Study of TeV neutrinos with upward showering muons in Super-Kamiokande

S. Desai; K. Abe; Y. Hayato; K. Iida; K. Ishihara; J. Kameda; Y. Koshio; A. Minamino; C. Mitsuda; M. Miura; S. Moriyama; M. Nakahata; Y. Obayashi; H. Ogawa; M. Shiozawa; Y. Suzuki; A. Takeda; Y. Takeuchi; K. Ueshima; H. Watanabe; S. Yamada; I. Higuchi; C. Ishihara; M. Ishitsuka; T. Kajita; K. Kaneyuki; G. Mitsuka; S. Nakayama; H. Nishino; K. Okumura; C. Saji; Y. Takenaga; S. T. Clark; F. Dufour; E. Kearns; S. Likhoded; J. L. Raaf; J. L. Stone; L. R. Sulak; W. Wang; M. Goldhaber; D. Casper; J. P. Cravens; J. Dunmore; W. R. Kropp; D. W. Liu; S. Mine; C. Regis; M. B. Smy; H. W. Sobel; M. R. Vagins; K. S. Ganezer; B. Hartfiel; J. Hill; W. E. Keig; J. S. Jang; I. S. Jeong; J. Y. Kim; I. T. Lim; M. Fechner; K. Scholberg; N. Tanimoto; C. W. Walter; R. Wendell; S. Tasaka; G. Guillian; J. G. Learned; S. Matsuno; M. D. Messier; A. K. Ichikawa; T. Ishida; T. Ishii; T. Kobayashi; T. Nakadaira; K. Nakamura; K. Nitta; Y. Oyama; Y. Totsuka; A. T. Suzuki; M. Hasegawa; K. Hiraide; I. Kato; H. Maesaka; T. Nakaya; K. Nishikawa; T. Sasaki; H. Sato; S. Yamamoto; M. Yokoyama; T. J. Haines; S. Dazeley; S. Hatakeyama; R. Svoboda; M. Swanson; A. Clough; R. Gran; A. Habig; Y. Fukuda; T. Sato; Y. Itow; T. Koike; T. Tanaka; C. K. Jung; T. Kato; K. Kobayashi; C. McGrew; A. Sarrat; R. Terri; C. Yanagisawa; N. Tamura; Y. Idehara; M. Sakuda; M. Sugihara; Y. Kuno; M. Yoshida; S. B. Kim; B. S. Yang; J. Yoo; T. Ishizuka; H. Okazawa; Y. Choi; H. K. Seo; Y. Gando; T. Hasegawa; K. Inoue; Y. Furuse; H. Ishii; K. Nishijima; H. Ishino; Y. Watanabe; M. Koshiba; D. Kielczewska; H. Berns; K. K. Shiraishi; E. Thrane; K. Washburn; R. J. Wilkes

doi:10.1016/j.astropartphys.2007.11.005

Study of TeV neutrinos with upward showering muons in Super-Kamiokande

S. Desai
, K. Abe
, Y. Hayato
, K. Iida
, K. Ishihara
, J. Kameda
, Y. Koshio
, A. Minamino
, C. Mitsuda
, M. Miura
, S. Moriyama
, M. Nakahata
, Y. Obayashi
, H. Ogawa
, M. Shiozawa
, Y. Suzuki
, A. Takeda
, Y. Takeuchi
, K. Ueshima
, H. Watanabe

