- Main
Measurement of electron antineutrino oscillation based on 1230 days of operation of the Daya Bay experiment
- An, FP;
- Balantekin, AB;
- Band, HR;
- Bishai, M;
- Blyth, S;
- Cao, D;
- Cao, GF;
- Cao, J;
- Cen, WR;
- Chan, YL;
- Chang, JF;
- Chang, LC;
- Chang, Y;
- Chen, HS;
- Chen, QY;
- Chen, SM;
- Chen, YX;
- Chen, Y;
- Cheng, J-H;
- Cheng, J;
- Cheng, YP;
- Cheng, ZK;
- Cherwinka, JJ;
- Chu, MC;
- Chukanov, A;
- Cummings, JP;
- de Arcos, J;
- Deng, ZY;
- Ding, XF;
- Ding, YY;
- Diwan, MV;
- Dolgareva, M;
- Dove, J;
- Dwyer, DA;
- Edwards, WR;
- Gill, R;
- Gonchar, M;
- Gong, GH;
- Gong, H;
- Grassi, M;
- Gu, WQ;
- Guan, MY;
- Guo, L;
- Guo, XH;
- Guo, YH;
- Guo, Z;
- Hackenburg, RW;
- Han, R;
- Hans, S;
- He, M;
- Heeger, KM;
- Heng, YK;
- Higuera, A;
- Hor, YK;
- Hsiung, YB;
- Hu, BZ;
- Hu, T;
- Hu, W;
- Huang, EC;
- Huang, HX;
- Huang, XT;
- Huber, P;
- Huo, W;
- Hussain, G;
- Jaffe, DE;
- Jaffke, P;
- Jen, KL;
- Jetter, S;
- Ji, XP;
- Ji, XL;
- Jiao, JB;
- Johnson, RA;
- Jones, D;
- Joshi, J;
- Kang, L;
- Kettell, SH;
- Kohn, S;
- Kramer, M;
- Kwan, KK;
- Kwok, MW;
- Kwok, T;
- Langford, TJ;
- Lau, K;
- Lebanowski, L;
- Lee, J;
- Lee, JHC;
- Lei, RT;
- Leitner, R;
- Leung, JKC;
- Li, C;
- Li, DJ;
- Li, F;
- Li, GS;
- Li, QJ;
- Li, S;
- Li, SC;
- Li, WD;
- Li, XN;
- Li, YF;
- Li, ZB;
- Liang, H;
- Lin, CJ;
- Lin, GL;
- Lin, S;
- Lin, SK;
- Lin, Y-C;
- Ling, JJ;
- Link, JM;
- Littenberg, L;
- Littlejohn, BR;
- Liu, DW;
- Liu, JL;
- Liu, JC;
- Loh, CW;
- Lu, C;
- Lu, HQ;
- Lu, JS;
- Luk, KB;
- Lv, Z;
- M., Q;
- Y., X;
- B., X;
- Q., Y;
- Malyshkin, Y;
- Caicedo, DA Martinez;
- McDonald, KT;
- McKeown, RD;
- Mitchell, I;
- Mooney, M;
- Nakajima, Y;
- Napolitano, J;
- Naumov, D;
- Naumova, E;
- Ngai, HY;
- Ning, Z;
- Ochoa-Ricoux, JP;
- Olshevskiy, A;
- Pan, H-R;
- Park, J;
- Patton, S;
- Pec, V;
- Peng, JC;
- Pinsky, L;
- Pun, CSJ;
- Qi, FZ;
- Qi, M;
- Qian, X;
- Raper, N;
- Ren, J;
- Rosero, R;
- Roskovec, B;
- Ruan, XC;
- Steiner, H;
- Sun, GX;
- Sun, JL;
- Tang, W;
- Taychenachev, D;
- Treskov, K;
- Tsang, KV;
- Tull, CE;
- Viaux, N;
- Viren, B;
- Vorobel, V;
- Wang, CH;
- Wang, M;
- Wang, NY;
- Wang, RG;
- Wang, W;
- Wang, X;
- Wang, YF;
- Wang, Z;
- Wang, Z;
- Wang, ZM;
- Wei, HY;
- Wen, LJ;
- Whisnant, K;
- White, CG;
- Whitehead, L;
- Wise, T;
- Wong, HLH;
- Wong, SCF;
- Worcester, E;
- Wu, C-H;
- Wu, Q;
- Wu, WJ;
- Xia, DM;
- Xia, JK;
- Xing, ZZ;
- Xu, JY;
- Xu, JL;
- Xu, Y;
- Xue, T;
- Yang, CG;
- Yang, H;
- Yang, L;
- Yang, MS;
- Yang, MT;
- Ye, M;
- Ye, Z;
- Yeh, M;
- Young, BL;
- Yu, ZY;
- Zeng, S;
- Zhan, L;
- Zhang, C;
- Zhang, HH;
- Zhang, JW;
- Zhang, QM;
- Zhang, XT;
- Zhang, YM;
- Zhang, YX;
- Zhang, YM;
- Zhang, ZJ;
- Zhang, ZY;
- Zhang, ZP;
- Zhao, J;
- Zhao, QW;
- Zhao, YB;
- Zhong, WL;
- Zhou, L;
- Zhou, N;
- Zhuang, HL;
- Zou, JH
Published Web Location
https://doi.org/10.1103/physrevd.95.072006Abstract
A measurement of electron antineutrino oscillation by the Daya Bay Reactor Neutrino Experiment is described in detail. Six 2.9-GWth nuclear power reactors of the Daya Bay and Ling Ao nuclear power facilities served as intense sources of ν¯e’s. Comparison of the ν¯e rate and energy spectrum measured by antineutrino detectors far from the nuclear reactors (∼1500–1950 m) relative to detectors near the reactors (∼350–600 m) allowed a precise measurement of ν¯e disappearance. More than 2.5 million ν¯e inverse beta-decay interactions were observed, based on the combination of 217 days of operation of six antineutrino detectors (December, 2011–July, 2012) with a subsequent 1013 days using the complete configuration of eight detectors (October, 2012–July, 2015). The ν¯e rate observed at the far detectors relative to the near detectors showed a significant deficit, R=0.949±0.002(stat)±0.002(syst). The energy dependence of ν¯e disappearance showed the distinct variation predicted by neutrino oscillation. Analysis using an approximation for the three-flavor oscillation probability yielded the flavor-mixing angle sin22θ13=0.0841±0.0027(stat)±0.0019(syst) and the effective neutrino mass-squared difference of |Δmee2|=(2.50±0.06(stat)±0.06(syst))×10-3 eV2. Analysis using the exact three-flavor probability found Δm322=(2.45±0.06(stat)±0.06(syst))×10-3 eV2 assuming the normal neutrino mass hierarchy and Δm322=(-2.56±0.06(stat)±0.06(syst))×10-3 eV2 for the inverted hierarchy.
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