Supernova Model Discrimination with Hyper-Kamiokande
Creators: name: Kamiokande Collaboration
name: Abe, K.
name: Adrich, P.
name: Aihara, H.
name: Akutsu, R.
name: Alekseev, I.
name: Ali, A.
name: Ameli, F.
name: Anghel, I.
name: Anthony, L. H. V.
name: Antonova, M.
name: Araya, A.
name: Asaoka, Y.
name: Ashida, Y.
name: Aushev, V.
name: Ballester, F.
name: Bandac, I.
name: Barbi, M.
name: Barker, G. J.
name: Barr, G.
name: Batkiewicz-Kwasniak, M.
name: Bellato, M.
name: Berardi, V.
name: Bergevin, M.
name: Bernard, L.
name: Bernardini, E.
name: Berns, L.
name: Bhadra, S.
name: Bian, J.
name: Blanchet, A.
name: Blaszczyk, F. d. M.
name: Blondel, A.
name: Boiano, A.
name: Bolognesi, S.
name: Bonavera, L.
name: Booth, N.
name: Borjabad, S.
name: Boschi, T.
name: Bose, D.
name: Boyd, S . B.
name: Bozza, C.
name: Bravar, A.
name: Bravo-Berguño, D.
name: Bronner, C.
name: Brown, L.
name: Bubak, A.
name: Buchowicz, A.
name: Avanzini, M. Buizza
name: Cafagna, F. S.
name: Calabria, N. F.
name: Calvo-Mozota, J. M.
name: Cao, S.
name: Cartwright, S. L.
name: Carroll, A.
name: Catanesi, M. G.
name: Cebriàn, S.
name: Chabera, M.
name: Chakraborty, S.
name: Checchia, C.
name: Choi, J. H.
name: Choubey, S.
name: Cicerchia, M.
name: Coleman, J.
name: Collazuol, G.
name: Cook, L.
name: Cowan, G.
name: Cuen-Rochin, S.
name: Danilov, M.
name: Lopez, G. Daz
name: De la Fuente, E.
name: de Perio, P.
name: De Rosa, G.
name: Dealtry, T.
name: Densham, C. J.
name: Dergacheva, A.
name: Deshmukh, N.
name: Devi, M. M.
name: Di Lodovico, F.
name: Di Meo, P.
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name: Doyle, T. A.
name: Drakopoulou, E.
name: Drapier, O.
name: Dumarchez, J.
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name: Dziewiecki, M.
name: Eklund, L.
name: Hedri, S. El
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name: Emery, S.
name: Esmaili, A.
name: Esteve, R.
name: Evangelisti, A.
name: Feely, M.
name: Fedotov, S.
name: Feng, J.
name: Fernandez, P.
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name: Ferrario, P.
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name: Feusels, T.
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name: Fiorentini, A.
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name: Gramegna, F.
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name: Gumplinger, P.
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Publisher: name: arXiv
Year: 2021
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: High Energy Physics - Experiment (hep-ex)
subject: Instrumentation and Detectors (physics.ins-det)
subject: FOS: Physical sciences
subject: FOS: Physical sciences

description: Core-collapse supernovae are among the most magnificent events in the observable universe. They produce many of the chemical elements necessary for life to exist and their remnants -- neutron stars and black holes -- are interesting astrophysical objects in their own right. However, despite millennia of observations and almost a century of astrophysical study, the explosion mechanism of core-collapse supernovae is not yet well understood. Hyper-Kamiokande is a next-generation neutrino detector that will be able to observe the neutrino flux from the next galactic core-collapse supernova in unprecedented detail. We focus on the first 500 ms of the neutrino burst, corresponding to the accretion phase, and use a newly-developed, high-precision supernova event generator to simulate Hyper-Kamiokande's response to five different supernova models. We show that Hyper-Kamiokande will be able to distinguish between these models with high accuracy for a supernova at a distance of up to 100 kpc. Once the next galactic supernova happens, this ability will be a powerful tool for guiding simulations towards a precise reproduction of the explosion mechanism observed in nature.
description: 21 pages, 7 figures. Article based on thesis published as arXiv:2002.01649. v2: added references and some explanations in response to reviewer comments