References
Works cited across this documentation. Entries are taken from INSPIRE-HEP, so the keys match the ones the literature uses and can be pasted straight into a paper.
GRANDlib itself performs comparatively little physics: air showers and their radio emission come from ZHAireS [1] or CoREAS [5], tau propagation from DANTON [8] and terrain from TURTLE [7]. The pipeline itself is described in [2], the experiment in [9] and offline signal identification for GRANDProto300 in [6]. Related frameworks in the same field are NuRadioMC [4] and the Pierre Auger Observatory’s Offline [3].
See How to cite for how to cite GRANDlib.
Jaime Alvarez-Muniz, Washington R. Carvalho, Jr., Matias Tueros, and Enrique Zas. Coherent Cherenkov radio pulses from hadronic showers up to EeV energies. Astropart. Phys., 35:287–299, 2012. arXiv:1005.0552, doi:10.1016/j.astropartphys.2011.10.002.
Rafael Alves Batista and others. GRANDlib: A simulation pipeline for the Giant Radio Array for Neutrino Detection (GRAND). Comput. Phys. Commun., 308:109461, 2025. arXiv:2408.10926, doi:10.1016/j.cpc.2024.109461.
S. Argiro, S. L. C. Barroso, J. Gonzalez, L. Nellen, Thomas Cantzon Paul, T. A. Porter, L. Prado, Jr., M. Roth, R. Ulrich, and D. Veberic. The Offline Software Framework of the Pierre Auger Observatory. Nucl. Instrum. Meth. A, 580:1485–1496, 2007. arXiv:0707.1652, doi:10.1016/j.nima.2007.07.010.
Christian Glaser and others. NuRadioMC: Simulating the radio emission of neutrinos from interaction to detector. Eur. Phys. J. C, 80(2):77, 2020. arXiv:1906.01670, doi:10.1140/epjc/s10052-020-7612-8.
T. Huege, M. Ludwig, and C. W. James. Simulating radio emission from air showers with CoREAS. AIP Conf. Proc., 1535(1):128, 2013. arXiv:1301.2132, doi:10.1063/1.4807534.
Pragati Mitra. Offline Signal Identification with GRANDProto300. PoS, ICRC2023:236, 2023. arXiv:2307.09600, doi:10.22323/1.444.0236.
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Jaime Álvarez-Muñiz and others. The Giant Radio Array for Neutrino Detection (GRAND): Science and Design. Sci. China Phys. Mech. Astron., 63(1):219501, 2020. arXiv:1810.09994, doi:10.1007/s11433-018-9385-7.