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arxiv: 2404.09920 · v3 · pith:YJR23IUE · submitted 2024-04-15 · hep-ex · astro-ph.HE· physics.ins-det

Combined Pre-Supernova Alert System with Kamland and Super-Kamiokande

KamLAND , Super-Kamiokande Collaborations: Seisho Abe , Minori Eizuka , Sawako Futagi , Azusa Gando , Yoshihito Gando , Shun Goto , Takahiko Hachiya
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Kazumi Hata Koichi Ichimura Sei Ieki Haruo Ikeda Kunio Inoue Koji Ishidoshiro Yuto Kamei Nanami Kawada Yasuhiro Kishimoto Masayuki Koga Maho Kurasawa Tadao Mitsui Haruhiko Miyake Daisuke Morita Takeshi Nakahata Rika Nakajima Kengo Nakamura Rikuo Nakamura Ryo Nakamura Jun Nakane Hideyoshi Ozaki Keita Saito Taichi Sakai Itaru Shimizu Junpei Shirai Kensuke Shiraishi Ryunosuke Shoji Atsuto Suzuki Atsuto Takeuchi Kyoko Tamae Hiroko Watanabe Kazuho Watanabe Sei Yoshida Saori Umehara Ken-Ichi Fushimi Kenta Kotera Yusuke Urano Bruce E. Berger Brian K. Fujikawa John G. Larned Jelena Maricic Zhenghao Fu Joseph Smolsky Lindley A. Winslow Yuri Efremenko Hugon J. Karwowski Diane M. Markoff Werner Tornow Stefano Dell'Oro Thomas O'Donnell Jason A. Detwiler Sanshiro Enomoto Michal P. Decowski Kelly M. Weerman Christopher Grant Hasung Song Aobo Li Spencer N. Axani Miles Garcia Ko Abe Seisho Abe Christophe Bronner Yoshinari Hayato Katsuki Hiraide Keishi Hosokawa Kei Ieki Motoyasu Ikeda June Kameda Yuki Kanemura Ryota Kaneshima Yuri Kashiwagi Yousuke Kataoka Shintaro Miki Shunichi Mine Makoto Miura Shigetaka Moriyama Masayuki Nakahata Yuuki Nakano Shoei Nakayama Yohei Noguchi Kazufumi Sato Hiroyuki Sekiya Hayato Shiba Kotaro Shimizu Masato Shiozawa Yutaro Sonoda Yoichiro Suzuki Atsushi Takeda Yasuhiro Takemoto Hidekazu K. Tanaka Takatomi Yano Seungho Han Takaaki Kajita Kimihiro Okumura Takuya Tashiro Takuya Tomiya Xubin Wang Shunsuke Yoshida Pablo Fernandez Luis Labarga Nataly Ospina Bryan Zaldivar Barry W. Pointon Edward Kearns Jennifer L. Raaf Linyan Wan Thomas Wester Jianming Bian Jeff Griskevich Michael B. Smy Henry W. Sobel Volodymyr Takhistov Alejandro Yankelevich James Hill MinCheol Jang Seonghak Lee DongHo Moon RyeongGyoon Park Baran Bodur Kate Scholberg Chris W. Walter Antoine Beauch\^ene Olivier Drapier Alberto Giampaolo Thomas A. Mueller Andrew D. Santos Pascal Paganini Benjamin Quilain Rudolph Rogly Taku Nakamura Jee-Seung Jang Lucas N. Machado John G. Learned Koun Choi Nadege Iovine Son V. Cao Lauren H. V. Anthony Daniel G.R. Martin Nick W. Prouse Mark Scott Yoshi Uchida Vincenzo Berardi Nicola F. Calabria M. G. Catanesi Emilio Radicioni Aurora Langella Gianfranca de Rosa Gianmaria Collazuol Matteo Feltre Fabio Iacob Marco Mattiazzi Lucio Ludovici Michel Gonin Lorenzo P\'eriss\'e Guillaume Pronost Chiori Fujisawa Shogo Horiuchi Misaki Kobayashi Yu-Ming Liu Yuto Maekawa Yasuhiro Nishimura Reo Okazaki Ryosuke Akutsu Megan Friend Takuya Hasegawa Taku Ishida Takashi Kobayashi Mahesh Jakkapu Tsunayuki Matsubara Takeshi Nakadaira Kenzo Nakamura Yuichi Oyama Ken Sakashita