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Indirect search for dark matter from the Galactic Center and halo with the Super-Kamiokande detector

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Title: Indirect search for dark matter from the Galactic Center and halo with the Super-Kamiokande detector
Authors: Abe, K
Bronner, C
Haga, Y
Hayato, Y
Ikeda, M
Imaizumi, S
Ito, H
Iyogi, K
Kameda, J
Kataoka, Y
Kato, Y
Kishimoto, Y
Marti, L
Miura, M
Moriyama, S
Mochizuki, T
Nagao, Y
Nakahata, M
Nakajima, Y
Nakajima, T
Nakayama, S
Okada, T
Okamoto, K
Orii, A
Pronost, G
Sekiya, H
Shiozawa, M
Sonoda, Y
Takeda, A
Takenaka, A
Tanaka, H
Tasaka, S
Tomura, T
Ueno, K
Yano, T
Yokozawa, T
Akutsu, R
Han, S
Irvine, T
Kajita, T
Kametani, I
Lee, KP
McLachlan, T
Okumura, K
Richard, E
Tashiro, T
Wang, R
Xia, J
Bravo-Berguno, D
Labarga, L
Fernandez, P
Blaszczyk, FDM
Gustafson, J
Kachulis, C
Kearns, E
Raaf, JL
Stone, JL
Sulak, LR
Sussman, S
Wan, L
Wester, T
Berkman, S
Tobayama, S
Bian, J
Carminati, G
Elnimr, M
Griskevich, NJ
Kropp, WR
Locke, S
Mine, S
Renshaw, A
Smy, MB
Sobel, HW
Takhistov, V
Weatherly, P
Hartfiel, BL
Hill, J
Keig, WE
Hong, N
Kim, JY
Lim, IT
Park, RG
Akiri, T
Bodur, B
Himmel, A
Li, Z
O'Sullivan, E
Scholberg, K
Walter, CW
Wongjirad, T
Coffani, A
Drapier, O
El Hedri, S
Giampaolo, A
Gonin, M
Imber, J
Mueller, TA
Paganini, P
Quilain, B
Ishizuka, T
Nakamura, T
Jang, JS
Choi, K
Learned, JG
Matsuno, S
Smith, SN
Amey, J
Anthony, LH
Litchfield, RP
Sztuc, AA
Uchida, Y
Wascko, MO
Berardi, V
Catanesi, MG
Intonti, RA
Radicioni, E
Calabria, NF
Machado, LN
De Rosa, G
Collazuol, G
Iacob, F
Lamoureux, M
Ospina, N
Ludovici, L
Boschi, T
Di Lodovico, F
Sedgwick, SM
Zsoldos, S
Nishimura, Y
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, K
Hasegawa, M
Isobe, Y
Miyabe, H
Nakano, Y
Shiozawa, T
Sugimoto, T
Suzuki, AT
Takeuchi, Y
Yamamoto, S
Ali, A
Ashida, Y
Hayashino, T
Hiraki, T
Hirota, S
Huang, K
Ieki, K
Jiang, M
Kikawa, T
Mori, M
Murakami, A
Nakamura, KE
Nakaya, T
Patel, ND
Suzuki, K
Takahashi, S
Tateishi, K
Wendell, RA
McCauley, N
Mehta, P
Pritchard, A
Tsui, KM
Fukuda, Y
Itow, Y
Menjo, H
Mitsuka, G
Murase, M
Muto, F
Niwa, T
Sato, K
Suzuki, T
Taani, M
Tsukada, M
Mijakowski, P
Frankiewicz, K
Hignight, J
Jung, CK
Li, X
Palomino, JL
Santucci, G
Vilela, C
Wilking, MJ
Yanagisawa, C
Fukuda, D
Hagiwara, K
Harada, M
Horai, T
Ishino, H
Ito, S
Kayano, T
Kibayashi, A
Koshio, Y
Ma, W
Mori, T
Nagata, H
Piplani, N
Sakuda, M
Seiya, S
Takahira, Y
Xu, C
Yamaguchi, R
Kuno, Y
Barr, G
Barrow, D
Cook, L
Simpson, C
Wark, D
Nova, F
Tacik, R
Yang, JY
Cole, A
Jenkins, SJ
McElwee, J
Thiesse, M
Thompson, L
Okazawa, H
Kim, SB
Choi, Y
Ito, K
Nishijima, K
Iwamoto, K
Koshiba, M
Suda, Y
Yokoyama, M
Calland, RG
Goldsack, A
Martens, K
Murdoch, M
Suzuki, Y
Vagins, MR
Hamabe, D
Kuze, M
Okajima, Y
Tanaka, M
Yoshida, T
Inomoto, M
Ishitsuka, M
Matsumoto, R
Ohta, K
Shinoki, M
Martin, JF
Nantais, CM
Tanaka, HA
Towstego, T
Hartz, M
Konaka, A
De Perio, P
Prouse, NW
Chen, S
Xu, BD
Zhang, Y
Richards, B
Connolly, K
Wilkes, RJ
Jamieson, B
Walker, J
Giorgio, P
Minamino, A
Pintaudi, G
Item Type: Journal Article
Abstract: We present a search for an excess of neutrino interactions due to dark matter in the form of weakly interacting massive particles (WIMPs) annihilating in the Galactic center or halo based on the data set of Super-Kamiokande-I, -II, -III and -IV taken from 1996 to 2016. We model the neutrino flux, energy, and flavor distributions assuming WIMP self-annihilation is dominant to ν ¯ ν , μ + μ − , b ¯ b , or W + W − . The excess is in comparison to atmospheric neutrino interactions which are modeled in detail and fit to data. Limits on the self-annihilation cross section ⟨ σ A V ⟩ are derived for WIMP masses in the range 1 GeV to 10 TeV, reaching as low as 9.6 × 10 − 23     cm 3   s − 1 for 5 GeV WIMPs in b ¯ b mode and 1.2 × 10 − 24     cm 3   s − 1 for 1 GeV WIMPs in ν ¯ ν mode. The obtained sensitivity of the Super-Kamiokande detector to WIMP masses below several tens of GeV is the best among similar indirect searches to date.
Issue Date: 9-Oct-2020
Date of Acceptance: 9-Sep-2020
URI: http://hdl.handle.net/10044/1/84547
DOI: 10.1103/PhysRevD.102.072002
ISSN: 1550-2368
Publisher: American Physical Society
Start Page: 072002 – 1
End Page: 072002 – 14
Journal / Book Title: Physical Review D: Particles, Fields, Gravitation and Cosmology
Volume: 102
Issue: 7
Copyright Statement: © 2020 The Author(s). Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.
Sponsor/Funder: Science and Technology Facilities Council (STFC)
Science and Technology Facilities Council (STFC)
Funder's Grant Number: ST/K001604/1
ST/S001174/4
Keywords: Science & Technology
Physical Sciences
Astronomy & Astrophysics
Physics, Particles & Fields
Physics
ANNIHILATIONS
PARTICLES
Science & Technology
Physical Sciences
Astronomy & Astrophysics
Physics, Particles & Fields
Physics
ANNIHILATIONS
PARTICLES
0201 Astronomical and Space Sciences
0202 Atomic, Molecular, Nuclear, Particle and Plasma Physics
0206 Quantum Physics
Nuclear & Particles Physics
Publication Status: Published
Open Access location: https://journals.aps.org/prd/abstract/10.1103/PhysRevD.102.072002
Article Number: ARTN 072002
Online Publication Date: 2020-10-09
Appears in Collections:Physics
High Energy Physics



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