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Gallacher, D. Goeldi, D. Keblbeck, D. Ray, D. S. Leonard, E. Angelico, E. Brown, E. Caden, E. Chambers, E. Hein, E. P. Bernard, E. van Bruggen, E. W. Hoppe, F. Spadoni, G. F. Cao, G. Gratta, G. Li, G. Richardson, G. S. Ortega, H. B. Yang, H. Lewis, H. Peltz Smalley, H. Rasiwala, H. Xu, I. Badhrees, I. J. Arnquist, J. Bane, J. Breslin, J. C. Nzobadila Ondze, J. Dalmasson, J. D. Holt, J. Farine, J.-F. Pratte, J. L. Orrell, J. Masbou, J. Nattress, J. P. Brodsky, J. Soderstrom, J. Zhao, K. G. Leach, K. McMichael, K. Ni, K. Raymond, K. S. Kumar, L. Darroch, L. Fabris, L. J. Wen, L. Pagani, L. Q. Cao, L. Yang, M. B. Latif, M. Chiu, M. Cvitan, M. Elbeltagi, M. Heffner, M. J. Dolinski, M. L. di Vacri, M. Medina-Peregrina, M. Vidal, M. Walent, M. Watts, M. Wehrfritz, M. Yu, M. Yvaine, nEXO Collaboration: S. Hedges, N. Fatemighomi, N. Gallice, O. A. Tyuka, O. Zeldovich, P. A. Breur, P. Arsenault, P. Kachru, P. Martel-Dion, Q. D. Wang, R. Collister, R. DeVoe, R. Elmansali, R. Gornea, R. H. M. Tsang, R. Lindsay, R. MacLellan, R. Ross, R. Saldanha, S. A. Charlebois, S. Al Kharusi, S. C. Nowicki, S. Majidi, S. Rescia, S. Sangiorgio, S. Schwartz, S. Sekula, S. Thibado, S. Triambak, S. Viel, S. Wilde, T. Bhatta, T. Brunner, T. Daniels, T. Pinto Franco, T. Totev, U. Wichoski, V. Belov, V. Riot, W. Fairbank, W. Gillis, W. Hunt, W. Wang, W. Wei, X. E. Ngwadla, X. L. Sun, X. M. Wu, Y. D. Guan, Y. G. Wang, Y. S. Fu, Y. Y. Ding, Z. Li","submitted_at":"2024-05-29T18:01:20Z","abstract_excerpt":"Electron-neutrino charged-current interactions with xenon nuclei were modeled in the nEXO neutrinoless double-$\\beta$ decay detector (~5 metric ton, 90% ${}^{136}$Xe, 10% ${}^{134}$Xe) to evaluate its sensitivity to supernova neutrinos. Predictions for event rates and detectable signatures were modeled using the Model of Argon Reaction Low Energy Yields (MARLEY) event generator. We find good agreement between MARLEY's predictions and existing theoretical calculations of the inclusive cross sections at supernova neutrino energies. 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Amy, A. Anker, A. Atencio, A. Bolotnikov, A. Gorham, A. House, A. Iverson, A. Karelin, A. K. Soma, A. Kuchenkov, A. Larson, A. Nolan, A. Pe\\~na-Perez, A. Perna, A. Piepke, A. Pocar, A. Tidball, B. Chana, B. Eckert, B. Foust, B. G. Lenardo, B. Mong, C. A. Hardy, C. Licciardi, C. Malbrunot, C. R. Natzke, C. T. Overman, D. Cesmecioglu, D. Chernyak, D. C. Moore, D. Gallacher, D. Goeldi, D. Keblbeck, D. Ray, D. S. Leonard, E. Angelico, E. Brown, E. Caden, E. Chambers, E. Hein, E. P. Bernard, E. van Bruggen, E. W. Hoppe, F. Spadoni, G. F. Cao, G. Gratta, G. Li, G. Richardson, G. S. Ortega, H. B. Yang, H. Lewis, H. Peltz Smalley, H. Rasiwala, H. Xu, I. Badhrees, I. J. Arnquist, J. Bane, J. Breslin, J. C. Nzobadila Ondze, J. Dalmasson, J. D. Holt, J. Farine, J.-F. Pratte, J. L. Orrell, J. Masbou, J. Nattress, J. P. Brodsky, J. Soderstrom, J. Zhao, K. G. Leach, K. McMichael, K. Ni, K. Raymond, K. S. Kumar, L. Darroch, L. Fabris, L. J. Wen, L. Pagani, L. Q. Cao, L. Yang, M. B. Latif, M. 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