Pre-supernova Alert System for Super-Kamiokande

Author:

Machado L. N.ORCID,Abe K.,Hayato Y.,Hiraide K.,Ieki K.,Ikeda M.,Kameda J.,Kanemura Y.,Kaneshima R.,Kashiwagi Y.,Kataoka Y.,Miki S.,Mine S.,Miura M.,Moriyama S.,Nakano Y.,Nakahata M.,Nakayama S.,Noguchi Y.,Okamoto K.,Sato K.,Sekiya H.,Shiba H.,Shimizu K.,Shiozawa M.,Sonoda Y.,Suzuki Y.,Takeda A.,Takemoto Y.,Takenaka A.,Tanaka H.,Watanabe S.,Yano T.,de Perio P.,Martens K.,Vagins M. R.,Bian J.,Griskevich N. J.,Kropp W. R.,Locke S.,Smy M. B.,Sobel H. W.,Takhistov V.,Yankelevich A.,Han S.,Kajita T.,Okumura K.,Tashiro T.,Tomiya T.,Wang X.,Xia J.,Yoshida S.,Megias G. D.,Fernandez P.,Labarga L.,Ospina N.,Zaldivar B.,Pointon B. W.,Akutsu R.,Gousy-Leblanc V.,Hartz M.,Konaka A.,Prouse N. W.,Kearns E.,Raaf J. L.,Wan L.,Wester T.,Hill J.,Kim J. Y.,Lim I. T.,Park R. G.,Bodur B.,Scholberg K.ORCID,Walter C. W.ORCID,Bernard L.,Coffani A.,Drapier O.,El Hedri S.,Giampaolo A.,Mueller Th. A.,Santos A. D.,Paganini P.,Quilain B.,Ishizuka T.,Nakamura T.,Jang J. S.,Learned J. G.,Cao S.,Choi K.,Anthony L. H. V.,Martin D.,Scott M.,Sztuc A. A.,Uchida Y.,Berardi V.,Catanesi M. G.,Radicioni E.,Calabria N. F.,De Rosa G.,Collazuol G.,Iacob F.,Lamoureux M.ORCID,Mattiazzi M.,Ludovici L.,Gonin M.,Pronost G.,Fujisawa C.,Maekawa Y.,Nishimura Y.,Sasaki R.,Friend M.,Hasegawa T.,Ishida T.,Jakkapu M.,Kobayashi T.,Matsubara T.,Nakadaira T.,Nakamura K.,Oyama Y.ORCID,Sakashita K.,Sekiguchi T.,Tsukamoto T.,Boschi T.,Di Lodovico F.,Gao J.,Goldsack A.,Katori T.,Migenda J.ORCID,Taani M.,Zsoldos S.,Kotsar Y.,Ozaki H.,Suzuki A. T.,Takeuchi Y.,Yaamoto S.,Bronner C.,Feng J.,Kikawa T.,Mori M.,Nakaya T.,Wendell R. A.,Yasutome K.,Jenkins S. J.,McCauley N.,Mehta P.,Tsui K. M.,Fukuda Y.,Itow Y.ORCID,Menjo H.,Ninomiya K.,Lagoda J.,Lakshmi S. M.,Mandal M.,Mijakowski P.,Prabhu Y. S.,Zalipska J.,Jia M.,Jiang J.,Jung C. K.,Wilking M. J.,Yanagisawa C.,Harada M.,Ishino H.,Ito S.,Kitagawa H.,Koshio Y.ORCID,Ma W.,Nakanishi F.,Sakai S.,Barr G.,Barrow D.,Cook L.,Samani S.,Wark D.,Nova F.,Yang J. Y.,Malek M.,McElwee J. M.,Stone O.,Thiesse M. D.,Thompson L. F.,Okazawa H.,Kim S. B.,Seo J. W.,Yu I.,Ichikawa A. K.,Nakamura K. D.,Tairafune S.,Nishijima K.,Iwamoto K.,Nakagiri K.,Nakajima Y.,Taniuchi N.,Yokoyama M.,Izumiyama S.,Kuze M.,Inomoto M.,Ishitsuka M.,Ito H.,Kinoshita T.,Matsumoto R.,Ommura Y.,Shigeta N.,Shinoki M.,Suganuma T.,Yonenaga M.,Martin J. F.,Tanaka H. A.,Towstego T.,Chen S.,Xu B. D.,Zhang B.,Posiadala-Zezula M.,Hadley D.,Nicholson M.,O’Flaherty M.,Richards B.,Ali A.,Jamieson B.,Marti Ll.,Minamino A.,Pintaudi G.,Sano S.,Suzuki S.,Wada K.

Abstract

Abstract In 2020, the Super-Kamiokande (SK) experiment moved to a new stage (SK-Gd) in which gadolinium (Gd) sulfate octahydrate was added to the water in the detector, enhancing the efficiency to detect thermal neutrons and consequently improving the sensitivity to low energy electron anti-neutrinos from inverse beta decay (IBD) interactions. SK-Gd has the potential to provide early alerts of incipient core-collapse supernovae through detection of electron anti-neutrinos from thermal and nuclear processes responsible for the cooling of massive stars before the gravitational collapse of their cores. These pre-supernova neutrinos emitted during the silicon burning phase can exceed the energy threshold for IBD reactions. We present the sensitivity of SK-Gd to pre-supernova stars and the techniques used for the development of a pre-supernova alarm based on the detection of these neutrinos in SK, as well as prospects for future SK-Gd phases with higher concentrations of Gd. For the current SK-Gd phase, high-confidence alerts for Betelgeuse could be issued up to 9 hr in advance of the core collapse itself.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 2 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Neutrinos and nucleosynthesis of elements;Progress in Particle and Nuclear Physics;2024-05

2. Supernova model discrimination with a kilotonne-scale Gd-H2O Cherenkov detector;Journal of Cosmology and Astroparticle Physics;2024-01-01

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