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Search for n - (n)over-bar oscillation in Super-Kamiokandeopen access

Authors
Abe, K[Abe, K.]Hayato, Y[Hayato, Y.]Iida, T[Iida, T.]Ishihara, K[Ishihara, K.]Kameda, J[Kameda, J.]Koshio, Y[Koshio, Y.]Minamino, A[Minamino, A.]Mitsuda, C[Mitsuda, C.]Miura, M[Miura, M.]Moriyama, S[Moriyama, S.]Nakahata, M[Nakahata, M.]Obayashi, Y[Obayashi, Y.]Ogawa, H[Ogawa, H.]Sekiya, H[Sekiya, H.]Shiozawa, M[Shiozawa, M.]Suzuki, Y[Suzuki, Y.]Takeda, A[Takeda, A.]Takeuchi, Y[Takeuchi, Y.]Ueshima, K[Ueshima, K.]Watanabe, H[Watanabe, H.]Higuchi, I[Higuchi, I.]Ishihara, C[Ishihara, C.]Ishitsuka, M[Ishitsuka, M.]Kajita, T[Kajita, T.]Kaneyuki, K[Kaneyuki, K.]Mitsuka, G[Mitsuka, G.]Nakayama, S[Nakayama, S.]Nishino, H[Nishino, H.]Okumura, K[Okumura, K.]Saji, C[Saji, C.]Takenaga, Y[Takenaga, Y.]Clark, S[Clark, S.]Desai, S[Desai, S.]Dufour, F[Dufour, F.]Herfurth, A[Herfurth, A.]Kearns, E[Kearns, E.]Likhoded, S[Likhoded, S.]Litos, M[Litos, M.]Raaf, JL[Raaf, J. L.]Stone, JL[Stone, J. L.]Sulak, LR[Sulak, L. R.]Wang, W[Wang, W.]Goldhaber, M[Goldhaber, M.]Casper, D[Casper, D.]Cravens, JP[Cravens, J. P.]Dunmore, J[Dunmore, J.]Griskevich, J[Griskevich, J.]Kropp, WR[Kropp, W. R.]Liu, DW[Liu, D. W.]Mine, S[Mine, S.]Regis, C[Regis, C.]Smy, MB[Smy, M. B.]Sobel, HW[Sobel, H. W.]Vagins, MR[Vagins, M. R.]Ganezer, KS[Ganezer, K. S.]Hartfiel, B[Hartfiel, B.]Hill, J[Hill, J.]Keig, WE[Keig, W. E.]Jang, JS[Jang, J. S.]Jeoung, IS[Jeoung, I. S.]Kim, JY[Kim, J. Y.]Lim, IT[Lim, I. T.]Scholberg, K[Scholberg, K.]Tanimoto, N[Tanimoto, N.]Walter, CW[Walter, C. W.]Wendell, R[Wendell, R.]Ellsworth, RW[Ellsworth, R. W.]Tasaka, S[Tasaka, S.]Guillian, G[Guillian, G.]Learned, JG[Learned, J. G.]Matsuno, S[Matsuno, S.]Messier, MD[Messier, M. D.]Ichikawa, AK[Ichikawa, A. K.]Ishida, T[Ishida, T.]Ishii, T[Ishii, T.]Iwashita, T[Iwashita, T.]Kobayashi, T[Kobayashi, T.]Nakadaira, T[Nakadaira, T.]Nakamura, K[Nakamura, K.]Nishikawa, K[Nishikawa, K.]Nitta, K[Nitta, K.]Oyama, Y[Oyama, Y.]Suzuki, AT[Suzuki, A. T.]Hasegawa, M[Hasegawa, M.]Maesaka, H[Maesaka, H.]Nakaya, T[Nakaya, T.]Sasaki, T[Sasaki, T.]Sato, H[Sato, H.]Tanaka, H[Tanaka, H.]Yamamoto, S[Yamamoto, S.]Yokoyama, M[Yokoyama, M.]Haines, TJ[Haines, T. J.]Dazeley, S[Dazeley, S.]Hatakeyama, S[Hatakeyama, S.]Svoboda, R[Svoboda, R.]Sullivan, GW[Sullivan, G. W.]Gran, R[Gran, R.]Habig, A[Habig, A.]Fukuda, Y[Fukuda, Y.]Itow, Y[Itow, Y.]Koike, T[Koike, T.]Jung, CK[Jung, C. K.]Kato, T[Kato, T.]Kobayashi, K[Kobayashi, K.]McGrew, C[McGrew, C.]Sarrat, A[Sarrat, A.]Terri, R[Terri, R.]Yanagisawa, C[Yanagisawa, C.]Tamura, N[Tamura, N.]Ikeda, M[Ikeda, M.]Sakuda, M[Sakuda, M.]Kuno, Y[Kuno, Y.]Yoshida, M[Yoshida, M.]Kim, SB[Kim, S. B.]Yang, BS[Yang, B. S.]Ishizuka, T[Ishizuka, T.]Okazawa, H[Okazawa, H.]Choi, Y[Choi, Y.]Seo, HK[Seo, H. K.]Gando, Y[Gando, Y.]Hasegawa, T[Hasegawa, T.]Inoue, K[Inoue, K.]Ishii, H[Ishii, H.]Nishijima, K[Nishijima, K.]Ishino, H[Ishino, H.]Watanabe, Y[Watanabe, Y.]Koshiba, M[Koshiba, M.]Totsuka, Y[Totsuka, Y.]Chen, S[Chen, S.]Deng, Z[Deng, Z.]Liu, Y[Liu, Y.]Kielczewska, D[Kielczewska, D.]Berns, HG[Berns, H. G.]Shiraishi, KK[Shiraishi, K. K.]Thrane, E[Thrane, E.]Washburn, K[Washburn, K.]Wilkes, RJ[Wilkes, R. J.]
Issue Date
10-Apr-2015
Publisher
AMER PHYSICAL SOC
Citation
PHYSICAL REVIEW D, v.91, no.7
Indexed
SCIE
SCOPUS
Journal Title
PHYSICAL REVIEW D
Volume
91
Number
7
URI
https://scholarworks.bwise.kr/skku/handle/2021.sw.skku/44160
DOI
10.1103/PhysRevD.91.072006
ISSN
1550-7998
Abstract
A search for neutron-antineutron (n - (n) over bar n) oscillation was undertaken in Super-Kamiokande using the 1489 live-day or 2.45 x 10(34) neutron-year exposure data. This process violates both baryon and baryon minus lepton numbers by an absolute value of two units and is predicted by a large class of hypothetical models where the seesaw mechanism is incorporated to explain the observed tiny neutrino masses and the matter-antimatter asymmetry in the Universe. No evidence for n - (n) over bar oscillation was found; the lower limit of the lifetime for neutrons bound in O-16, in an analysis that included all of the significant sources of experimental uncertainties, was determined to be 1.9 x 10(32) years at the 90% confidence level. The corresponding lower limit for the oscillation time of free neutrons was calculated to be 2.7 x 10(8) s using a theoretical value of the nuclear suppression factor of 0.517 x 10(23) s(-1) and its uncertainty.
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