Accès ouvert déclaré
2024
article
Combined Pre-supernova Alert System with KamLAND and Super-Kamiokande
S. Abe, M. Eizuka, S. Futagi, A. Gando, Y. Gando, Shusaku Goto, Takahiko Hachiya, K. Hata, K. Ichimura, S. Ieki, H. Ikeda, K. Inoue, K. Ishidoshiro, Y. Kamei, N. Kawada, Y. Kishimoto, M. Koga, M. Kurasawa, T. Mitsui, H. Miyake, Daisuke Morita, T. Nakahata, R. Nakajima, K. Nakamura, R. Nakamura, J. Nakane, H. Ozaki, K. Saito, T. Sakai, I. Shimizu, J. Shirai, Kiyoshi Shiraishi, Ruri SHOJI, A. T. Suzuki, A. Takeuchi, K. Tamae, Hiroki Watanabe, K. Watanabe, S. Yoshida, S. Umehara, K. Fushimi, Kumiko Kotera, Y. Urano, B. E. Berger, B. K. Fujikawa, J. G. Learned, J. Maricic, Z. Fu, J. Smolsky, L. A. Winslow, Y. Efremenko, H. J. Karwowski, D. M. Markoff, W. Tornow, S. Dell’Oro, T. O’Donnell, J. A. Detwiler, Seishi Enomoto, M. P. Decowski, K. M. Weerman, C. Grant, H. C. Song, A. Li, Spencer Axani, M.C. Alonso‐García, K. Abe, C. Bronner, Y. Hayato, K. Hiraide, K. Hosokawa, K. Ieki, M. Ikeda, J. Kameda, Y. Kanemura, R. Kaneshima, Y. Kashiwagi, Y. Kataoka, S. Miki, S. Mine, M. Miura, S. Moriyama, M. Nakahata, Y. Nakano, S. Nakayama, Y. Noguchi, K. Satô, H. Sekiya, Hayato Shiba, K. Shimizu, M. Shiozawa, Y. Sonoda, Y. Suzuki, A. Takeda, Y. Takemoto, H. Tanaka, T. Yano, S. Han, T. Kajita, K. Okumura, T. Tashiro, Tomoaki Tomiya, X. Wang, P. Fernández, L. Labarga, N. Ospina, Bryan Zaldívar, B. W. Pointon, E. Kearns, J. L. Raaf, L. Wan, T. Wester, J. Bian, N. J. Griskevich, M. B. Smy, H. W. Sobel, Volodymyr Takhistov, A. Yankelevich, J. Hill, M. C. Jang, S. H. Lee, D. H. Moon, R. G. Park, B. Bodur, C. W. Walter, A. Beauchêne, O. Drapier, A. Giampaolo, Th. A. Mueller, A. D. Santos, P. Paganini, B. Quilain, R. Rogly, T. Nakamura, J. S. Jang, L. N. Machado, K. Choi, N. Iovine, S. Cao, L. H. V. Anthony, D. Martin, N. W. Prouse, M. Scott, Y. Uchida, V. Berardi, N. F. Calabria, M. G. Catanesi, E. Radicioni, A. Langella, G. De Rosa, G. Collazuol, M Feltre, F. Iacob, M. Mattiazzi, L. Ludovici, M. Gonin, Lorenzo Périssé, G. Pronost, C. Fujisawa, Shunsaku Horiuchi, Masakazu A. R. Kobayashi, Yongmin Liu, Y. Maekawa, Y. Nishimura, R. Okazaki, R. Akutsu, M. Friend, T. Hasegawa, Toru Ishida, T. Kobayashi, M. Jakkapu, T. Nakadaira, K. Nakamura, Y. Oyama, K. Sakashita, T. Tsukamoto, A. Portocarrero Yrey, G. T. Burton, F. Di Lodovico, A. Goldsack, T. Katori, J. Migenda, R. M. Ramsden, Z. Xie, Yusuke Takagi, Y. Takeuchi, H. Zhong, J. Feng, L. Feng, Jun Hu, Z. Hu, M. Kawaue, T. Kikawa, M. Mori, T. Nakaya, R. A. Wendell, S. J. Jenkins, N. McCauley, Poonam Mehta, A. Tarrant, Y. Itow, H. Menjo, K. Ninomiya, Yumiko Yoshioka, J. Łagoda, M. Mandal, Y.S Prabhu, J. Zalipska, M. Jia, J. Jiang, W. Shi, C. Yanagisawa, M. Harada, Y. Hino, H. Ishino, Y. Koshio, S. Sakai, Tomofumi Tada, T. Tano, T. Ishizuka, G. Barr, D. Barrow, L. Cook, S. Samani, D. Wark, A. Holin, F. Nova, S. Jung, B. S. Yang, J. Yang, J. Yoo, J. E. P. Fannon, L. Kneale, M. Malek, J. M. McElwee, M. D. Thiesse, L.F. Thompson, Stephen