First Constraints on the Complete Neutrino Mixing Matrix with a Sterile Neutrino
arXiv:1607.00011 · doi:10.1103/PhysRevLett.117.221801
Abstract
Neutrino oscillation models involving one extra mass eigenstate beyond the standard three () are fit to global short baseline experimental data and the recent IceCube disappearance search result. We find a best fit of with (dof) of 50.61 (4). We find that the combined IceCube and short baseline data constrain to at 90\% C.L. for , which is improved over present limits. Incorporating the IceCube information provides the first constraints on all entries of the 3+1 mixing matrix.
7 pages, 4 figures
References in corpus (10)
- The Reactor Antineutrino Anomaly
- Measurement of the solar neutrino capture rate with gallium metal. III: Results for the 2002--2007 data-taking period
- Updated fit to three neutrino mixing: status of leptonic CP violation
- Physics Reach of High-Energy and High-Statistics IceCube Atmospheric Neutrino Data
- Improved Search for a Light Sterile Neutrino with the Full Configuration of the Daya Bay Experiment
- Search for Sterile Neutrinos Mixing with Muon Neutrinos in MINOS
- Dual baseline search for muon antineutrino disappearance at 0.1 eV^2 < Δm^2 < 100 eV^2
- Sterile neutrinos, lepton asymmetries, primordial elements: how much of each?
- Signature of sterile species in atmospheric neutrino data at neutrino telescopes
- Searches for sterile neutrinos with IceCube DeepCore
Cited by in corpus (7)
- Sterile Neutrinos or Flux Uncertainties? - Status of the Reactor Anti-Neutrino Anomaly
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- Neutrinos in Large Extra Dimensions and Short-Baseline Appearance
- A Combined View of Sterile-Neutrino Constraints from CMB and Neutrino Oscillation Measurements
- Joint short- and long-baseline constraints on light sterile neutrinos
- What measurements of neutrino neutral current events can reveal
- Dark matter, supernova neutrinos and other backgrounds in direct dark matter searches. The ANDES laboratory prospects