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Search for Boosted Dark Matter Interacting With Electrons in Super-Kamiokande

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arxiv 1711.05278 v2 pith:GFFTVZ53 submitted 2017-11-14 hep-ex hep-ph

Super-Kamiokande Collaboration: C. Kachulis , K. Abe , C. Bronner , Y. Hayato , M. Ikeda , K. Iyogi , J. Kameda , Y. Kato
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Y. Kishimoto Ll. Marti M. Miura S. Moriyama M. Nakahata Y. Nakano S. Nakayama Y. Okajima A. Orii G. Pronost H. Sekiya M. Shiozawa Y. Sonoda A. Takeda A. Takenaka H. Tanaka S. Tasaka T. Tomura R. Akutsu T. Kajita K. Kaneyuki Y. Nishimura K. Okumura K. M. Tsui L. Labarga P. Fernandez F. d. M. Blaszczyk. J. Gustafson E. Kearns J. L. Raaf J. L. Stone L. R. Sulak S. Berkman S. Tobayama M. Goldhaber M. Elnimr W. R. Kropp S. Mine S. Locke P. Weatherly M. B. Smy H. W. Sobel V. Takhistov K. S. Ganezer J. Hill J. Y. Kim I. T. Lim R. G. Park A. Himmel Z. Li E. O'Sullivan K. Scholberg C. W. Walter T. Ishizuka T. Nakamura J. S. Jang K. Choi J. G. Learned S. Matsuno S. N. Smith J. Amey R. P. Litchfield W. Y. Ma Y. Uchida. M. O. Wascko S. Cao M. Friend T. Hasegawa T. Ishida T. Ishii T. Kobayashi T. Nakadaira K. Nakamura Y. Oyama K. Sakashita T. Sekiguchi T. Tsukamoto KE. Abe M. Hasegawa A. T. Suzuki Y. Takeuchi T. Yano T. Hayashino T. Hiraki S. Hirota K. Huang M. Jiang KE. Nakamura T. Nakaya B. Quilain N. D. Patel R. A. Wendell L. H. V. Anthony N. McCauley A. Pritchard Y. Fukuda Y. Itow M. Murase F. Muto P. Mijakowski K. Frankiewicz C. K. Jung X. Li J. L. Palomino G. Santucci C. Vilela M. J. Wilking C. Yanagisawa S. Ito D. Fukuda H. Ishino A. Kibayashi Y. Koshio H. Nagata M. Sakuda C. Xu Y. Kuno D. Wark F. Di Lodovico B. Richards R. Tacik S. B. Kim A. Cole L. Thompson H. Okazawa Y. Choi K. Ito K. Nishijima M. Koshiba Y. Totsuka Y. Suda M. Yokoyama R. G. Calland M. Hartz K. Martens C. Simpson Y. Suzuki M. R. Vagins D. Hamabe M. Kuze T. Yoshida M. Ishitsuka J. F. Martin C. M. Nantais H. A. Tanaka A. Konaka S. Chen L. Wan Y. Zhang R. J. Wilkes A. Minamino
This is my paper · ORCID
classification hep-exhep-ph
keywords darkmatterboostedsearchcalculatedcenterelectronsexcess
verification ladder T0 review T1 audit T2 compute T3 formal

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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.

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