Abstract
The Daya Bay Reactor Neutrino Experiment was designed to achieve a sensitivity on the value of sin22θ13 to better than 0.01 at 90% CL. The experiment consists of eight antineutrino detectors installed underground at different baselines from six nuclear reactors. With data collected with six antineutrino detectors for 55 days, Daya Bay announced the discovery of a non-zero value for sin22θ13 with a significance of 5.2 standard deviations in March 2012. The most recent analysis with 139 days of data acquired in a six-detector configuration yields sin22θ13=0.089±0.010(stat.)±0.005(syst.), which is the most precise measurement of sin22θ13 to date.
Original language | English (US) |
---|---|
Pages (from-to) | 18-22 |
Number of pages | 5 |
Journal | Nuclear Physics B - Proceedings Supplements |
Volume | 246-247 |
DOIs | |
State | Published - Jan 2014 |
All Science Journal Classification (ASJC) codes
- Atomic and Molecular Physics, and Optics
- Nuclear and High Energy Physics
Keywords
- Daya Bay
- Neutrino Mixing
- Neutrino Oscillation
- Reactor
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In: Nuclear Physics B - Proceedings Supplements, Vol. 246-247, 01.2014, p. 18-22.
Research output: Contribution to journal › Article › peer-review
TY - JOUR
T1 - Results from the daya bay reactor neutrino experiment
AU - Tsang, K. V.
AU - An, F. P.
AU - An, Q.
AU - Bai, J. Z.
AU - Balantekin, A. B.
AU - Band, H. R.
AU - Beriguete, W.
AU - Bishai, M.
AU - Blyth, S.
AU - Brown, R. L.
AU - Cao, G. F.
AU - Cao, J.
AU - Carr, R.
AU - Chan, W. T.
AU - Chang, J. F.
AU - Chang, Y.
AU - Chasman, C.
AU - Chen, H. S.
AU - Chen, H. Y.
AU - Chen, S. J.
AU - Chen, S. M.
AU - Chen, X. C.
AU - Chen, X. H.
AU - Chen, X. S.
AU - Chen, Y.
AU - Chen, Y. X.
AU - Cherwinka, J. J.
AU - Chu, M. C.
AU - Cummings, J. P.
AU - Deng, Z. Y.
AU - Ding, Y. Y.
AU - Diwan, M. V.
AU - Draeger, E.
AU - Du, X. F.
AU - Dwyer, D.
AU - Edwards, W. R.
AU - Ely, S. R.
AU - Fang, S. D.
AU - Fu, J. Y.
AU - Fu, Z. W.
AU - Ge, L. Q.
AU - Gill, R. L.
AU - Gonchar, M.
AU - Gong, G. H.
AU - Gong, H.
AU - Gornushkin, Y. A.
AU - Gu, W. Q.
AU - Guan, M. Y.
AU - Guo, X. H.
AU - Hackenburg, R. W.
AU - Hahn, R. L.
AU - Hans, S.
AU - Hao, H. F.
AU - He, M.
AU - He, Q.
AU - Heeger, K. M.
AU - Heng, Y. K.
AU - Hinrichs, P.
AU - Hor, Y. K.
AU - Hsiung, Y. B.
AU - Hu, B. Z.
AU - Hu, T.
AU - Huang, H. X.
AU - Huang, H. Z.
AU - Huang, X. T.
AU - Huber, P.
AU - Issakov, V.
AU - Isvan, Z.
AU - Jaffe, D. E.
AU - Jetter, S.
AU - Ji, X. L.
AU - Ji, X. P.
AU - Jiang, H. J.
AU - Jiao, J. B.
AU - Johnson, R. A.
AU - Kang, L.
AU - Kettell, S. H.
AU - Kramer, M.
AU - Kwan, K. K.
AU - Kwok, M. W.
AU - Kwok, T.
AU - Lai, C. Y.
AU - Lai, W. C.
AU - Lai, W. H.
AU - Lau, K.
AU - Lebanowski, L.
AU - Lee, J.
AU - Lei, R. T.
AU - Leitner, R.
AU - Leung, J. K.C.
AU - Leung, K. Y.
