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gSeaGen: The KM3NeT GENIE-based code for neutrino telescopes
Aiello, S.; Albert, A.; Garre, S. Alves; Aly, Z.; Ameli, F.; Andre, M.; Androulakis, G.; Anghinolfi, M.; Anguita, M.; Anton, G.; Ardid, M.; Aublin, J.; Bagatelas, C.; Barbarino, G.; Baret, B.; Basegmez du Pree, S.; Bendahman, M.; Berbee, E.; van den Berg, A.M.; Bertin, V.; Biagi, S.; Biagioni, A.; Bissinger, M.; Boettcher, M.; Boumaaza, J.; Bouta, M.; Bouwhuis, M.; Bozza, C.; Brânzaş, H.; Bruchner, M.; Bruijn, R.; Brunner, J.; Buis, E.; Buompane, R.; Busto, J.; Calvo, D.; Capone, A.; Carretero, V.; Castaldi, P.; Celli, S.; Chabab, M.; Chau, N.; Chen, A.; Cherubini, S.; Chiarella, V.; Chiarusi, T.; Circella, M.; Cocimano, R.; Coelho, J.A.B.; Coleiro, A.; Molla, M. Colomer; Coniglione, R.; Corredoira, I.; Coyle, P.; Creusot, A.; Cuttone, G.; D’Onofrio, A.; Dallier, R.; De Palma, M.; Di Palma, I.; Díaz, A.F.; Diego-Tortosa, D.; Distefano, C.; Domi, A.; Donà, R.; Donzaud, C.; Dornic, D.; Dörr, M.; Drouhin, D.; Durocher, M.; Eberl, T.; van Eijk, D.; El Bojaddaini, I.; Elsaesser, D.; Enzenhöfer, A.; Roselló, V. Espinosa; Fermani, P.; Ferrara, G.; Filipović, M.D.; Filippini, F.; Franco, A.; Fusco, L.A.; Gabella, O.; Gal, T.; Soto, A. Garcia; Garufi, F.; Gatelet, Y.; Geißelbrecht, N.; Gialanella, L.; Giorgio, E.; Gozzini, S.R.; Gracia, R.; Graf, K.; Grasso, D.; Grella, G.; Guderian, D.; Guidi, C.; Hallmann, S.; Hamdaoui, H.; van Haren, H.; Heijboer, A.; Hekalo, A.; Hernández-Rey, J.J.; Hofestädt, J.; Huang, F.; Ibnsalih, W. Idrissi; Illuminati, G.; James, C.W.; de Jong, M.; de Jong, P.; Jung, B.J.; Kadler, M.; Kalaczyński, P.; Kalekin, O.; Katz, U.F.; Chowdhury, N.R. Khan; van der Knaap, F.; Koffeman, E.N.; Kooijman, P.; Kouchner, A.; Kreter, M.; Kulikovskiy, V.; Lahmann, R.; Larosa, G.; Le Breton, R.; Leonardi, O.; Leone, F.; Leonora, E.; Levi, G.; Lincetto, M.; Lindsey Clark, M.; Lipreau, T.; Lonardo, A.; Longhitano, F.; Lopez-Coto, D.; Maderer, L.; Mańczak, J.; Mannheim, K.; Margiotta, A.; Marinelli, A.; Markou, C.; Martin, L.; Martínez-Mora, J.A.; Martini, A.; Marzaioli, F.; Mastroianni, S.; Mazzou, S.; Melis, K.W.; Miele, G.; Migliozzi, P.; Migneco, E.; Mijakowski, P.; Miranda, L.S.; Modebadze, Z.; Mollo, C.M.; Morganti, M.; Moser, M.; Moussa, A.; Muller, R.; Musumeci, M.; Nauta, L.; Navas, S.; Nicolau, C.A.; Ó Fearraigh, B.; Organokov, M.; Orlando, A.; Papalashvili, G.; Papaleo, R.; Pastore, C.; Paun, A.M.; Păvălaş, G.E.; Pellegrino, C.; Perrin-Terrin, M.; Piattelli, P.; Pieterse, C.; Pikounis, K.; Pisanti, O.; Poirè, C.; Popa, V.; Post, M.; Pradier, T.; Pühlhofer, G.; Pulvirenti, S.; Quinn, L.; Rabyang, O.; Raffaelli, F.; Randazzo, N.; Rapicavoli, A.; Razzaque, S.; Real, D.; Reck, S.; Reubelt, J.; Riccobene, G.; Richer, M.; Rivoire, S.; Rovelli, A.; Greus, F. Salesa; Samtleben, D.F.E.; Losa, A. Sánchez; Sanguineti, M.; Santangelo, A.; Santonocito, D.; Sapienza, P.; Schnabel, J.; Sciacca, V.; Seneca, J.; Sgura, I.; Shanidze, R.; Sharma, A.; Simeone, F.; Sinopoulou, A.; Spisso, B.; Spurio, M.; Stavropoulos, D.; Steijger, J.; Stellacci, S.M.; Taiuti, M.; Tayalati, Y.; Tenllado, E.; Thakore, T.; Tingay, S.; Tzamariudaki, E.; Tzanetatos, D.; Van Elewyck, V.; Vannoye, G.; Vasileiadis, G.; Versari, F.; Viola, S.; Vivolo, D.; de Wasseige, G.; Wilms, J.; Wojaczyński, R.; de Wolf, E.; Zaborov, D.; Zavatarelli, S.; Zegarelli, A.; Zornoza, J.D.; Zúñiga, J.; Zywucka, N. (2020). gSeaGen: The KM3NeT GENIE-based code for neutrino telescopes. Computer Physics Communications 256: 107477. https://dx.doi.org/10.1016/j.cpc.2020.107477
In: Computer Physics Communications. ELSEVIER SCIENCE BV: Amsterdam. ISSN 0010-4655; e-ISSN 1879-2944, more
Peer reviewed article  

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Author keywords
    Astroparticle physics; High energy neutrinos; Monte Carlo event generator; Neutrino telescopes; Neutrino oscillations; KM3NeTGENIE

Abstract
    The gSeaGen code is a GENIE-based application developed to efficiently generate high statistics samples of events, induced by neutrino interactions, detectable in a neutrino telescope. The gSeaGen code is able to generate events induced by all neutrino flavours, considering topological differences between track-type and shower-like events. Neutrino interactions are simulated taking into account the density and the composition of the media surrounding the detector. The main features of gSeaGen are presented together with some examples of its application within the KM3NeT project.

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