학술논문

Combined Pre-Supernova Alert System with Kamland and Super-Kamiokande
Document Type
Working Paper
Author
KamLANDCollaborations, Super-KamiokandeAbe, SeishoEizuka, MinoriFutagi, SawakoGando, AzusaGando, YoshihitoGoto, ShunHachiya, TakahikoHata, KazumiIchimura, KoichiIeki, SeiIkeda, HaruoInoue, KunioIshidoshiro, KojiKamei, YutoKawada, NanamiKishimoto, YasuhiroKoga, MasayukiKurasawa, MahoMitsui, TadaoMiyake, HaruhikoMorita, DaisukeNakahata, TakeshiNakajima, RikaNakamura, KengoNakamura, RikuoNakamura, RyoNakane, JunOzaki, HideyoshiSaito, KeitaSakai, TaichiShimizu, ItaruShirai, JunpeiShiraishi, KensukeShoji, RyunosukeSuzuki, AtsutoTakeuchi, AtsutoTamae, KyokoWatanabe, HirokoWatanabe, KazuhoYoshida, SeiUmehara, SaoriFushimi, Ken-IchiKotera, KentaUrano, YusukeBerger, Bruce E.Fujikawa, Brian K.Larned, John G.Maricic, JelenaFu, ZhenghaoSmolsky, JosephWinslow, Lindley A.Efremenko, YuriKarwowski, Hugon J.Markoff, Diane M.Tornow, WernerDell'Oro, StefanoO'Donnell, ThomasDetwiler, Jason A.Enomoto, SanshiroDecowski, Michal P.Weerman, Kelly M.Grant, ChristopherSong, HasungLi, AoboAxani, Spencer N.Garcia, MilesAbe, KoBronner, ChristopheHayato, YoshinariHiraide, KatsukiHosokawa, KeishiIeki, KeiIkeda, MotoyasuKameda, JuneKanemura, YukiKaneshima, RyotaKashiwagi, YuriKataoka, YousukeMiki, ShintaroMine, ShunichiMiura, MakotoMoriyama, ShigetakaNakahata, MasayukiNakano, YuukiNakayama, ShoeiNoguchi, YoheiSato, KazufumiSekiya, HiroyukiShiba, HayatoShimizu, KotaroShiozawa, MasatoSonoda, YutaroSuzuki, YoichiroTakeda, AtsushiTakemoto, YasuhiroTanaka, Hidekazu K.Yano, TakatomiHan, SeunghoKajita, TakaakiOkumura, KimihiroTashiro, TakuyaTomiya, TakuyaWang, XubinYoshida, ShunsukeFernandez, PabloLabarga, LuisOspina, NatalyZaldivar, BryanPointon, Barry W.Kearns, EdwardRaaf, Jennifer L.Wan, LinyanWester, ThomasBian, JianmingGriskevich, JeffSmy, Michael B.Sobel, Henry W.Takhistov, VolodymyrYankelevich, AlejandroHill, JamesJang, MinCheolLee, SeonghakMoon, DongHoPark, RyeongGyoonBodur, BaranScholberg, KateWalter, Chris W.Beauchêne, AntoineDrapier, OlivierGiampaolo, AlbertoMueller, Thomas A.Santos, Andrew D.Paganini, PascalQuilain, BenjaminRogly, RudolphNakamura, TakuJang, Jee-SeungMachado, Lucas N.Learned, John G.Choi, KounIovine, NadegeCao, Son V.Anthony, Lauren H. V.Martin, Daniel G. R.Prouse, Nick W.Scott, MarkUchida, YoshiBerardi, VincenzoCalabria, Nicola F.Catanesi, M. G.Radicioni, EmilioLangella, Aurorade