AU - Lewis, C. A.
AU - Li, F.
AU - Li, G. S.
AU - Li, Q. J.
AU - Li, W. D.
AU - Li, X. B.
AU - Li, X. N.
AU - Li, X. Q.
AU - Li, Y.
AU - Li, Z. B.
AU - Liang, H.
AU - Lin, C. J.
AU - Lin, G. L.
AU - Lin, S. K.
AU - Lin, Y. C.
AU - Ling, J. J.
AU - Link, J. M.
AU - Littenberg, L.
AU - Littlejohn, B. R.
AU - Liu, D. W.
AU - Liu, J. C.
AU - Liu, J. L.
AU - Liu, Y. B.
AU - Lu, C.
AU - Lu, H. Q.
AU - Luk, A.
AU - Luk, K. B.
AU - Ma, Q. M.
AU - Ma, X. B.
AU - Ma, X. Y.
AU - Ma, Y. Q.
AU - McDonald, K. T.
AU - McFarlane, M. C.
AU - McKeown, R. D.
AU - Meng, Y.
AU - Mohapatra, D.
AU - Nakajima, Y.
AU - Napolitano, J.
AU - Naumov, D.
AU - Nemchenok, I.
AU - Ngai, H. Y.
AU - Ngai, W. K.
AU - Nie, Y. B.
AU - Ning, Z.
AU - Ochoa-Ricoux, J. P.
AU - Olshevski, A.
AU - Patton, S.
AU - Pec, V.
AU - Peng, J. C.
AU - Piilonen, L. E.
AU - Pinsky, L.
AU - Pun, C. S.J.
AU - Qi, F. Z.
AU - Qi, M.
AU - Qian, X.
AU - Raper, N.
AU - Ren, J.
AU - Rosero, R.
AU - Roskovec, B.
AU - Ruan, X. C.
AU - Shao, B. B.
AU - Shih, K.
AU - Steiner, H.
AU - Sun, G. X.
AU - Sun, J. L.
AU - Tagg, N.
AU - Tam, Y. H.
AU - Tanaka, H. K.
AU - Tang, X.
AU - Themann, H.
AU - Torun, Y.
AU - Trentalange, S.
AU - Tsai, O.
AU - Tsang, R. H.M.
AU - Tull, C. E.
AU - Tung, Y. C.
AU - Viren, B.
AU - Vorobel, V.
AU - Wang, C. H.
AU - Wang, L. S.
AU - Wang, L. Y.
AU - Wang, L. Z.
AU - Wang, M.
AU - Wang, N. Y.
AU - Wang, R. G.
AU - Wang, W.
AU - Wang, X.
AU - Wang, Y. F.
AU - Wang, Z.
AU - Wang, Z.
AU - Wang, Z. M.
AU - Webber, D. M.
AU - Wei, H. Y.
AU - Wei, Y. D.
AU - Wen, L. J.
AU - Whisnant, K.
AU - White, C. G.
AU - Whitehead, L.
AU - Williamson, Y.
AU - Wise, T.
AU - Wong, H. L.H.
AU - Worcester, E. T.
AU - Wu, F. F.
AU - Wu, Q.
AU - Xi, J. B.
AU - Xia, D. M.
AU - Xing, Z. Z.
AU - Xu, J.
AU - Xu, J.
AU - Xu, J. L.
AU - Xu, Y.
AU - Xue, T.
AU - Yang, C. G.
AU - Yang, L.
AU - Ye, M.
AU - Yeh, M.
AU - Yeh, Y. S.
AU - Young, B. L.
AU - Yu, Z. Y.
AU - Zhan, L.
AU - Zhang, C.
AU - Zhang, F. H.
AU - Zhang, J. W.
AU - Zhang, Q. M.
AU - Zhang, S. H.
AU - Zhang, Y. C.
AU - Zhang, Y. H.
AU - Zhang, Y. X.
AU - Zhang, Z. J.
AU - Zhang, Z. P.
AU - Zhang, Z. Y.
AU - Zhao, J.
AU - Zhao, Q. W.
AU - Zhao, Y. B.
AU - Zheng, L.
AU - Zhong, W. L.
