TY - JOUR
T1 - GRANDLIB
T2 - A simulation pipeline for the Giant Radio Array for Neutrino Detection (GRAND)
AU - The GRAND collaboration
AU - Alves Batista, R.
AU - Benoit-Lévy, A.
AU - Bister, T.
AU - Bohacova, M.
AU - Bustamante, M.
AU - Carvalho, W.
AU - Chen, Y.
AU - Cheng, L.
AU - Chiche, S.
AU - Colley, J. M.
AU - Correa, P.
AU - Cucu Laurenciu, N.
AU - Dai, Z.
AU - de Almeida, R. M.
AU - de Errico, B.
AU - de Jong, S.
AU - de Mello Neto, J. R.T.
AU - de Vries, K. D.
AU - Decoene, V.
AU - Denton, P. B.
AU - Duan, B.
AU - Duan, K.
AU - Engel, R.
AU - Erba, W.
AU - Fan, Y.
AU - Ferrière, A.
AU - Gou, Q.
AU - Gu, J.
AU - Guelfand, M.
AU - Guo, J.
AU - Guo, Y.
AU - Guépin, C.
AU - Gülzow, L.
AU - Haungs, A.
AU - Havelka, M.
AU - He, H.
AU - Hivon, E.
AU - Hu, H.
AU - Huang, X.
AU - Huang, Y.
AU - Huege, T.
AU - Jiang, W.
AU - Koirala, R.
AU - Kong, C.
AU - Kotera, K.
AU - Köhler, J.
AU - Lago, B. L.
AU - Lai, Z.
AU - Mostafá, M.
AU - Murase, K.
N1 - Publisher Copyright:
© 2024
PY - 2025/3
Y1 - 2025/3
N2 - The operation of upcoming ultra-high-energy cosmic-ray, gamma-ray, and neutrino radio-detection experiments, like the Giant Radio Array for Neutrino Detection (GRAND), poses significant computational challenges involving the production of numerous simulations of particle showers and their detection, and a high data throughput. GRANDLIB is an open-source software tool designed to meet these challenges. Its primary goal is to perform end-to-end simulations of the detector operation, from the interaction of ultra-high-energy particles, through—by interfacing with external air-shower simulations—the ensuing particle shower development and its radio emission, to its detection by antenna arrays and its processing by data-acquisition systems. Additionally, GRANDLIB manages the visualization, storage, and retrieval of experimental and simulated data. We present an overview of GRANDLIB to serve as the basis of future GRAND analyses.
AB - The operation of upcoming ultra-high-energy cosmic-ray, gamma-ray, and neutrino radio-detection experiments, like the Giant Radio Array for Neutrino Detection (GRAND), poses significant computational challenges involving the production of numerous simulations of particle showers and their detection, and a high data throughput. GRANDLIB is an open-source software tool designed to meet these challenges. Its primary goal is to perform end-to-end simulations of the detector operation, from the interaction of ultra-high-energy particles, through—by interfacing with external air-shower simulations—the ensuing particle shower development and its radio emission, to its detection by antenna arrays and its processing by data-acquisition systems. Additionally, GRANDLIB manages the visualization, storage, and retrieval of experimental and simulated data. We present an overview of GRANDLIB to serve as the basis of future GRAND analyses.
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U2 - 10.1016/j.cpc.2024.109461
DO - 10.1016/j.cpc.2024.109461
M3 - Article
AN - SCOPUS:85211445955
SN - 0010-4655
VL - 308
JO - Computer Physics Communications
JF - Computer Physics Communications
M1 - 109461
ER -