Diagnosing the Reactor Antineutrino Anomaly with Global Antineutrino Flux Data
arXiv:1901.01807 · doi:10.1103/PhysRevD.99.073005
Abstract
We have examined the impact of new Daya Bay, Double Chooz, and RENO measurements on global fits of reactor antineutrino flux data to a variety of hypotheses regarding the origin of the reactor antineutrino anomaly. In comparing RENO and Daya Bay measurements of inverse beta decay (IBD) yield versus Pu fission fraction, we find differing levels of precision in measurements of time-integrated yield and yield slope, but similar central values, leading to modestly enhanced isotopic IBD yield measurements in a joint fit of the two datasets. In the absence of sterile neutrino oscillations, global fits to all measurements now provide 3σ preference for incorrect modeling of specific fission isotopes over common mis-modeling of all beta-converted isotopes. If sterile neutrino oscillations are considered, global IBD yield fits provide no substantial preference between oscillation-including and oscillation-excluding hypotheses: hybrid models containing both sterile neutrino oscillations and incorrect U or Pu flux predictions are favored at only 1-2σ with respect to models where U, U, and Pu are assumed to be incorrectly predicted.
7 pages, 4 figures, 3 tables
References in corpus (11)
- The Reactor Antineutrino Anomaly
- Sterile neutrino search at NEOS Experiment
- Light Sterile Neutrinos: Models and Phenomenology
- Spectral Structure of Electron Antineutrinos from Nuclear Reactors
- Sterile Neutrinos or Flux Uncertainties? - Status of the Reactor Anti-Neutrino Anomaly
- Imprints of CP violation induced by sterile neutrinos in T2K data
- Reactor Fuel Fraction Information on the Antineutrino Anomaly
- Precise Determination of the U-235 Reactor Antineutrino Cross Section per Fission
- Prospects for Improved Understanding of Isotopic Reactor Antineutrino Fluxes
- Nuclear Zemach Moments and Finite-Size Corrections to Allowed Beta Decay
- CP-Invariance Violation at Short-Baseline Experiments in 3+1 Neutrino Scenarios