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The Giant Radio Array for Neutrino Detection (GRAND) : Science and design. / Alvarez-Muniz, Jaime; Batista, Rafael Alves; Balagopal, Aswathi; Bolmont, Julien; Bustamante, Mauricio; Carvalho, Washington; Charrier, Didier; Cognard, Ismael; Decoene, Valentin; Denton, Peter B.; De Jong, Sijbrand; De Vries, Krijn D.; Engel, Ralph; Fang, Ke; Finley, Chad; Gabici, Stefano; Gou, QuanBu; Gu, JunHua; Guepin, Claire; Hu, HongBo; Huang, Yan; Kotera, Kumiko; Le Coz, Sandra; Lenain, Jean-Philippe; Lu, GuoLiang; Martineau-Huynh, Olivier; Mostafa, Miguel; Mottez, Fabrice; Murase, Kohta; Niess, Valentin; Oikonomou, Foteini; Pierog, Tanguy; Qian, XiangLi; Qin, Bo; Ran, Duan; Renault-Tinacci, Nicolas; Roth, Markus; Schroeder, Frank G.; Schussler, Fabian; Tasse, Cyril; Timmermans, Charles; Tueros, Matias; Wu, XiangPing; Zarka, Philippe; Zech, Andreas; Zhang, B. Theodore; Zhang, JianLi; Zhang, Yi; Zheng, Qian; Zilles, Anne; GRAND Collaboration.
I:
Science China Physics, Mechanics and Astronomy, Bind 63, Nr. 1, 219501, 04.08.2020.
Publikation: Bidrag til tidsskrift › Review › Forskning › fagfællebedømt
Harvard
Alvarez-Muniz, J, Batista, RA, Balagopal, A, Bolmont, J
, Bustamante, M, Carvalho, W, Charrier, D, Cognard, I, Decoene, V, Denton, PB, De Jong, S, De Vries, KD, Engel, R, Fang, K, Finley, C, Gabici, S, Gou, Q, Gu, J, Guepin, C, Hu, H, Huang, Y, Kotera, K, Le Coz, S, Lenain, J-P, Lu, G, Martineau-Huynh, O, Mostafa, M, Mottez, F, Murase, K, Niess, V, Oikonomou, F, Pierog, T, Qian, X, Qin, B, Ran, D, Renault-Tinacci, N, Roth, M, Schroeder, FG, Schussler, F, Tasse, C, Timmermans, C, Tueros, M, Wu, X, Zarka, P, Zech, A, Zhang, BT, Zhang, J, Zhang, Y, Zheng, Q, Zilles, A & GRAND Collaboration 2020, '
The Giant Radio Array for Neutrino Detection (GRAND): Science and design',
Science China Physics, Mechanics and Astronomy, bind 63, nr. 1, 219501.
https://doi.org/10.1007/s11433-018-9385-7APA
Alvarez-Muniz, J., Batista, R. A., Balagopal, A., Bolmont, J.
, Bustamante, M., Carvalho, W., Charrier, D., Cognard, I., Decoene, V., Denton, P. B., De Jong, S., De Vries, K. D., Engel, R., Fang, K., Finley, C., Gabici, S., Gou, Q., Gu, J., Guepin, C., ... GRAND Collaboration (2020).
The Giant Radio Array for Neutrino Detection (GRAND): Science and design.
Science China Physics, Mechanics and Astronomy,
63(1), [219501].
https://doi.org/10.1007/s11433-018-9385-7Vancouver
Alvarez-Muniz J, Batista RA, Balagopal A, Bolmont J
, Bustamante M, Carvalho W o.a.
The Giant Radio Array for Neutrino Detection (GRAND): Science and design.
