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ORCID: 0000-0003-1319-0889, Collazuol, G, Cook, L, Cowan, G, Cuen-Rochin, S, Danilov, M, Daz Lopez, G, 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, El Hedri, S, Ellis, J, Emery, S, Esmaili, A, Esteve, R, Evangelisti, A, Feely, M, Fedotov, S, Feng, J, Fernandez, P, Fernandez-Martinez, E, Ferrario, P, Ferrazzi, B, Feusels, T, Finch, A, Finley, C, Fiorentini, A, Fiorillo, G, Fitton, M, Frankiewicz, K, Friend, M, Fujii, Y, Fukuda, Y, Galinski, G, Gao, J, Garde, C, Garfagnini, A, Garode, S, Gialanella, L, Giganti, C, Gomez-Cadenas, JJ, Gonin, M, Gonzalez-Nuevo, J, Gorin, A, Gornea, R, Gousy-Leblanc, V, Gramegna, F, Grassi, M, Grella, G, Guigue, M, Gumplinger, P, Hadley, DR, Harada, M, Hartfiel, B, Hartz, M, Hassani, S, Hastings, NC, Hayato, Y, Hernando-Morata, JA, Herrero, V, Hill, J, Hiraide, K, Hirota, S, Holin, A, Horiuchi, S, Hoshina, K, Hultqvist, K, Iacob, F, Ichikawa, AK, Ibnsalih, W Idrissi, Iijima, T, Ikeda, M, Inomoto, M, Inoue, K, Insler, J, Ioannisian, A, Ishida, T, Ishidoshiro, K, Ishino, H, Ishitsuka, M, Ito, H, Ito, S, Itow, Y, Iwamoto, K, Izmaylov, A, Izumi, N, Izumiyama, S, Jakkapu, M, Jamieson, B, Jang, HI, Jang, JS, Jenkins, SJ ORCID: 0000-0002-0982-8141, Jeon, SH, Jiang, M, Jo, HS, Jonsson, P, Joo, KK, Kajita, T, Kakuno, H, Kameda, J, Kano, Y, Kalaczynski, P, Karlen, D, Kasperek, J, Kataoka, Y, Kato, A, Katori, T, Kazarian, N, Kearns, E, Khabibullin, M, Khotjantsev, A, Kikawa, T, Kikec, M, Kim, JH, Kim, JY, Kim, SB, Kim, SY, King, S, Kinoshita, T, Kisiel, J, Klekotko, A, Kobayashi, T, Koch, L, Koga, M, Koerich, L, Kolev, N, Konaka, A, Kormos, LL, Koshio, Y, Korzenev, A, Kotsar, Y, Kouzakov, KA, Kowalik, KL, Kravchuk, L, Kryukov, AP, Kudenko, Y, Kumita, T, Kurjata, R, Kutter, T, Kuze, M, Kwak, K, La Commara, M, Labarga, L, Lagoda, J, James, M Lamers, Lamoureux, M, 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S, Nakayoshi, K, Machado, L Nascimento, Naseby, CER, Navarro-Garcia, B, Needham, M, Nicholls, T, Niewczas, K, Nishimura, Y, Noah, E, Nova, F, Nugent, JC, Nunokawa, H, Obrebski, W, Ochoa-Ricoux, JP, O'Connor, E, Ogawa, N, Ogitsu, T, Ohta, K, Okamoto, K, O'Keeffe, HM, Okumura, K, Onishchuk, Y, Orozco-Luna, F, Oshlianskyi, A, Ospina, N, Ostrowski, M, O'Sullivan, E, O'Sullivan, L, Ovsiannikova, T, Oyama, Y, Ozaki, H, Pac, MY, Paganini, P, Palladino, V, Paolone, V, Pari, M, Parsa, S, Pasternak, J, Pastore, C, Pastuszak, G, Patel, DA, Pavin, M, Payne, D, Pena-Garay, C, Pidcott, C, Guerra, E Pinzon, Playfer, S, Pointon, BW, Popov, A, Popov, B, Porwit, K, Posiadala-Zezula, M, Poutissou, J-M, Pozimski, J, Pronost, G, Prouse, NW, Przewlocki, P, Quilain, B, Quiroga, AA, Radicioni, E, Radics, B, Rajda, PJ, Renner, J, Rescigno, M, Retiere, F, Ricciardi, G, Riccio, C, Richards, B, Rondio, E, Rose, HJ ORCID: 0000-0002-3388-8136, Roskovec, B, Roth, S, Rott, C, Rountree, SD, Rubbia, A, Ruggeri, AC, 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(2021)
Supernova Model Discrimination with Hyper-Kamiokande.
ASTROPHYSICAL JOURNAL, 916 (1).
15-.
Abstract
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.
| Item Type: |
Article
|
| Additional Information: |
21 pages, 7 figures. Article based on thesis published as
arXiv:2002.01649. v2: added references and some explanations in response to
reviewer comments |
| Uncontrolled Keywords: |
astro-ph.IM, astro-ph.IM, astro-ph.HE, hep-ex, physics.ins-det |
| Divisions: |
Faculty of Science and Engineering > School of Physical Sciences |
| Depositing User: |
Symplectic Admin
|
| Date Deposited: |
04 Oct 2021 16:10 |
| Last Modified: |
18 Jan 2023 21:27 |
| DOI: |
10.3847/1538-4357/abf7c4 |
| Related URLs: |
|
| URI: |
https://livrepository.liverpool.ac.uk/id/eprint/3139277 |
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