S. Yamada, I. Higuchi, C. Ishihara, M. Ishitsuka, T. Kajita, K. Kaneyuki, G. Mitsuka, S. Nakayama, H. Nishino, K. Okumura, C. Saji, Y. Takenaga, S. T. Clark, F. Dufour, E. Kearns, S. Likhoded, J. L. Raaf, J. L. Stone, L. R. Sulak, W. Wang, M. Goldhaber, D. Casper, J. P. Cravens, J. Dunmore, W. R. Kropp, D. W. Liu, S. Mine, C. Regis, M. B. Smy, H. W. Sobel, M. R. Vagins, K. S. Ganezer, B. Hartfiel, J. Hill, W. E. Keig, J. S. Jang, I. S. Jeong, J. Y. Kim, I. T. Lim, M. Fechner, K. Scholberg, N. Tanimoto, C. W. Walter, R. Wendell, S. Tasaka, G. Guillian, J. G. Learned, S. Matsuno, M. D. Messier, A. K. Ichikawa, T. Ishida, T. Ishii, T. Kobayashi, T. Nakadaira, K. Nakamura, K. Nitta, Y. Oyama, Y. Totsuka, A. T. Suzuki, M. Hasegawa, K. Hiraide, I. Kato, H. Maesaka, T. Nakaya, K. Nishikawa, T. Sasaki, H. Sato, S. Yamamoto, M. Yokoyama, T. J. Haines, S. Dazeley, S. Hatakeyama, R. Svoboda, M. Swanson, A. Clough, R. Gran, A. Habig, Y. Fukuda, T. Sato, Y. Itow, T. Koike, T. Tanaka, C. K. Jung, T. Kato, K. Kobayashi, C. McGrew, A. Sarrat, R. Terri, C. Yanagisawa, N. Tamura, Y. Idehara, M. Sakuda, M. Sugihara, Y. Kuno, M. Yoshida, S. B. Kim, B. S. Yang, J. Yoo, T. Ishizuka, H. Okazawa, Y. Choi, H. K. Seo, Y. Gando, T. Hasegawa, K. Inoue, Y. Furuse, H. Ishii, K. Nishijima, H. Ishino, Y. Watanabe, M. Koshiba, D. Kielczewska, H. Berns, K. K. Shiraishi, E. Thrane, K. Washburn, R. J. Wilkes

Physics and Astronomy

Sungkyunkwan University
The University of Tokyo
Shizuoka University
Tohoku University
Tokai University
Institute of Science Tokyo
University of Warsaw
University of Washington
Boston University
Brookhaven National Laboratory
University of California at Irvine
California State University Dominguez Hills
Chonnam National University
Duke University
Gifu University
University of Hawai'i at Mānoa
Indiana University Bloomington
High Energy Accelerator Research Organization, Tsukuba
Kobe University
Kyoto University
Los Alamos National Laboratory
Louisiana State University
Massachusetts Institute of Technology
Miyagi University of Education
University of Minnesota Duluth
Nagoya University
Stony Brook University
Niigata University
Okayama University
The University of Osaka
Seoul National University
International and Cultural Studies

Research output: Contribution to journal › Article › peer-review

55 Scopus citations

Abstract

A subset of neutrino-induced upward through-going muons in the Super-Kamiokande detector consists of high-energy muons which lose energy through radiative processes such as bremsstrahlung, e⁺ e^- pair production and photonuclear interactions. These "upward showering muons" comprise an event sample whose mean parent neutrino energy is approximately 1 TeV. We show that the zenith angle distribution of upward showering muons is consistent with negligible distortion due to neutrino oscillations, as expected of such a high-energy neutrino sample. We present astronomical searches using these high-energy events, such as those from WIMP annihilations in the Sun, Earth and Galactic Center, some suspected point sources, as well as searches for diffuse flux from the interstellar medium.

Original language	English
Pages (from-to)	42-54
Number of pages	13
Journal	Astroparticle Physics
Volume	29
Issue number	1
DOIs	https://doi.org/10.1016/j.astropartphys.2007.11.005
State	Published - Feb 2008

Keywords

95.55.Ka
95.55.Vj
96.40.Pq
Astrophysics
High-energy neutrinos
Muon energy losses

Access to Document

10.1016/j.astropartphys.2007.11.005

Cite this

Desai, S., Abe, K., Hayato, Y., Iida, K., Ishihara, K., Kameda, J., Koshio, Y., Minamino, A., Mitsuda, C., Miura, M., Moriyama, S., Nakahata, M., Obayashi, Y., Ogawa, H., Shiozawa, M., Suzuki, Y., Takeda, A., Takeuchi, Y., Ueshima, K., ... Wilkes, R. J. (2008). Study of TeV neutrinos with upward showering muons in Super-Kamiokande. Astroparticle Physics, 29(1), 42-54. https://doi.org/10.1016/j.astropartphys.2007.11.005