AU - Zhou, L.
AU - Zhou, Z. Y.
AU - Zhuang, H. L.
AU - Zou, J. H.
N1 - Funding Information: aLawrence Berkeley National Laboratory, Berkeley, CA bInstitute of High Energy Physics, Beijing cUniversity of Science and Technology of China, Hefei dUniversity of Wisconsin, Madison, WI eBrookhaven National Laboratory, Upton, NY fNational United University, Miao-Li gCalifornia Institute of Technology, Pasadena, CA hInstitute of Physics, National Chiao-Tung University, Hsinchu iNanjing University, Nanjing jDepartment of Engineering Physics, Tsinghua University, Beijing kChinese University of Hong Kong, Hong Kong lShenzhen Univeristy, Shen Zhen mNorth China Electric Power University, Beijing nSiena College, Loudonville, NY oDepartment of Physics, Illinois Institute of Technology, Chicago, IL pDepartment of Physics, University of California, Berkeley, CA qDepartment of Physics, University of Illinois at Urbana-Champaign, Urbana, IL rChengdu University of Technology, Chengdu Funding Information: sJoint Institute for Nuclear Research, Dubna, Moscow Region tShanghai Jiao Tong University, Shanghai uBeijing Normal University, Beijing vJoseph Henry Laboratories, Princeton University, Princeton, NJ wCenter for Neutrino Physics, Virginia Tech, Blacksburg, VA xDepartment of Physics, National Taiwan University, Taipei yChina Institute of Atomic Energy, Beijing zUniversity of California, Los Angeles, CA aaShandong University, Jinan abSchool of Physics, Nankai University, Tianjin acUniversity of Cincinnati, Cincinnati, OH adDongguan University of Technology, Dongguan aeDepartment of Physics, The University of Hong Kong, Pokfulam, Hong Kong afDepartment of Physics, University of Houston, Houston, TX agCharles University, Faculty of Mathematics and Physics, Prague ahSun Yat-Sen (Zhongshan) University, Guangzhou aiCollege of William and Mary, Williamsburg, VA ajRensselaer Polytechnic Institute, Troy, NY akChina Guangdong Nuclear Power Group, Shenzhen alIowa State University, Ames, IA amXi’an Jiaotong University, Xi’an
PY - 2014/1
Y1 - 2014/1
N2 - The Daya Bay Reactor Neutrino Experiment was designed to achieve a sensitivity on the value of sin22θ13 to better than 0.01 at 90% CL. The experiment consists of eight antineutrino detectors installed underground at different baselines from six nuclear reactors. With data collected with six antineutrino detectors for 55 days, Daya Bay announced the discovery of a non-zero value for sin22θ13 with a significance of 5.2 standard deviations in March 2012. The most recent analysis with 139 days of data acquired in a six-detector configuration yields sin22θ13=0.089±0.010(stat.)±0.005(syst.), which is the most precise measurement of sin22θ13 to date.
AB - The Daya Bay Reactor Neutrino Experiment was designed to achieve a sensitivity on the value of sin22θ13 to better than 0.01 at 90% CL. The experiment consists of eight antineutrino detectors installed underground at different baselines from six nuclear reactors. With data collected with six antineutrino detectors for 55 days, Daya Bay announced the discovery of a non-zero value for sin22θ13 with a significance of 5.2 standard deviations in March 2012. The most recent analysis with 139 days of data acquired in a six-detector configuration yields sin22θ13=0.089±0.010(stat.)±0.005(syst.), which is the most precise measurement of sin22θ13 to date.
KW - Daya Bay
KW - Neutrino Mixing
KW - Neutrino Oscillation
KW - Reactor
UR - http://www.scopus.com/inward/record.url?scp=84891956113&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84891956113&partnerID=8YFLogxK
U2 - 10.1016/j.nuclphysbps.2013.10.059
DO - 10.1016/j.nuclphysbps.2013.10.059
M3 - Article
AN - SCOPUS:84891956113
SN - 0920-5632
VL - 246-247
SP - 18
EP - 22
JO - Nuclear Physics B - Proceedings Supplements
JF - Nuclear Physics B - Proceedings Supplements
ER -