File Download

There are no files associated with this item.

  • Find it @ UNIST can give you direct access to the published full text of this article. (UNISTARs only)
Related Researcher

곽규진

Kwak, Kyujin
Computational Astrophysics Lab.
Read More

Views & Downloads

Detailed Information

Cited time in webofscience Cited time in scopus
Metadata Downloads

Supernova Model Discrimination with Hyper-Kamiokande

Author(s)
Abe, K.Adrich, P.Aihara, H.Akutsu, R.Alekseev, I.Ali, A.Ameli, F.Anghel, I.Anthony, L. H. V.Antonova, M.Araya, A.Asaoka, Y.Ashida, Y.Aushev, V.Ballester, F.Bandac, I.Barbi, M.Barker, G. J.Barr, G.Batkiewicz-Kwasniak, M.Bellato, M.Berardi, V.Bergevin, M.Bernard, L.Bernardini, E.Berns, L.Bhadra, S.Bian, J.Blanchet, A.Blaszczyk, F. d. M.Blondel, A.Boiano, A.Bolognesi, S.Bonavera, L.Booth, N.Borjabad, S.Boschi, T.Bose, D.Boyd, S . B.Bozza, C.Bravar, A.Bravo-Berguño, D.Bronner, C.Brown, L.Bubak, A.Buchowicz, A.Buizza Avanzini, M.Cafagna, F. S.Calabria, N. F.Calvo-Mozota, J. M.Cao, S.Cartwright, S. L.Carroll, A.Catanesi, M. G.Cebriàn, S.Chabera, M.Chakraborty, S.Checchia, C.Choi, J. H.Choubey, S.Cicerchia, M.Coleman, J.Collazuol, G.Cook, L.Cowan, G.Cuen-Rochin, S.Danilov, M.Díaz López, G.De la Fuente, E.de Perio, P.De Rosa, G.Dealtry, T.Densham, C. J.Dergacheva, A.Deshmukh, N.Devi, M. M.Di Lodovico, F.Di Meo, P.Di Palma, I.Doyle, T. A.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.Fernández-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, J. J.Gonin, M.González-Nuevo, J.Gorin, A.Gornea, R.Gousy-Leblanc, V.Gramegna, F.Grassi, M.Grella, G.Guigue, M.Gumplinger, P.Hadley, D. R.Harada, M.Hartfiel, B.Hartz, M.Hassani, S.Hastings, N. C.Hayato, Y.Hernando-Morata, J. A.Herrero, V.Hill, J.Hiraide, K.Hirota, S.Holin, A.Horiuchi, S.Hoshina, K.Hultqvist, K.Iacob, F.Ichikawa, A. K.Idrissi Ibnsalih, W.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, H. I.Jang, J. S.Jenkins, S. J.Jeon, S. H.Jiang, M.Jo, H. S.Jonsson, P.Joo, K. K.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.Kekic, M.Kim, J. H.Kim, J. Y.Kim, S. B.Kim, S. Y.King, S.Kinoshita, T.Kisiel, J.Klekotko, A.Kobayashi, T.Koch, L.Koga, M.Koerich, L.Kolev, N.Konaka, A.Kormos, L. L.Koshio, Y.Korzenev, A.Kotsar, Y.Kouzakov, K. A.Kowalik, K. L.Kravchuk, L.Kryukov, A. P.Kudenko, Y.Kumita, T.Kurjata, R.Kutter, T.Kuze, M.Kwak, KyujinLa Commara, M.Labarga, L.Lagoda, J.Lamers James, M.Lamoureux, M.Laveder, M.Lavitola, L.Lawe, M.Learned, J. G.Lee, J.Leitner, R.Lezaun, V.Lim, I. T.Lindner, T.Litchfield, R. P.Long, K. R.Longhin, A.Loverre, P.Lu, X.Ludovici, L.Maekawa, Y.Magaletti, L.Magar, K.Mahn, K.Makida, Y.Malek, M.Malinský, M.Marchi, T.Maret, L.Mariani, C.Marinelli, A.Martens, K.Marti, Ll.Martin, J. F.Martin, D.Marzec, J.Matsubara, T.Matsumoto, R.Matsuno, S.Matusiak, M.Mazzucato, E.McCarthy, M.McCauley, N.McElwee, J.McGrew, C.Mefodiev, A.Medhi, A.Mehta, P.Mellet, L.Menjo, H.Mermod, P.Metelko, C.Mezzetto, M.Migenda, J.Migliozzi, P.Mijakowski, P.Miki, S.Miller, E. W.Minakata, H.Minamino, A.Mine, S.Mineev, O.Mitra, A.Miura, M.Moharana, R.Mollo, C. M.Mondal, T.Mongelli, M.Monrabal, F.Moon, D. H.Moon, C. S.Mora, F. J.Moriyama, S.Mueller, Th. A.Munteanu, L.Murase, K.Nagao, Y.Nakadaira, T.Nakagiri, K.Nakahata, M.Nakai, S.Nakajima, Y.Nakamura, K.Nakamura, KI.Nakamura, H.Nakano, Y.Nakaya, T.Nakayama, S.Nakayoshi, K.Nascimento