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DC Field | Value | Language |
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dc.citation.number | 1 | - |
dc.citation.startPage | 15 | - |
dc.citation.title | ASTROPHYSICAL JOURNAL | - |
dc.citation.volume | 916 | - |
dc.contributor.author | Abe, K. | - |
dc.contributor.author | Adrich, P. | - |
dc.contributor.author | Aihara, H. | - |
dc.contributor.author | Akutsu, R. | - |
dc.contributor.author | Alekseev, I. | - |
dc.contributor.author | Ali, A. | - |
dc.contributor.author | Ameli, F. | - |
dc.contributor.author | Anghel, I. | - |
dc.contributor.author | Anthony, L. H. V. | - |
dc.contributor.author | Antonova, M. | - |
dc.contributor.author | Araya, A. | - |
dc.contributor.author | Asaoka, Y. | - |
dc.contributor.author | Ashida, Y. | - |
dc.contributor.author | Aushev, V. | - |
dc.contributor.author | Ballester, F. | - |
dc.contributor.author | Bandac, I. | - |
dc.contributor.author | Barbi, M. | - |
dc.contributor.author | Barker, G. J. | - |
dc.contributor.author | Barr, G. | - |
dc.contributor.author | Batkiewicz-Kwasniak, M. | - |
dc.contributor.author | Bellato, M. | - |
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dc.contributor.author | Tanaka, M. | - |
dc.contributor.author | Tashiro, T. | - |
dc.contributor.author | Thiesse, M. | - |
dc.contributor.author | Thompson, L. F. | - |
dc.contributor.author | Toledo, J. | - |
dc.contributor.author | Tomatani-Sánchez, A. K. | - |
dc.contributor.author | Tortone, G. | - |
dc.contributor.author | Tsui, K. M. | - |
dc.contributor.author | Tsukamoto, T. | - |
dc.contributor.author | Tzanov, M. | - |
dc.contributor.author | Uchida, Y. | - |
dc.contributor.author | Vagins, M. R. | - |
dc.contributor.author | Valder, S. | - |
dc.contributor.author | Valentino, V. | - |
dc.contributor.author | Vasseur, G. | - |
dc.contributor.author | Vijayvargi, A. | - |
dc.contributor.author | Vilela, C. | - |
dc.contributor.author | Vinning, W. G. S. | - |
dc.contributor.author | Vivolo, D. | - |
dc.contributor.author | Vladisavljevic, T. | - |
dc.contributor.author | Vogelaar, R. B. | - |
dc.contributor.author | Vyalkov, M. M. | - |
dc.contributor.author | Wachala, T. | - |
dc.contributor.author | Walker, J. | - |
dc.contributor.author | Wark, D. | - |
dc.contributor.author | Wascko, M. O. | - |
dc.contributor.author | Wendell, R. A. | - |
dc.contributor.author | Wilkes, R. J. | - |
dc.contributor.author | Wilking, M. J. | - |
dc.contributor.author | Wilson, J. R. | - |
dc.contributor.author | Wronka, S. | - |
dc.contributor.author | Xia, J. | - |
dc.contributor.author | Xie, Z. | - |
dc.contributor.author | Xin, T. | - |
dc.contributor.author | Yamaguchi, Y. | - |
dc.contributor.author | Yamamoto, K. | - |
dc.contributor.author | Yanagisawa, C. | - |
dc.contributor.author | Yano, T. | - |
dc.contributor.author | Yen, S. | - |
dc.contributor.author | Yershov, N. | - |
dc.contributor.author | Yeum, D. N. | - |
dc.contributor.author | Yokoyama, M. | - |
dc.contributor.author | Yonenaga, M. | - |
dc.contributor.author | Yoo, J. | - |
dc.contributor.author | Yu, I. | - |
dc.contributor.author | Yu, M. | - |
dc.contributor.author | Zakrzewski, T. | - |
dc.contributor.author | Zaldivar, B. | - |
dc.contributor.author | Zalipska, J. | - |
dc.contributor.author | Zaremba, K. | - |
dc.contributor.author | Zarnecki, G. | - |
dc.contributor.author | Ziembicki, M. | - |
dc.contributor.author | Zietara, K. | - |
dc.contributor.author | Zito, M. | - |
dc.contributor.author | Zsoldos, S. | - |
dc.date.accessioned | 2023-12-21T15:39:03Z | - |
dc.date.available | 2023-12-21T15:39:03Z | - |
dc.date.created | 2021-07-26 | - |
dc.date.issued | 2021-07 | - |
dc.description.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. | - |
dc.identifier.bibliographicCitation | ASTROPHYSICAL JOURNAL, v.916, no.1, pp.15 | - |
dc.identifier.doi | 10.3847/1538-4357/abf7c4 | - |
dc.identifier.issn | 0004-637X | - |
dc.identifier.uri | https://scholarworks.unist.ac.kr/handle/201301/53307 | - |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/1538-4357/abf7c4 | - |
dc.identifier.wosid | 000674707600001 | - |
dc.language | 영어 | - |
dc.publisher | IOP PUBLISHING LTD | - |
dc.title | Supernova Model Discrimination with Hyper-Kamiokande | - |
dc.type | Article | - |
dc.description.isOpenAccess | FALSE | - |
dc.relation.journalWebOfScienceCategory | Astronomy & Astrophysics | - |
dc.relation.journalResearchArea | Astronomy & Astrophysics | - |
dc.type.docType | Article | - |
dc.description.journalRegisteredClass | scie | - |
dc.description.journalRegisteredClass | scopus | - |
dc.subject.keywordPlus | CORE-COLLAPSE SUPERNOVAEEQUATION-OF-STATENEUTRINO BURSTRADIATION HYDRODYNAMICSMAGELLANIC-CLOUDOSCILLATIONSEVOLUTIONSIMULATIONSEXPLOSIONMATTER | - |
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