1. Supernova Model Discrimination with Hyper-Kamiokande
- Author
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Collaboration, Hyper-Kamiokande, :, Abe, K, Adrich, P, Aihara, H, Akutsu, R, Alekseev, I, Ali, A, Ameli, F, Anghel, I, Anthony, LHV, Antonova, M, Araya, A, Asaoka, Y, Ashida, Y, Aushev, V, Ballester, F, Bandac, I, Barbi, M, Barker, GJ, Barr, G, Batkiewicz-Kwasniak, M, Bellato, M, Berardi, V, Bergevin, M, Bernard, L, Bernardini, E, Berns, L, Bhadra, S, Bian, J, Blanchet, A, Blaszczyk, FDM, Blondel, A, Boiano, A, Bolognesi, S, Bonavera, L, Booth, N, Borjabad, S, Boschi, T, Bose, D, Boyd, SB, Bozza, C, Bravar, A, Bravo-Berguño, D, Bronner, C, Brown, L, Bubak, A, Buchowicz, A, Avanzini, M Buizza, Cafagna, FS, Calabria, NF, Calvo-Mozota, JM, Cao, S, Cartwright, SL, Carroll, A, Catanesi, MG, Cebriàn, S, Chabera, M, Chakraborty, S, Checchia, C, Choi, JH, Choubey, S, Cicerchia, M, Coleman, J, Collazuol, G, Cook, L, Cowan, G, Cuen-Rochin, S, Danilov, M, Lopez, G Daz, De la Fuente, E, de Perio, P, De Rosa, G, Dealtry, T, Densham, CJ, Dergacheva, A, Deshmukh, N, Devi, MM, Di Lodovico, F, Di Meo, P, Di Palma, I, Doyle, TA, Drakopoulou, E, Drapier, O, Dumarchez, J, Dunne, P, Dziewiecki, M, Eklund, L, Hedri, S El, Ellis, J, Emery, S, Esmaili, A, Esteve, R, Evangelisti, A, Feely, M, Fedotov, S, Feng, J, Fernandez, P, Fernández-Martinez, E, and Ferrario, P
- Subjects
astro-ph.IM ,astro-ph.HE ,hep-ex ,physics.ins-det - Abstract
Core-collapse supernovae are among the most magnificent events in theobservable universe. They produce many of the chemical elements necessary forlife to exist and their remnants -- neutron stars and black holes -- areinteresting astrophysical objects in their own right. However, despitemillennia of observations and almost a century of astrophysical study, theexplosion mechanism of core-collapse supernovae is not yet well understood.Hyper-Kamiokande is a next-generation neutrino detector that will be able toobserve the neutrino flux from the next galactic core-collapse supernova inunprecedented detail. We focus on the first 500 ms of the neutrino burst,corresponding to the accretion phase, and use a newly-developed, high-precisionsupernova event generator to simulate Hyper-Kamiokande's response to fivedifferent supernova models. We show that Hyper-Kamiokande will be able todistinguish between these models with high accuracy for a supernova at adistance of up to 100 kpc. Once the next galactic supernova happens, thisability will be a powerful tool for guiding simulations towards a precisereproduction of the explosion mechanism observed in nature.
- Published
- 2021