to 100 events per year are expected for the standard models. GRAND would also probe the neutrino signals produced at the potential sources of UHECRs.

Original language	English (US)
Title of host publication	Very Large Volume Neutrino Telescope, VLVnT 2015
Editors	Giulia De Bonis, Antonio Capone, Irene Di Palma, Chiara Perrina
Publisher	EDP Sciences
ISBN (Electronic)	9782759820160
DOIs	https://doi.org/10.1051/epjconf/201611603005
State	Published - Apr 11 2016
Event	7th Biannual Very Large Volume Neutrino Telescope Workshop, VLVnT 2015 - Roma, Italy Duration: Sep 14 2015 → Sep 16 2015

Publication series

Name	EPJ Web of Conferences
Volume	116
ISSN (Print)	2101-6275
ISSN (Electronic)	2100-014X

Other

Other	7th Biannual Very Large Volume Neutrino Telescope Workshop, VLVnT 2015
Country/Territory	Italy
City	Roma
Period	9/14/15 → 9/16/15

All Science Journal Classification (ASJC) codes

General Physics and Astronomy

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10.1051/epjconf/201611603005

Cite this

Martineau-Huynh, O., Kotera, K., Bustamente, M., Charrier, D., De Jong, S., De Vries, K. D., Fang, K., Feng, Z., Finley, C., Gou, Q., Gu, J., Hanson, J. C., Hu, H., Murase, K., Niess, V., Oikonomou, F., Renault-Tinacci, N., Schmid, J., Timmermans, C., ... Zhang, Y. (2016). The Giant Radio Array for Neutrino Detection. In G. De Bonis, A. Capone, I. Di Palma, & C. Perrina (Eds.), Very Large Volume Neutrino Telescope, VLVnT 2015 Article 03005 (EPJ Web of Conferences; Vol. 116). EDP Sciences. https://doi.org/10.1051/epjconf/201611603005

@inproceedings{b2d9d27af8d04bec89c64f18574d1edc,

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

abstract = "High-energy neutrino astronomy will probe the working of the most violent phenomena in the Universe. The Giant Radio Array for Neutrino Detection (GRAND) project consists of an array of ∼ 105 radio antennas deployed over ∼ 200 000 km2 in a mountainous site. It aims at detecting high-energy neutrinos via the measurement of air showers induced by the decay in the atmosphere of τ leptons produced by the interaction of cosmic neutrinos under the Earth surface. Our objective with GRAND is to reach a neutrino sensitivity of 5 × 10-11E-2 GeV-1 cm-2 s-1 sr-1 above 3 × 1016 eV. This sensitivity ensures the detection of cosmogenic neutrinos in the most pessimistic source models, and up to 100 events per year are expected for the standard models. GRAND would also probe the neutrino signals produced at the potential sources of UHECRs.",

author = "Olivier Martineau-Huynh and Kumiko Kotera and Mauricio Bustamente and Didier Charrier and {De Jong}, Sijbrand and {De Vries}, {Krijn D.} and Ke Fang and Zhaoyang Feng and Chad Finley and Quanbu Gou and Junhua Gu and Hanson, {Jordan C.} and Hongbo Hu and Kohta Murase and Valentin Niess and Foteini Oikonomou and Nicolas Renault-Tinacci and Julia Schmid and Charles Timmermans and Zhen Wang and Xiangping Wu and Jianli Zhang and Yi Zhang",

note = "Publisher Copyright: {\textcopyright} Owned by the authors, published by EDP Sciences, 2016.; 7th Biannual Very Large Volume Neutrino Telescope Workshop, VLVnT 2015 ; Conference date: 14-09-2015 Through 16-09-2015",

year = "2016",

month = apr,

day = "11",

doi = "10.1051/epjconf/201611603005",

language = "English (US)",

series = "EPJ Web of Conferences",

publisher = "EDP Sciences",

editor = "{De Bonis}, Giulia and Antonio Capone and {Di Palma}, Irene and Chiara Perrina",