@article{cfc7235f5f1944f6a564801c245e682a,

title = "Study of TeV neutrinos with upward showering muons in Super-Kamiokande",

abstract = "A subset of neutrino-induced upward through-going muons in the Super-Kamiokande detector consists of high-energy muons which lose energy through radiative processes such as bremsstrahlung, e+ e- pair production and photonuclear interactions. These {"}upward showering muons{"} comprise an event sample whose mean parent neutrino energy is approximately 1 TeV. We show that the zenith angle distribution of upward showering muons is consistent with negligible distortion due to neutrino oscillations, as expected of such a high-energy neutrino sample. We present astronomical searches using these high-energy events, such as those from WIMP annihilations in the Sun, Earth and Galactic Center, some suspected point sources, as well as searches for diffuse flux from the interstellar medium.",

keywords = "95.55.Ka, 95.55.Vj, 96.40.Pq, Astrophysics, High-energy neutrinos, Muon energy losses",

author = "S. Desai and K. Abe and Y. Hayato and K. Iida and K. Ishihara and J. Kameda and Y. Koshio and A. Minamino and C. Mitsuda and M. Miura and S. Moriyama and M. Nakahata and Y. Obayashi and H. Ogawa and M. Shiozawa and Y. Suzuki and A. Takeda and Y. Takeuchi and K. Ueshima and H. Watanabe and S. Yamada and I. Higuchi and C. Ishihara and M. Ishitsuka and T. Kajita and K. Kaneyuki and G. Mitsuka and S. Nakayama and H. Nishino and K. Okumura and C. Saji and Y. Takenaga and Clark, \{S. T.\} and F. Dufour and E. Kearns and S. Likhoded and Raaf, \{J. L.\} and Stone, \{J. L.\} and Sulak, \{L. R.\} and W. Wang and M. Goldhaber and D. Casper and Cravens, \{J. P.\} and J. Dunmore and Kropp, \{W. R.\} and Liu, \{D. W.\} and S. Mine and C. Regis and Smy, \{M. B.\} and Sobel, \{H. W.\} and Vagins, \{M. R.\} and Ganezer, \{K. S.\} and B. Hartfiel and J. Hill and Keig, \{W. E.\} and Jang, \{J. S.\} and Jeong, \{I. S.\} and Kim, \{J. Y.\} and Lim, \{I. T.\} and M. Fechner and K. Scholberg and N. Tanimoto and Walter, \{C. W.\} and R. Wendell and S. Tasaka and G. Guillian and Learned, \{J. G.\} and S. Matsuno and Messier, \{M. D.\} and Ichikawa, \{A. K.\} and T. Ishida and T. Ishii and T. Kobayashi and T. Nakadaira and K. Nakamura and K. Nitta and Y. Oyama and Y. Totsuka and Suzuki, \{A. T.\} and M. Hasegawa and K. Hiraide and I. Kato and H. Maesaka and T. Nakaya and K. Nishikawa and T. Sasaki and H. Sato and S. Yamamoto and M. Yokoyama and Haines, \{T. J.\} and S. Dazeley and S. Hatakeyama and R. Svoboda and M. Swanson and A. Clough and R. Gran and A. Habig and Y. Fukuda and T. Sato and Y. Itow and T. Koike and T. Tanaka and Jung, \{C. K.\} and T. Kato and K. Kobayashi and C. McGrew and A. Sarrat and R. Terri and C. Yanagisawa and N. Tamura and Y. Idehara and M. Sakuda and M. Sugihara and Y. Kuno and M. Yoshida and Kim, \{S. B.\} and Yang, \{B. S.\} and J. Yoo and T. Ishizuka and H. Okazawa and Y. Choi and Seo, \{H. K.\} and Y. Gando and T. Hasegawa and K. Inoue and Y. Furuse and H. Ishii and K. Nishijima and H. Ishino and Y. Watanabe and M. Koshiba and D. Kielczewska and H. Berns and Shiraishi, \{K. K.\} and E. Thrane and K. Washburn and Wilkes, \{R. J.\}",