Rosa, GianfrancaCollazuol, GianmariaFeltre, MatteoIacob, FabioMattiazzi, MarcoLudovici, LucioGonin, MichelPérissé, LorenzoPronost, GuillaumeFujisawa, ChioriHoriuchi, ShogoKobayashi, MisakiLiu, Yu-MingMaekawa, YutoNishimura, YasuhiroOkazaki, ReoAkutsu, RyosukeFriend, MeganHasegawa, TakuyaIshida, TakuKobayashi, TakashiJakkapu, MaheshMatsubara, TsunayukiNakadaira, TakeshiNakamura, KenzoOyama, YuichiSakashita, KenSekiguchi, TetsuroTsukamoto, ToshifumiYrey, Antoniosk PortocarreroBhuiyan, NahidBurton, George T.Di Lodovico, FrancescaGao, JoannaGoldsack, AlexanderKatori, TeppeiMigenda, JostRamsden, Rory M.Xie, ZhenxiongZsoldos, StephaneSuzuki, Atsumu T.Takagi, YusukeTakeuchi, YasuoZhong, HaiwenFeng, JiahuiFeng, Li-ChengHu, JianrunHu, ZhuojunKawaue, MasakiKikawa, TatsuyaMori, MasamitsuNakaya, TsuyoshiWendell, Roger A.Yasutome, KenjiJenkins, Sam J.McCauley, Neil K.Mehta, PruthviTarrant, AdamWilking, Mike J.Fukuda, YoshiyukiItow, YoshitakaMenjo, HiroakiNinomiya, KotaroYoshioka, YushiLagoda, JustynaMandal, MaitrayeeMijakowski, PiotrPrabhu, Yashwanth S.Zalipska, JoannaJia, MoJiang, JunjieShi, WeiYanagisawa, ChiakiHarada, MasayukiHino, YotaIshino, HirokazuKoshio, YusukeNakanishi, FumiSakai, SeiyaTada, TomoakiTano, TomohiroIshizuka, TakeharuBarr, GilesBarrow, DanielCook, LaurenceSamani, SoniyaWark, DavidHolin, AnnaNova, FedericoJung, SeunghyunYang, ByeongsuYang, JeongYeolYoo, JongheeFannon, Jack E. P.Kneale, LizMalek, MatthewMcElwee, Jordan M.Thiesse, Matthew D.Thompson, Lee F.Wilson, Stephen T.Okazawa, HirokoMohan, Lakshmi S.Kim, SooBongKwon, EunhyangSeo, Ji-WoongYu, IntaeIchikawa, Atsuko K.Nakamura, Kiseki D.Tairafune, SeidaiNishijima, KyoshiEguchi, AoiNakagiri, KotaNakajima, YasuhiroShima, ShizukaTaniuchi, NatsumiWatanabe, EiichiroYokoyama, Masashide Perio, PatrickFujita, SakiJesus-Valls, CesarMartens, KaiTsui, Ka M.Vagins, Mark R.Xia, JunjieIzumiyama, ShotaKuze, MasahiroMatsumoto, RyoTerada, KotaroAsaka, RyuseiIshitsuka, MasakiIto, HiroshiOmmura, YugaShigeta, NatsukiShinoki, MasatakaYamauchi, KokiYoshida, TsukasaGaur, RheaGousy-Leblan, VincentHartz, MarkKonaka, AkiraLi, XiaoyueChen, ShaominXu, BendaZhang, AiqiangZhang, BinPosiadala-Zezula, MagdalenaBoyd, Steven B.Edwards, RoryHadley, DavidNicholson, MatthewO'Flaherty, MarcusRichards, BenjaminAli, AjmiJamieson, BlairAmanai, ShogoMarti-Magro, LluisMinamino, AkihiroShibayama, RyoSuzuki, Serina
Source
Subject
High Energy Physics - Experiment
Astrophysics - High Energy Astrophysical Phenomena
Physics - Instrumentation and Detectors
Language
Abstract
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 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 is 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.
Comment: 22 pages, 16 figures, for more information about the combined pre-supernova alert system, see https://www.lowbg.org/presnalarm/