ScholarWorks@SUNGKYUNKWAN UNIVERSITY

Detailed Information

Cited 66 time in webofscience Cited 94 time in scopus
Metadata Downloads

First Indication of Terrestrial Matter Effects on Solar Neutrino Oscillation

Full metadata record
DC Field Value Language
dc.contributor.authorRenshaw, A[Renshaw, A.]-
dc.contributor.authorAbe, K[Abe, K.]-
dc.contributor.authorHayato, Y[Hayato, Y.]-
dc.contributor.authorIyogi, K[Iyogi, K.]-
dc.contributor.authorKameda, J[Kameda, J.]-
dc.contributor.authorKishimoto, Y[Kishimoto, Y.]-
dc.contributor.authorMiura, M[Miura, M.]-
dc.contributor.authorMoriyama, S[Moriyama, S.]-
dc.contributor.authorNakahata, M[Nakahata, M.]-
dc.contributor.authorNakano, Y[Nakano, Y.]-
dc.contributor.authorNakayama, S[Nakayama, S.]-
dc.contributor.authorSekiya, H[Sekiya, H.]-
dc.contributor.authorShiozawa, M[Shiozawa, M.]-
dc.contributor.authorSuzuki, Y[Suzuki, Y.]-
dc.contributor.authorTakeda, A[Takeda, A.]-
dc.contributor.authorTakenaga, Y[Takenaga, Y.]-
dc.contributor.authorTomura, T[Tomura, T.]-
dc.contributor.authorUeno, K[Ueno, K.]-
dc.contributor.authorYokozawa, T[Yokozawa, T.]-
dc.contributor.authorWendell, RA[Wendell, R. A.]-
dc.contributor.authorIrvine, T[Irvine, T.]-
dc.contributor.authorKajita, T[Kajita, T.]-
dc.contributor.authorKaneyuki, K[Kaneyuki, K.]-
dc.contributor.authorLee, KP[Lee, K. P.]-
dc.contributor.authorNishimura, Y[Nishimura, Y.]-
dc.contributor.authorOkumura, K[Okumura, K.]-
dc.contributor.authorMcLachlan, T[McLachlan, T.]-
dc.contributor.authorLabarga, L[Labarga, L.]-
dc.contributor.authorBerkman, S[Berkman, S.]-
dc.contributor.authorTanaka, HA[Tanaka, H. A.]-
dc.contributor.authorTobayama, S[Tobayama, S.]-
dc.contributor.authorKearns, E[Kearns, E.]-
dc.contributor.authorRaaf, JL[Raaf, J. L.]-
dc.contributor.authorStone, JL[Stone, J. L.]-
dc.contributor.authorSulak, LR[Sulak, L. R.]-
dc.contributor.authorGoldhabar, M[Goldhabar, M.]-
dc.contributor.authorBays, K[Bays, K.]-
dc.contributor.authorCarminati, G[Carminati, G.]-
dc.contributor.authorKropp, WR[Kropp, W. R.]-
dc.contributor.authorMine, S[Mine, S.]-
dc.contributor.authorSmy, MB[Smy, M. B.]-
dc.contributor.authorSobel, HW[Sobel, H. W.]-
dc.contributor.authorGanezer, KS[Ganezer, K. S.]-
dc.contributor.authorHill, J[Hill, J.]-
dc.contributor.authorKeig, WE[Keig, W. E.]-
dc.contributor.authorHong, N[Hong, N.]-
dc.contributor.authorKim, JY[Kim, J. Y.]-
dc.contributor.authorLim, IT[Lim, I. T.]-
dc.contributor.authorAkiri, T[Akiri, T.]-
dc.contributor.authorHimmel, A[Himmel, A.]-
dc.contributor.authorScholberg, K[Scholberg, K.]-
dc.contributor.authorWalter, CW[Walter, C. W.]-
dc.contributor.authorWongjirad, T[Wongjirad, T.]-
dc.contributor.authorIshizuka, T[Ishizuka, T.]-
dc.contributor.authorTasaka, S[Tasaka, S.]-
dc.contributor.authorJang, JS[Jang, J. S.]-
dc.contributor.authorLearned, JG[Learned, J. G.]-
dc.contributor.authorMatsuno, S[Matsuno, S.]-
dc.contributor.authorSmith, SN[Smith, S. N.]-
dc.contributor.authorHasegawa, T[Hasegawa, T.]-
dc.contributor.authorIshida, T[Ishida, T.]-
dc.contributor.authorIshii, T[Ishii, T.]-
dc.contributor.authorKobayashi, T[Kobayashi, T.]-
dc.contributor.authorNakadaira, T[Nakadaira, T.]-
dc.contributor.authorNakamura, K[Nakamura, K.]-
dc.contributor.authorOyama, Y[Oyama, Y.]-
dc.contributor.authorSakashita, K[Sakashita, K.]-
dc.contributor.authorSekiguchi, T[Sekiguchi, T.]-
dc.contributor.authorTsukamoto, T[Tsukamoto, T.]-
dc.contributor.authorSuzuki, AT[Suzuki, A. T.]-
dc.contributor.authorTakeuchi, Y[Takeuchi, Y.]-
dc.contributor.authorBronner, C[Bronner, C.]-
dc.contributor.authorHirota, S[Hirota, S.]-
dc.contributor.authorHuang, K[Huang, K.]-
dc.contributor.authorIeki, K[Ieki, K.]-
dc.contributor.authorIkeda, M[Ikeda, M.]-
dc.contributor.authorKikawa, T[Kikawa, T.]-
dc.contributor.authorMinamino, A[Minamino, A.]-
dc.contributor.authorNakaya, T[Nakaya, T.]-
dc.contributor.authorSuzuki, K[Suzuki, K.]-
dc.contributor.authorTakahashi, S[Takahashi, S.]-
dc.contributor.authorFukuda, Y[Fukuda, Y.]-
dc.contributor.authorChoi, K[Choi, K.]-