year = "2008",

month = feb,

doi = "10.1016/j.astropartphys.2007.11.005",

language = "English",

volume = "29",

pages = "42--54",

journal = "Astroparticle Physics",

issn = "0927-6505",

number = "1",

}

Desai, S, Abe, K, Hayato, Y, Iida, K, Ishihara, K, Kameda, J, Koshio, Y, Minamino, A, Mitsuda, C, Miura, M, Moriyama, S, Nakahata, M, Obayashi, Y, Ogawa, H, Shiozawa, M, Suzuki, Y, Takeda, A, Takeuchi, Y, Ueshima, K, Watanabe, H, Yamada, S, Higuchi, I, Ishihara, C, Ishitsuka, M, Kajita, T, Kaneyuki, K, Mitsuka, G, Nakayama, S, Nishino, H, Okumura, K, Saji, C, Takenaga, Y, Clark, ST, Dufour, F, Kearns, E, Likhoded, S, Raaf, JL, Stone, JL, Sulak, LR, Wang, W, Goldhaber, M, Casper, D, Cravens, JP, Dunmore, J, Kropp, WR, Liu, DW, Mine, S, Regis, C, Smy, MB, Sobel, HW, Vagins, MR, Ganezer, KS, Hartfiel, B, Hill, J, Keig, WE, Jang, JS, Jeong, IS, Kim, JY, Lim, IT, Fechner, M, Scholberg, K, Tanimoto, N, Walter, CW, Wendell, R, Tasaka, S, Guillian, G, Learned, JG, Matsuno, S, Messier, MD, Ichikawa, AK, Ishida, T, Ishii, T, Kobayashi, T, Nakadaira, T, Nakamura, K, Nitta, K, Oyama, Y, Totsuka, Y, Suzuki, AT, Hasegawa, M, Hiraide, K, Kato, I, Maesaka, H, Nakaya, T, Nishikawa, K, Sasaki, T, Sato, H, Yamamoto, S, Yokoyama, M, Haines, TJ, Dazeley, S, Hatakeyama, S, Svoboda, R, Swanson, M, Clough, A, Gran, R, Habig, A, Fukuda, Y, Sato, T, Itow, Y, Koike, T, Tanaka, T, Jung, CK, Kato, T, Kobayashi, K, McGrew, C, Sarrat, A, Terri, R, Yanagisawa, C, Tamura, N, Idehara, Y, Sakuda, M, Sugihara, M, Kuno, Y, Yoshida, M, Kim, SB, Yang, BS, Yoo, J, Ishizuka, T, Okazawa, H, Choi, Y, Seo, HK, Gando, Y, Hasegawa, T, Inoue, K, Furuse, Y, Ishii, H, Nishijima, K, Ishino, H, Watanabe, Y, Koshiba, M, Kielczewska, D, Berns, H, Shiraishi, KK, Thrane, E, Washburn, K & Wilkes, RJ 2008, 'Study of TeV neutrinos with upward showering muons in Super-Kamiokande', Astroparticle Physics, vol. 29, no. 1, pp. 42-54. https://doi.org/10.1016/j.astropartphys.2007.11.005

TY - JOUR

T1 - Study of TeV neutrinos with upward showering muons in Super-Kamiokande

AU - Desai, S.

AU - Abe, K.

AU - Hayato, Y.

AU - Iida, K.

AU - Ishihara, K.

AU - Kameda, J.

AU - Koshio, Y.

AU - Minamino, A.

AU - Mitsuda, C.

AU - Miura, M.

AU - Moriyama, S.

AU - Nakahata, M.

AU - Obayashi, Y.

AU - Ogawa, H.

AU - Shiozawa, M.

AU - Suzuki, Y.

AU - Takeda, A.

AU - Takeuchi, Y.

AU - Ueshima, K.

AU - Watanabe, H.

AU - Yamada, S.

AU - Higuchi, I.

AU - Ishihara, C.

AU - Ishitsuka, M.

AU - Kajita, T.

AU - Kaneyuki, K.

AU - Mitsuka, G.

AU - Nakayama, S.

AU - Nishino, H.

AU - Okumura, K.

AU - Saji, C.

AU - Takenaga, Y.

AU - Clark, S. T.

AU - Dufour, F.

AU - Kearns, E.

AU - Likhoded, S.

AU - Raaf, J. L.

AU - Stone, J. L.

AU - Sulak, L. R.

AU - Wang, W.

AU - Goldhaber, M.

AU - Casper, D.

AU - Cravens, J. P.

AU - Dunmore, J.

AU - Kropp, W. R.

AU - Liu, D. W.

AU - Mine, S.

AU - Regis, C.

AU - Smy, M. B.

AU - Sobel, H. W.

AU - Vagins, M. R.

AU - Ganezer, K. S.

AU - Hartfiel, B.

AU - Hill, J.

AU - Keig, W. E.

AU - Jang, J. S.

AU - Jeong, I. S.

AU - Kim, J. Y.

AU - Lim, I. T.