booktitle = "Very Large Volume Neutrino Telescope, VLVnT 2015",

address = "France",

}

Martineau-Huynh, O, Kotera, K, Bustamente, M, Charrier, D, De Jong, S, De Vries, KD, Fang, K, Feng, Z, Finley, C, Gou, Q, Gu, J, Hanson, JC, Hu, H, Murase, K, Niess, V, Oikonomou, F, Renault-Tinacci, N, Schmid, J, Timmermans, C, Wang, Z, Wu, X, Zhang, J & Zhang, Y 2016, The Giant Radio Array for Neutrino Detection. in G De Bonis, A Capone, I Di Palma & C Perrina (eds), Very Large Volume Neutrino Telescope, VLVnT 2015., 03005, EPJ Web of Conferences, vol. 116, EDP Sciences, 7th Biannual Very Large Volume Neutrino Telescope Workshop, VLVnT 2015, Roma, Italy, 9/14/15. https://doi.org/10.1051/epjconf/201611603005

The Giant Radio Array for Neutrino Detection. / Martineau-Huynh, Olivier; Kotera, Kumiko; Bustamente, Mauricio et al.
Very Large Volume Neutrino Telescope, VLVnT 2015. ed. / Giulia De Bonis; Antonio Capone; Irene Di Palma; Chiara Perrina. EDP Sciences, 2016. 03005 (EPJ Web of Conferences; Vol. 116).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

TY - GEN

T1 - The Giant Radio Array for Neutrino Detection

AU - Martineau-Huynh, Olivier

AU - Kotera, Kumiko

AU - Bustamente, Mauricio

AU - Charrier, Didier

AU - De Jong, Sijbrand

AU - De Vries, Krijn D.

AU - Fang, Ke

AU - Feng, Zhaoyang

AU - Finley, Chad

AU - Gou, Quanbu

AU - Gu, Junhua

AU - Hanson, Jordan C.

AU - Hu, Hongbo

AU - Murase, Kohta

AU - Niess, Valentin

AU - Oikonomou, Foteini

AU - Renault-Tinacci, Nicolas

AU - Schmid, Julia

AU - Timmermans, Charles

AU - Wang, Zhen

AU - Wu, Xiangping

AU - Zhang, Jianli

AU - Zhang, Yi

PY - 2016/4/11

Y1 - 2016/4/11

N2 - High-energy neutrino astronomy will probe the working of the most violent phenomena in the Universe. The Giant Radio Array for Neutrino Detection (GRAND) project consists of an array of ∼ 105 radio antennas deployed over ∼ 200 000 km2 in a mountainous site. It aims at detecting high-energy neutrinos via the measurement of air showers induced by the decay in the atmosphere of τ leptons produced by the interaction of cosmic neutrinos under the Earth surface. Our objective with GRAND is to reach a neutrino sensitivity of 5 × 10-11E-2 GeV-1 cm-2 s-1 sr-1 above 3 × 1016 eV. This sensitivity ensures the detection of cosmogenic neutrinos in the most pessimistic source models, and up to 100 events per year are expected for the standard models. GRAND would also probe the neutrino signals produced at the potential sources of UHECRs.

AB - High-energy neutrino astronomy will probe the working of the most violent phenomena in the Universe. The Giant Radio Array for Neutrino Detection (GRAND) project consists of an array of ∼ 105 radio antennas deployed over ∼ 200 000 km2 in a mountainous site. It aims at detecting high-energy neutrinos via the measurement of air showers induced by the decay in the atmosphere of τ leptons produced by the interaction of cosmic neutrinos under the Earth surface. Our objective with GRAND is to reach a neutrino sensitivity of 5 × 10-11E-2 GeV-1 cm-2 s-1 sr-1 above 3 × 1016 eV. This sensitivity ensures the detection of cosmogenic neutrinos in the most pessimistic source models, and up to 100 events per year are expected for the standard models. GRAND would also probe the neutrino signals produced at the potential sources of UHECRs.

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DO - 10.1051/epjconf/201611603005

M3 - Conference contribution

AN - SCOPUS:84969752496

T3 - EPJ Web of Conferences

BT - Very Large Volume Neutrino Telescope, VLVnT 2015

A2 - De Bonis, Giulia

A2 - Capone, Antonio

A2 - Di Palma, Irene

A2 - Perrina, Chiara

PB - EDP Sciences

T2 - 7th Biannual Very Large Volume Neutrino Telescope Workshop, VLVnT 2015

Y2 - 14 September 2015 through 16 September 2015

ER -

The Giant Radio Array for Neutrino Detection

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