dc.contributor.authorItow, Y[Itow, Y.]-
dc.contributor.authorMitsuka, G[Mitsuka, G.]-
dc.contributor.authorMijakowski, P[Mijakowski, P.]-
dc.contributor.authorHignight, J[Hignight, J.]-
dc.contributor.authorImber, J[Imber, J.]-
dc.contributor.authorJung, CK[Jung, C. K.]-
dc.contributor.authorYanagisawa, C[Yanagisawa, C.]-
dc.contributor.authorIshino, H[Ishino, H.]-
dc.contributor.authorKibayashi, A[Kibayashi, A.]-
dc.contributor.authorKoshio, Y[Koshio, Y.]-
dc.contributor.authorMori, T[Mori, T.]-
dc.contributor.authorSakuda, M[Sakuda, M.]-
dc.contributor.authorYano, T[Yano, T.]-
dc.contributor.authorKuno, Y[Kuno, Y.]-
dc.contributor.authorTacik, R[Tacik, R.]-
dc.contributor.authorKim, SB[Kim, S. B.]-
dc.contributor.authorOkazawa, H[Okazawa, H.]-
dc.contributor.authorChoi, Y[Choi, Y.]-
dc.contributor.authorNishijima, K[Nishijima, K.]-
dc.contributor.authorKoshiba, M[Koshiba, M.]-
dc.contributor.authorTotsuka, Y[Totsuka, Y.]-
dc.contributor.authorYokoyama, M[Yokoyama, M.]-
dc.contributor.authorMartens, K[Martens, K.]-
dc.contributor.authorMarti, L[Marti, Ll.]-
dc.contributor.authorVagins, MR[Vagins, M. R.]-
dc.contributor.authorMartin, JF[Martin, J. F.]-
dc.contributor.authorde Perio, P[de Perio, P.]-
dc.contributor.authorKonaka, A[Konaka, A.]-
dc.contributor.authorWilking, MJ[Wilking, M. J.]-
dc.contributor.authorChen, S[Chen, S.]-
dc.contributor.authorZhang, Y[Zhang, Y.]-
dc.contributor.authorWilkes, RJ[Wilkes, R. J.]-
dc.date.accessioned2021-08-03T17:50:23Z-
dc.date.available2021-08-03T17:50:23Z-
dc.date.created2016-08-07-
dc.date.issued2014-03-07-
dc.identifier.issn0031-9007-
dc.identifier.urihttps://scholarworks.bwise.kr/skku/handle/2021.sw.skku/53675-
dc.description.abstractWe report an indication that the elastic scattering rate of solar B-8 neutrinos with electrons in the Super-Kamiokande detector is larger when the neutrinos pass through Earth during nighttime. We determine the day-night asymmetry, defined as the difference of the average day rate and average night rate divided by the average of those two rates, to be [-3.2 +/- 1.1(stat) +/- 0.5(syst)]%, which deviates from zero by 2.7 sigma. Since the elastic scattering process is mostly sensitive to electron-flavored solar neutrinos, a nonzero day-night asymmetry implies that the flavor oscillations of solar neutrinos are affected by the presence of matter within the neutrinos' flight path. Super-Kamiokande's day-night asymmetry is consistent with neutrino oscillations for 4 x 10(-5) eV(2) <= Delta m(21)(2) <= 7 x 10(-5) eV(2) and large mixing values of theta(12), at the 68% C.L.-
dc.publisherAMER PHYSICAL SOC-
dc.subjectMODEL-
dc.titleFirst Indication of Terrestrial Matter Effects on Solar Neutrino Oscillation-
dc.typeArticle-
dc.contributor.affiliatedAuthorChoi, Y[Choi, Y.]-
dc.identifier.doi10.1103/PhysRevLett.112.091805-
dc.identifier.scopusid2-s2.0-84896368473-
dc.identifier.wosid000332688400001-
dc.identifier.bibliographicCitationPHYSICAL REVIEW LETTERS, v.112, no.9-
dc.relation.isPartOfPHYSICAL REVIEW LETTERS-
dc.citation.titlePHYSICAL REVIEW LETTERS-
dc.citation.volume112-
dc.citation.number9-
dc.type.rimsART-
dc.description.journalClass1-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
Files in This Item
There are no files associated with this item.
Appears in
Collections
Science > Department of Physics > 1. Journal Articles
Show simple item record

qrcode

Items in ScholarWorks are protected by copyright, with all rights reserved, unless otherwise indicated.

Altmetrics

Total Views & Downloads

STATISTICS
Total View :5,592,390
Today View :2,234

RSS_1.0 RSS_2.0 ATOM_1.0

CONTACT US

(03063) 25-2, SUNGKYUNKWAN-RO, JONGNO-GU, SEOUL, KOREAsamsunglib@skku.edu

COPYRIGHT © 2021 SUNGKYUNKWAN UNIVERSITY ALL RIGHTS RESERVED.

Certain data included herein are derived from the © Web of Science of Clarivate Analytics. All rights reserved.
You may not copy or re-distribute this material in whole or in part without the prior written consent of Clarivate Analytics.

BROWSE

한국어