Science China Physics, Mechanics and Astronomy. 2020 aug. 4;63(1). 219501.
https://doi.org/10.1007/s11433-018-9385-7Author
Alvarez-Muniz, Jaime ; Batista, Rafael Alves ; Balagopal, Aswathi ; Bolmont, Julien ; Bustamante, Mauricio ; Carvalho, Washington ; Charrier, Didier ; Cognard, Ismael ; Decoene, Valentin ; Denton, Peter B. ; De Jong, Sijbrand ; De Vries, Krijn D. ; Engel, Ralph ; Fang, Ke ; Finley, Chad ; Gabici, Stefano ; Gou, QuanBu ; Gu, JunHua ; Guepin, Claire ; Hu, HongBo ; Huang, Yan ; Kotera, Kumiko ; Le Coz, Sandra ; Lenain, Jean-Philippe ; Lu, GuoLiang ; Martineau-Huynh, Olivier ; Mostafa, Miguel ; Mottez, Fabrice ; Murase, Kohta ; Niess, Valentin ; Oikonomou, Foteini ; Pierog, Tanguy ; Qian, XiangLi ; Qin, Bo ; Ran, Duan ; Renault-Tinacci, Nicolas ; Roth, Markus ; Schroeder, Frank G. ; Schussler, Fabian ; Tasse, Cyril ; Timmermans, Charles ; Tueros, Matias ; Wu, XiangPing ; Zarka, Philippe ; Zech, Andreas ; Zhang, B. Theodore ; Zhang, JianLi ; Zhang, Yi ; Zheng, Qian ; Zilles, Anne ; GRAND Collaboration. / The Giant Radio Array for Neutrino Detection (GRAND) : Science and design. I: Science China Physics, Mechanics and Astronomy. 2020 ; Bind 63, Nr. 1.
Bibtex
@article{3220909e8ffe4582a9eb0c76a99af021,
title = "The Giant Radio Array for Neutrino Detection (GRAND): Science and design",
abstract = "The Giant Radio Array for Neutrino Detection (GRAND) is a planned large-scale observatory of ultra-high-energy (UHE) cosmic particles, with energies exceeding 108 GeV. Its goal is to solve the long-standing mystery of the origin of UHE cosmic rays. To do this, GRAND will detect an unprecedented number of UHE cosmic rays and search for the undiscovered UHE neutrinos and gamma rays associated to them with unmatched sensitivity. GRAND will use large arrays of antennas to detect the radio emission coming from extensive air showers initiated by UHE particles in the atmosphere. Its design is modular: 20 separate, independent sub-arrays, each of 10000 radio antennas deployed over 10000 km(2). A staged construction plan will validate key detection techniques while achieving important science goals early. Here we present the science goals, detection strategy, preliminary design, performance goals, and construction plans for GRAND.",
keywords = "radio telescopes, neutrinos in astronomical observations, cosmic rays in astronomical observations, radiowave radiation: sources, galactic and extragalactic, cosmic rays: galactic and extragalactic, HIGH-ENERGY NEUTRINOS, EXTENSIVE AIR-SHOWERS, COSMIC-RAYS, PAIR PRODUCTION, SPECTRUM, SIMULATIONS, EMISSION, PULSES, BURST, LIMIT",
author = "Jaime Alvarez-Muniz and Batista, {Rafael Alves} and Aswathi Balagopal and Julien Bolmont and Mauricio Bustamante and Washington Carvalho and Didier Charrier and Ismael Cognard and Valentin Decoene and Denton, {Peter B.} and {De Jong}, Sijbrand and {De Vries}, {Krijn D.} and Ralph Engel and Ke Fang and Chad Finley and Stefano Gabici and QuanBu Gou and JunHua Gu and Claire Guepin and HongBo Hu and Yan Huang and Kumiko Kotera and {Le Coz}, Sandra and Jean-Philippe Lenain and GuoLiang Lu and Olivier Martineau-Huynh and Miguel Mostafa and Fabrice Mottez and Kohta Murase and Valentin Niess and Foteini Oikonomou and Tanguy Pierog and XiangLi Qian and Bo Qin and Duan Ran and Nicolas Renault-Tinacci and Markus Roth and Schroeder, {Frank G.} and Fabian Schussler and Cyril Tasse and Charles Timmermans and Matias Tueros and XiangPing Wu and Philippe Zarka and Andreas Zech and Zhang, {B. Theodore} and JianLi Zhang and Yi Zhang and Qian Zheng and Anne Zilles and {GRAND Collaboration}",
year = "2020",
month = aug,
day = "4",
doi = "10.1007/s11433-018-9385-7",
language = "English",
volume = "63",
journal = "Science China Physics, Mechanics and Astronomy",
issn = "1674-7348",
publisher = "Zhongguo Kexue Zazhishe",
number = "1",
}
RIS
TY - JOUR
T1 - The Giant Radio Array for Neutrino Detection (GRAND)
T2 - Science and design
AU - Alvarez-Muniz, Jaime
AU - Batista, Rafael Alves
AU - Balagopal, Aswathi
AU - Bolmont, Julien
AU - Bustamante, Mauricio
AU - Carvalho, Washington
AU - Charrier, Didier
AU - Cognard, Ismael
AU - Decoene, Valentin
AU - Denton, Peter B.
