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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