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Real-time supernova neutrino burst monitor at Super-Kamiokande

Authors
Abe K.[Abe K.]Haga Y.[Haga Y.]Hayato Y.[Hayato Y.]Ikeda M.[Ikeda M.]Iyogi K.[Iyogi K.]Kameda J.[Kameda J.]Kishimoto Y.[Kishimoto Y.]Miura M.[Miura M.]Moriyama S.[Moriyama S.]Nakahata M.[Nakahata M.]Nakano Y.[Nakano Y.]Nakayama S.[Nakayama S.]Sekiya H.[Sekiya H.]Shiozawa M.[Shiozawa M.]Suzuki Y.[Suzuki Y.]Takeda A.[Takeda A.]Tanaka H.[Tanaka H.]Tomura T.[Tomura T.]Ueno K.[Ueno K.]Wendell R.A.[Wendell R.A.]Yokozawa T.[Yokozawa T.]Irvine T.[Irvine T.]Kajita T.[Kajita T.]Kametani I.[Kametani I.]Kaneyuki K.[Kaneyuki K.]Lee K.P.[Lee K.P.]McLachlan T.[McLachlan T.]Nishimura Y.[Nishimura Y.]Richard E.[Richard E.]Okumura K.[Okumura K.]Labarga L.[Labarga L.]Fernandez P.[Fernandez P.]Berkman S.[Berkman S.]Tanaka H.A.[Tanaka H.A.]Tobayama S.[Tobayama S.]Gustafson J.[Gustafson J.]Kearns E.[Kearns E.]Raaf J.L.[Raaf J.L.]Stone J.L.[Stone J.L.]Sulak L.R.[Sulak L.R.]Goldhaber M.[Goldhaber M.]Carminati G.[Carminati G.]Kropp W.R.[Kropp W.R.]Mine S.[Mine S.]Weatherly P.[Weatherly P.]Renshaw A.[Renshaw A.]Smy M.B.[Smy M.B.]Sobel H.W.[Sobel H.W.]Takhistov V.[Takhistov V.]Ganezer K.S.[Ganezer K.S.]Hartfiel B.L.[Hartfiel B.L.]Hill J.[Hill J.]Keig W.E.[Keig W.E.]Hong N.[Hong N.]Kim J.Y.[Kim J.Y.]Lim I.T.[Lim I.T.]Akiri T.[Akiri T.]Himmel A.[Himmel A.]Scholberg K.[Scholberg K.]Walter C.W.[Walter C.W.]Wongjirad T.[Wongjirad T.]Ishizuka T.[Ishizuka T.]Tasaka S.[Tasaka S.]Jang J.S.[Jang J.S.]Learned J.G.[Learned J.G.]Matsuno S.[Matsuno S.]Smith S.N.[Smith S.N.]Hasegawa T.[Hasegawa T.]Ishida T.[Ishida T.]Ishii T.[Ishii T.]Kobayashi T.[Kobayashi T.]Nakadaira T.[Nakadaira T.]Nakamura K.[Nakamura K.]Oyama Y.[Oyama Y.]Sakashita K.[Sakashita K.]Sekiguchi T.[Sekiguchi T.]Tsukamoto T.[Tsukamoto T.]Suzuki A.T.[Suzuki A.T.]Takeuchi Y.[Takeuchi Y.]Bronner C.[Bronner C.]Hirota S.[Hirota S.]Huang K.[Huang K.]Ieki K.[Ieki K.]Kikawa T.[Kikawa T.]Minamino A.[Minamino A.]Murakami A.[Murakami A.]Nakaya T.[Nakaya T.]Suzuki K.[Suzuki K.]Takahashi S.[Takahashi S.]Tateishi K.[Tateishi K.]Fukuda Y.[Fukuda Y.]Choi K.[Choi K.]Itow Y.[Itow Y.]Mitsuka G.[Mitsuka G.]Mijakowski P.[Mijakowski P.]Hignight J.[Hignight J.]Imber J.[Imber J.]Jung C.K.[Jung C.K.]Yanagisawa C.[Yanagisawa C.]Wilking M.J.[Wilking M.J.]Ishino H.[Ishino H.]Kibayashi A.[Kibayashi A.]Koshio Y.[Koshio Y.]Mori T.[Mori T.]Sakuda M.[Sakuda M.]Yamaguchi R.[Yamaguchi R.]Yano T.[Yano T.]Kuno Y.[Kuno Y.]Tacik R.[Tacik R.]Kim S.B.[Kim S.B.]Okazawa H.[Okazawa H.]Choi Y.[Choi Y.]Nishijima K.[Nishijima K.]Koshiba M.[Koshiba M.]Suda Y.[Suda Y.]Totsuka Y.[Totsuka Y.]Yokoyama M.[Yokoyama M.]Martens K.[Martens K.]Marti L.[Marti L.]Vagins M.R.[Vagins M.R.]Martin J.F.[Martin J.F.]De Perio P.[De Perio P.]Konaka A.[Konaka A.]Chen S.[Chen S.]Zhang Y.[Zhang Y.]Connolly K.[Connolly K.]Wilkes R.J.[Wilkes R.J.]
Issue Date
Aug-2016
Publisher
ELSEVIER SCIENCE BV
Keywords
Neutrinos; Super-Kamiokande; Supernova
Citation
ASTROPARTICLE PHYSICS, v.81, pp.39 - 48
Indexed
SCIE
SCOPUS
Journal Title
ASTROPARTICLE PHYSICS
Volume
81
Start Page
39
End Page
48
URI
https://scholarworks.bwise.kr/skku/handle/2021.sw.skku/35856
DOI
10.1016/j.astropartphys.2016.04.003
ISSN
0927-6505
Abstract
We present a real-time supernova neutrino burst monitor at Super-Kamiokande (SIC). Detecting supernova explosions by neutrinos in real time is crucial for giving a clear picture of the explosion mechanism. Since the neutrinos are expected to come earlier than light, a fast broadcasting of the detection may give astronomers a chance to make electromagnetic radiation observations of the explosions right at the onset. The role of the monitor includes a fast announcement of the neutrino burst detection to the world and a determination of the supernova direction. We present the online neutrino burst detection system and studies of the direction determination accuracy based on simulations at SK. (C) 2016 Elsevier B.V. All rights reserved.
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