AU - De Jong, Sijbrand
AU - De Vries, Krijn D.
AU - Engel, Ralph
AU - Fang, Ke
AU - Finley, Chad
AU - Gabici, Stefano
AU - Gou, QuanBu
AU - Gu, JunHua
AU - Guepin, Claire
AU - Hu, HongBo
AU - Huang, Yan
AU - Kotera, Kumiko
AU - Le Coz, Sandra
AU - Lenain, Jean-Philippe
AU - Lu, GuoLiang
AU - Martineau-Huynh, Olivier
AU - Mostafa, Miguel
AU - Mottez, Fabrice
AU - Murase, Kohta
AU - Niess, Valentin
AU - Oikonomou, Foteini
AU - Pierog, Tanguy
AU - Qian, XiangLi
AU - Qin, Bo
AU - Ran, Duan
AU - Renault-Tinacci, Nicolas
AU - Roth, Markus
AU - Schroeder, Frank G.
AU - Schussler, Fabian
AU - Tasse, Cyril
AU - Timmermans, Charles
AU - Tueros, Matias
AU - Wu, XiangPing
AU - Zarka, Philippe
AU - Zech, Andreas
AU - Zhang, B. Theodore
AU - Zhang, JianLi
AU - Zhang, Yi
AU - Zheng, Qian
AU - Zilles, Anne
AU - GRAND Collaboration
PY - 2020/8/4
Y1 - 2020/8/4
N2 - The Giant Radio Array for Neutrino Detection (GRAND) is a planned large-scale observatory of ultra-high-energy (UHE) cosmic particles, with energies exceeding 108 GeV. Its goal is to solve the long-standing mystery of the origin of UHE cosmic rays. To do this, GRAND will detect an unprecedented number of UHE cosmic rays and search for the undiscovered UHE neutrinos and gamma rays associated to them with unmatched sensitivity. GRAND will use large arrays of antennas to detect the radio emission coming from extensive air showers initiated by UHE particles in the atmosphere. Its design is modular: 20 separate, independent sub-arrays, each of 10000 radio antennas deployed over 10000 km(2). A staged construction plan will validate key detection techniques while achieving important science goals early. Here we present the science goals, detection strategy, preliminary design, performance goals, and construction plans for GRAND.
AB - The Giant Radio Array for Neutrino Detection (GRAND) is a planned large-scale observatory of ultra-high-energy (UHE) cosmic particles, with energies exceeding 108 GeV. Its goal is to solve the long-standing mystery of the origin of UHE cosmic rays. To do this, GRAND will detect an unprecedented number of UHE cosmic rays and search for the undiscovered UHE neutrinos and gamma rays associated to them with unmatched sensitivity. GRAND will use large arrays of antennas to detect the radio emission coming from extensive air showers initiated by UHE particles in the atmosphere. Its design is modular: 20 separate, independent sub-arrays, each of 10000 radio antennas deployed over 10000 km(2). A staged construction plan will validate key detection techniques while achieving important science goals early. Here we present the science goals, detection strategy, preliminary design, performance goals, and construction plans for GRAND.
KW - radio telescopes
KW - neutrinos in astronomical observations
KW - cosmic rays in astronomical observations
KW - radiowave radiation: sources
KW - galactic and extragalactic
KW - cosmic rays: galactic and extragalactic
KW - HIGH-ENERGY NEUTRINOS
KW - EXTENSIVE AIR-SHOWERS
KW - COSMIC-RAYS
KW - PAIR PRODUCTION
KW - SPECTRUM
KW - SIMULATIONS
KW - EMISSION
KW - PULSES
KW - BURST
KW - LIMIT
U2 - 10.1007/s11433-018-9385-7
DO - 10.1007/s11433-018-9385-7
M3 - Review
VL - 63
JO - Science China Physics, Mechanics and Astronomy
JF - Science China Physics, Mechanics and Astronomy
SN - 1674-7348
IS - 1
M1 - 219501
ER -