Tetsuro Sekiguchi Toshifumi Tsukamoto Antoniosk Portocarrero Yrey Nahid Bhuiyan George T. Burton Francesca Di Lodovico Joanna Gao Alexander Goldsack Teppei Katori Jost Migenda Rory M. Ramsden Zhenxiong Xie Stephane Zsoldos Atsumu T. Suzuki Yusuke Takagi Yasuo Takeuchi Haiwen Zhong Jiahui Feng Li-Cheng Feng Jianrun Hu Zhuojun Hu Masaki Kawaue Tatsuya Kikawa Masamitsu Mori Tsuyoshi Nakaya Roger A. Wendell Kenji Yasutome Sam J. Jenkins Neil K. McCauley Pruthvi Mehta Adam Tarrant Mike J. Wilking Yoshiyuki Fukuda Yoshitaka Itow Hiroaki Menjo Kotaro Ninomiya Yushi Yoshioka Justyna Lagoda Maitrayee Mandal Piotr Mijakowski Yashwanth S. Prabhu Joanna Zalipska Mo Jia Junjie Jiang Wei Shi Chiaki Yanagisawa Masayuki Harada Yota Hino Hirokazu Ishino Yusuke Koshio Fumi Nakanishi Seiya Sakai Tomoaki Tada Tomohiro Tano Takeharu Ishizuka Giles Barr Daniel Barrow Laurence Cook Soniya Samani David Wark Anna Holin Federico Nova Seunghyun Jung Byeongsu Yang JeongYeol Yang Jonghee Yoo Jack E.P. Fannon Liz Kneale Matthew Malek Jordan M. McElwee Matthew D. Thiesse Lee F. Thompson Stephen T. Wilson Hiroko Okazawa Lakshmi S. Mohan SooBong Kim Eunhyang Kwon Ji-Woong Seo Intae Yu Atsuko K. Ichikawa Kiseki D. Nakamura Seidai Tairafune Kyoshi Nishijima Aoi Eguchi Kota Nakagiri Yasuhiro Nakajima Shizuka Shima Natsumi Taniuchi Eiichiro Watanabe Masashi Yokoyama Patrick de Perio Saki Fujita Cesar Jesus-Valls Kai Martens Ka M. Tsui Mark R. Vagins Junjie Xia Shota Izumiyama Masahiro Kuze Ryo Matsumoto Kotaro Terada Ryusei Asaka Masaki Ishitsuka Hiroshi Ito Yuga Ommura Natsuki Shigeta Masataka Shinoki Koki Yamauchi Tsukasa Yoshida Rhea Gaur Vincent Gousy-Leblan Mark Hartz Akira Konaka Xiaoyue Li Shaomin Chen Benda Xu Aiqiang Zhang Bin Zhang Magdalena Posiadala-Zezula Steven B. Boyd Rory Edwards David Hadley Matthew Nicholson Marcus O'Flaherty Benjamin Richards Ajmi Ali Blair Jamieson Shogo Amanai Lluis Marti-Magro Akihiro Minamino Ryo Shibayama Serina Suzuki
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classification hep-ex astro-ph.HEphysics.ins-det
keywords pre-supernovakamlandsuper-kamiokandealertneutrinoneutrinossupernovacombined
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Preceding a core-collapse supernova, 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 via inverse beta decay interactions. Once these pre-supernova neutrinos are observed, an early warning of the upcoming core-collapse supernova can be provided. In light of this, KamLAND and Super-Kamiokande, both located in the Kamioka mine in Japan, have been monitoring pre-supernova neutrinos since 2015 and 2021, respectively. Recently, we performed a joint study between KamLAND and Super-Kamiokande on pre-supernova neutrino detection. A pre-supernova alert system combining the KamLAND detector and the Super-Kamiokande 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-supernova neutrino signal from a 15 M$_{\odot}$ 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 hours in advance.

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