18 research outputs found
Precision measurement of reactor antineutrino oscillation at kilometer-scale baselines by Daya Bay
We present a new determination of the smallest neutrino mixing angle
and the mass-squared difference
using a final sample of inverse beta-decay (IBD)
candidates with the final-state neutron captured on gadolinium. This sample was
selected from the complete data set obtained by the Daya Bay reactor neutrino
experiment in 3158 days of operation. Compared to the previous Daya Bay
results, selection of IBD candidates has been optimized, energy calibration
refined, and treatment of backgrounds further improved. The resulting
oscillation parameters are ,
for
the normal mass ordering or for the inverted mass ordering.Comment: 7 pages, 3 figures, 1 table, 10 supplementary file
Improved constraints on sterile neutrino mixing from disappearance searches in the MINOS, MINOS+, Daya Bay, and Bugey-3 experiments
Searches for electron antineutrino, muon neutrino, and muon antineutrino disappearance driven by sterile neutrino mixing have been carried out by the Daya Bay and MINOS+ collaborations. This Letter presents the combined results of these searches, along with exclusion results from the Bugey-3 reactor experiment, framed in a minimally extended four-neutrino scenario. Significantly improved constraints on the θμe mixing angle are derived that constitute the most constraining limits to date over five orders of magnitude in the mass-squared splitting Δm412, excluding the 90% C.L. sterile-neutrino parameter space allowed by the LSND and MiniBooNE observations at 90% CLs for Δm412<13 eV2. Furthermore, the LSND and MiniBooNE 99% C.L. allowed regions are excluded at 99% CLs for Δm412<1.6 eV2
First measurement of high-energy reactor antineutrinos at Daya Bay
This Letter reports the first measurement of high-energy reactor
antineutrinos at Daya Bay, with nearly 9000 inverse beta decay candidates in
the prompt energy region of 8-12~MeV observed over 1958 days of data
collection. A multivariate analysis is used to separate 2500 signal events from
background statistically. The hypothesis of no reactor antineutrinos with
neutrino energy above 10~MeV is rejected with a significance of 6.2 standard
deviations. A 29\% antineutrino flux deficit in the prompt energy region of
8-11~MeV is observed compared to a recent model prediction. We provide the
unfolded antineutrino spectrum above 7 MeV as a data-based reference for other
experiments. This result provides the first direct observation of the
production of antineutrinos from several high- isotopes in
commercial reactors.Comment: 7 pages, 4 figures, accepted by Physical Review Letter
Improved Measurement of the Evolution of the Reactor Antineutrino Flux and Spectrum at Daya Bay
International audienceReactor neutrino experiments play a crucial role in advancing our knowledge of neutrinos. In this Letter, the evolution of the flux and spectrum as a function of the reactor isotopic content is reported in terms of the inverse-beta-decay yield at Daya Bay with 1958Â days of data and improved systematic uncertainties. These measurements are compared with two signature model predictions: the Huber-Mueller model based on the conversion method and the SM2018 model based on the summation method. The measured average flux and spectrum, as well as the flux evolution with the Pu239 isotopic fraction, are inconsistent with the predictions of the Huber-Mueller model. In contrast, the SM2018 model is shown to agree with the average flux and its evolution but fails to describe the energy spectrum. Altering the predicted inverse-beta-decay spectrum from Pu239 fission does not improve the agreement with the measurement for either model. The models can be brought into better agreement with the measurements if either the predicted spectrum due to U235 fission is changed or the predicted U235, U238, Pu239, and Pu241 spectra are changed in equal measure
Precision Measurement of Reactor Antineutrino Oscillation at Kilometer-Scale Baselines by Daya Bay
We present a new determination of the smallest neutrino mixing angle θ13 and the mass-squared difference Δm322 using a final sample of 5.55×106 inverse beta-decay (IBD) candidates with the final-state neutron captured on gadolinium. This sample is selected from the complete dataset obtained by the Daya Bay reactor neutrino experiment in 3158 days of operation. Compared to the previous Daya Bay results, selection of IBD candidates has been optimized, energy calibration refined, and treatment of backgrounds further improved. The resulting oscillation parameters are sin22θ13=0.0851±0.0024, Δm322=(2.466±0.060)×10-3  eV2 for the normal mass ordering or Δm322=-(2.571±0.060)×10-3  eV2 for the inverted mass ordering.We present a new determination of the smallest neutrino mixing angle and the mass-squared difference using a final sample of inverse beta-decay (IBD) candidates with the final-state neutron captured on gadolinium. This sample was selected from the complete data set obtained by the Daya Bay reactor neutrino experiment in 3158 days of operation. Compared to the previous Daya Bay results, selection of IBD candidates has been optimized, energy calibration refined, and treatment of backgrounds further improved. The resulting oscillation parameters are , for the normal mass ordering or for the inverted mass ordering
Improved Constraints on Sterile Neutrino Mixing from Disappearance Searches in the MINOS, MINOS+, Daya Bay, and Bugey-3 Experiments
Searches for electron antineutrino, muon neutrino, and muon antineutrino disappearance driven by sterile neutrino mixing have been carried out by the Daya Bay and MINOSþ collaborations. This Letter presents the combined results of these searches, along with exclusion results from the Bugey-3 reactor experiment, framed in a minimally extended four-neutrino scenario. Significantly improved constraints on the θμe mixing angle are derived that constitute the most constraining limits to date over five orders of magnitude in the mass-squared splitting Δm2 41, excluding the 90% C.L. sterile-neutrino parameter space allowed by the LSND and MiniBooNE observations at 90% CLs for Δm2 41 < 13 eV2. Furthermore, the LSND and MiniBooNE 99% C.L. allowed regions are excluded at 99% CLs for Δm2 41 < 1.6 eV2