T. Wilson, H. Okazawa, S. M. Lakshmi, S. B. Kim, J. W. Seo, I. Yu, A. K. Ichikawa, K. D. Nakamura, S. Tairafune, K. Nishijima, A. Eguchi, K. Nakagiri, Y. Nakajima, S. Shima, N. Taniuchi, Eiji Watanabe, M. Yokoyama, P. de Perio, S. Fujita, C. Jesús-Valls, K. Martens, K. M. Tsui, M. R. Vagins, J. Xia, S. Izumiyama, M. Kuze, R. Matsumoto, K. Terada, Ryoichi Asaka, M. Ishitsuka, Hiroshi Itô, Y. Ommura, N. Shigeta, M. Shinoki, K. Yamauchi, T. Yoshida, R Gaur, V. Gousy-Leblanc, M. Hartz, A. Konaka, S. Chen, B. D. Xu, A. Q. Zhang, B. Zhang, M. Posiadała-Zezula, S. B. Boyd, Robert G. Edwards, D. Hadley, M. Nicholson, M. O’Flaherty, B. Richards, A. Ali, B. Jamieson, S. Amanai, Ll. Marti, A. Minamino, Rie Shibayama, S. Suzuki
14Citations signalées — pas une note de qualité
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Résumé fourni par la source
Abstract Preceding a core-collapse supernova (CCSN), various processes produce an increasing amount of neutrinos of all flavors characterized by mounting energies from the interior of massive stars. Among them, the electron antineutrinos are potentially detectable by terrestrial neutrino experiments such as KamLAND and Super-Kamiokande (SK) via inverse beta decay interactions. Once these pre-supernova (pre-SN) neutrinos are observed, an early warning of the upcoming CCSN can be provided. In light of this, KamLAND and SK, both located in the Kamioka mine in Japan, have been monitoring pre-SN neutrinos since 2015 and 2021, respectively. Recently, we performed a joint study between KamLAND and SK on pre-SN neutrino detection. A pre-SN alert system combining the KamLAND detector and the SK detector was developed and put into operation, which can provide a supernova alert to the astrophysics community. Fully leveraging the complementary properties of these two detectors, the combined alert is expected to resolve a pre-SN neutrino signal from a 15 M ⊙ star within 510 pc of the Earth at a significance level corresponding to a false alarm rate of no more than 1 per century. For a Betelgeuse-like model with optimistic parameters, it can provide early warnings up to 12 hr in advance.
Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.
Contrôle bibliographique ouvert
DOI retrouvé dans Crossref DOI retrouvé ; titre concordant.
- Titre Crossref
- Combined Pre-supernova Alert System with KamLAND and Super-Kamiokande
- Date Crossref
- 26/09/2024
- Éditeur
- American Astronomical Society
- Type
- journal-article
Ce recoupement confirme des métadonnées liées au DOI. Il ne confirme ni la méthode ni les conclusions de l’étude et ne compte pas comme une seconde source scientifique indépendante.
Institutions déclarées
Une affiliation ne permet pas de déduire la nationalité d’un auteur.
Sujets associés
Neutrino Physics ResearchAstrophysics and Cosmic PhenomenaParticle physics theoretical and experimental studies