학술논문

Search for Boosted Dark Matter Interacting With Electrons in Super-Kamiokande
Document Type
Working Paper
Author
Collaboration, Super-KamiokandeKachulis, C.Abe, K.Bronner, C.Hayato, Y.Ikeda, M.Iyogi, K.Kameda, J.Kato, Y.Kishimoto, Y.Marti, Ll.Miura, M.Moriyama, S.Nakahata, M.Nakano, Y.Nakayama, S.Okajima, Y.Orii, A.Pronost, G.Sekiya, H.Shiozawa, M.Sonoda, Y.Takeda, A.Takenaka, A.Tanaka, H.Tasaka, S.Tomura, T.Akutsu, R.Kajita, T.Kaneyuki, K.Nishimura, Y.Okumura, K.Tsui, K. M.Labarga, L.Fernandez, P.Blaszczyk., F. d. M.Gustafson, J.Kearns, E.Raaf, J. L.Stone, J. L.Sulak, L. R.Berkman, S.Tobayama, S.Goldhaber, M.Elnimr, M.Kropp, W. R.Mine, S.Locke, S.Weatherly, P.Smy, M. B.Sobel, H. W.Takhistov, V.Ganezer, K. S.Hill, J.Kim, J. Y.Lim, I. T.Park, R. G.Himmel, A.Li, Z.O'Sullivan, E.Scholberg, K.Walter, C. W.Ishizuka, T.Nakamura, T.Jang, J. S.Choi, K.Learned, J. G.Matsuno, S.Smith, S. N.Amey, J.Litchfield, R. P.Ma, W. Y.Wascko, Y. Uchida. M. O.Cao, S.Friend, M.Hasegawa, T.Ishida, T.Ishii, T.Kobayashi, T.Nakadaira, T.Nakamura, K.Oyama, Y.Sakashita, K.Sekiguchi, T.Tsukamoto, T.Abe, KE.Hasegawa, M.Suzuki, A. T.Takeuchi, Y.Yano, T.Hayashino, T.Hiraki, T.Hirota, S.Huang, K.Jiang, M.Nakamura, KE.Nakaya, T.Quilain, B.Patel, N. D.Wendell, R. A.Anthony, L. H. V.McCauley, N.Pritchard, A.Fukuda, Y.Itow, Y.Murase, M.Muto, F.Mijakowski, P.Frankiewicz, K.Jung, C. K.Li, X.Palomino, J. L.Santucci, G.Vilela, C.Wilking, M. J.Yanagisawa, C.Ito, S.Fukuda, D.Ishino, H.Kibayashi, A.Koshio, Y.Nagata, H.Sakuda, M.Xu, C.Kuno, Y.Wark, D.Di Lodovico, F.Richards, B.Tacik, R.Kim, S. B.Cole, A.Thompson, L.Okazawa, H.Choi, Y.Ito, K.Nishijima, K.Koshiba, M.Totsuka, Y.Suda, Y.Yokoyama, M.Calland, R. G.Hartz, M.Martens, K.Simpson, C.Suzuki, Y.Vagins, M. R.Hamabe, D.Kuze, M.Yoshida, T.Ishitsuka, M.Martin, J. F.Nantais, C. M.Tanaka, H. A.Konaka, A.Chen, S.Wan, L.Zhang, Y.Wilkes, R. J.Minamino, A.
Source
Phys. Rev. Lett. 120, 221301 (2018)
Subject
High Energy Physics - Experiment
High Energy Physics - Phenomenology
Language
Abstract
A search for boosted dark matter using 161.9 kiloton-years of Super-Kamiokande IV data is presented. We search for an excess of elastically scattered electrons above the atmospheric neutrino background, with a visible energy between 100 MeV and 1 TeV, pointing back to the Galactic Center or the Sun. No such excess is observed. Limits on boosted dark matter event rates in multiple angular cones around the Galactic Center and Sun are calculated. Limits are also calculated for a baseline model of boosted dark matter produced from cold dark matter annihilation or decay.