AU - Fechner, M.

AU - Scholberg, K.

AU - Tanimoto, N.

AU - Walter, C. W.

AU - Wendell, R.

AU - Tasaka, S.

AU - Guillian, G.

AU - Learned, J. G.

AU - Matsuno, S.

AU - Messier, M. D.

AU - Ichikawa, A. K.

AU - Ishida, T.

AU - Ishii, T.

AU - Kobayashi, T.

AU - Nakadaira, T.

AU - Nakamura, K.

AU - Nitta, K.

AU - Oyama, Y.

AU - Totsuka, Y.

AU - Suzuki, A. T.

AU - Hasegawa, M.

AU - Hiraide, K.

AU - Kato, I.

AU - Maesaka, H.

AU - Nakaya, T.

AU - Nishikawa, K.

AU - Sasaki, T.

AU - Sato, H.

AU - Yamamoto, S.

AU - Yokoyama, M.

AU - Haines, T. J.

AU - Dazeley, S.

AU - Hatakeyama, S.

AU - Svoboda, R.

AU - Swanson, M.

AU - Clough, A.

AU - Gran, R.

AU - Habig, A.

AU - Fukuda, Y.

AU - Sato, T.

AU - Itow, Y.

AU - Koike, T.

AU - Tanaka, T.

AU - Jung, C. K.

AU - Kato, T.

AU - Kobayashi, K.

AU - McGrew, C.

AU - Sarrat, A.

AU - Terri, R.

AU - Yanagisawa, C.

AU - Tamura, N.

AU - Idehara, Y.

AU - Sakuda, M.

AU - Sugihara, M.

AU - Kuno, Y.

AU - Yoshida, M.

AU - Kim, S. B.

AU - Yang, B. S.

AU - Yoo, J.

AU - Ishizuka, T.

AU - Okazawa, H.

AU - Choi, Y.

AU - Seo, H. K.

AU - Gando, Y.

AU - Hasegawa, T.

AU - Inoue, K.

AU - Furuse, Y.

AU - Ishii, H.

AU - Nishijima, K.

AU - Ishino, H.

AU - Watanabe, Y.

AU - Koshiba, M.

AU - Kielczewska, D.

AU - Berns, H.

AU - Shiraishi, K. K.

AU - Thrane, E.

AU - Washburn, K.

AU - Wilkes, R. J.

PY - 2008/2

Y1 - 2008/2

N2 - A subset of neutrino-induced upward through-going muons in the Super-Kamiokande detector consists of high-energy muons which lose energy through radiative processes such as bremsstrahlung, e+ e- pair production and photonuclear interactions. These "upward showering muons" comprise an event sample whose mean parent neutrino energy is approximately 1 TeV. We show that the zenith angle distribution of upward showering muons is consistent with negligible distortion due to neutrino oscillations, as expected of such a high-energy neutrino sample. We present astronomical searches using these high-energy events, such as those from WIMP annihilations in the Sun, Earth and Galactic Center, some suspected point sources, as well as searches for diffuse flux from the interstellar medium.

AB - A subset of neutrino-induced upward through-going muons in the Super-Kamiokande detector consists of high-energy muons which lose energy through radiative processes such as bremsstrahlung, e+ e- pair production and photonuclear interactions. These "upward showering muons" comprise an event sample whose mean parent neutrino energy is approximately 1 TeV. We show that the zenith angle distribution of upward showering muons is consistent with negligible distortion due to neutrino oscillations, as expected of such a high-energy neutrino sample. We present astronomical searches using these high-energy events, such as those from WIMP annihilations in the Sun, Earth and Galactic Center, some suspected point sources, as well as searches for diffuse flux from the interstellar medium.

KW - 95.55.Ka

KW - 95.55.Vj

KW - 96.40.Pq

KW - Astrophysics

KW - High-energy neutrinos

KW - Muon energy losses

UR - https://www.scopus.com/pages/publications/38749141850

U2 - 10.1016/j.astropartphys.2007.11.005

DO - 10.1016/j.astropartphys.2007.11.005

M3 - Article

AN - SCOPUS:38749141850

SN - 0927-6505

VL - 29

SP - 42

EP - 54

JO - Astroparticle Physics

JF - Astroparticle Physics

IS - 1

ER -

Study of TeV neutrinos with upward showering muons in Super-Kamiokande

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Keywords

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