Machado, L.Naseby, C. E. R.Navarro-Garcia, B.Needham, M.Nicholls, T.Niewczas, K.Nishimura, Y.Noah, E.Nova, F.Nugent, J. C.Nunokawa, H.Obrebski, W.Ochoa-Ricoux, J. P.O’Connor, E.Ogawa, N.Ogitsu, T.Ohta, K.Okamoto, K.O’Keeffe, H. M.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, M. Y.Paganini, P.Palladino, V.Paolone, V.Pari, M.Parsa, S.Pasternak, J.Pastore, C.Pastuszak, G.Patel, D. A.Pavin, M.Payne, D.Peña-Garay, C.Pidcott, C.Pinzon Guerra, E.Playfer, S.Pointon, B. W.Popov, A.Popov, B.Porwit, K.Posiadala-Zezula, M.Poutissou, J.-M.Pozimski, J.Pronost, G.Prouse, N. W.Przewlocki, P.Quilain, B.Quiroga, A. A.Radicioni, E.Radics, B.Rajda, P. J.Renner, J.Rescigno, M.Retiere, F.Ricciardi, G.Riccio, C.Richards, B.Rondio, E.Rose, H. J.Roskovec, B.Roth, S.Rott, C.Rountree, S. D.Rubbia, A.Ruggeri, A. C.Ruggles, C.Russo, S.Rychter, A.Ryu, DongsuSakashita, K.Samani, S.Sánchez, F.Sánchez, M. L.Sanchez, M. C.Sano, S.Santos, J. D.Santucci, G.Sarmah, P.Sashima, I.Sato, K.Scott, M.Seiya, Y.Sekiguchi, T.Sekiya, H.Seo, J. W.Seo, S. H.Sgalaberna, D.Shaikhiev, A.Shan, Z.Shaykina, A.Shimizu, I.Shin, C. D.Shinoki, M.Shiozawa, M.Sinnis, G.Skrobova, N.Skwarczynski, K.Smy, M. B.Sobczyk, J.Sobel, H. W.Soler, F. J. P.Sonoda, Y.Spina, R.Spisso, B.Spradlin, P.Stankevich, K. L.Stawarz, L.Stellacci, S. M.Stopa, K.Studenikin, A. I.Suárez Gómez, S. L.Suganuma, T.Suvorov, S.Suwa, Y.Suzuki, A. T.Suzuki, S. Y.Suzuki, Y.Svirida, D.Svoboda, R.Taani, M.Tada, M.Takeda, A.Takemoto, Y.Takenaka, A.Taketa, A.Takeuchi, Y.Takhistov, V.Tanaka, H.Tanaka, H. A.Tanaka, H. I.Tanaka, M.Tashiro, T.Thiesse, M.Thompson, L. F.Toledo, J.Tomatani-Sánchez, A. K.Tortone, G.Tsui, K. M.Tsukamoto, T.Tzanov, M.Uchida, Y.Vagins, M. R.Valder, S.Valentino, V.Vasseur, G.Vijayvargi, A.Vilela, C.Vinning, W. G. S.Vivolo, D.Vladisavljevic, T.Vogelaar, R. B.Vyalkov, M. M.Wachala, T.Walker, J.Wark, D.Wascko, M. O.Wendell, R. A.Wilkes, R. J.Wilking, M. J.Wilson, J. R.Wronka, S.Xia, J.Xie, Z.Xin, T.Yamaguchi, Y.Yamamoto, K.Yanagisawa, C.Yano, T.Yen, S.Yershov, N.Yeum, D. N.Yokoyama, M.Yonenaga, M.Yoo, J.Yu, I.Yu, M.Zakrzewski, T.Zaldivar, B.Zalipska, J.Zaremba, K.Zarnecki, G.Ziembicki, M.Zietara, K.Zito, M.Zsoldos, S.
Issued Date
2021-07
DOI
10.3847/1538-4357/abf7c4
URI
https://scholarworks.unist.ac.kr/handle/201301/53307
Fulltext
https://iopscience.iop.org/article/10.3847/1538-4357/abf7c4
Citation
ASTROPHYSICAL JOURNAL, v.916, no.1, pp.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 toward a precise reproduction of the explosion mechanism observed in nature.
Publisher
IOP PUBLISHING LTD
ISSN
0004-637X
Keyword
CORE-COLLAPSE SUPERNOVAEEQUATION-OF-STATENEUTRINO BURSTRADIATION HYDRODYNAMICSMAGELLANIC-CLOUDOSCILLATIONSEVOLUTIONSIMULATIONSEXPLOSIONMATTER

qrcode

Items in Repository are protected by copyright, with all rights reserved, unless otherwise indicated.