The Smallness of Matter Effects in Long-Baseline Muon Neutrino Disappearance
arXiv:2401.10326 · doi:10.1103/PhysRevD.109.053002
Abstract
Current long-baseline accelerator experiments, NOvA and T2K, are making excellent measurements of neutrino oscillations and the next generation of experiments, DUNE and HK, will make measurements at the level of precision. These measurements are a combination of the appearance channel which is more challenging experimentally but depends on many oscillation parameters, and the disappearance channel which is somewhat easier and allows for precision measurements of the atmospheric mass splitting and the atmospheric mixing angle. It is widely recognized that the matter effect plays a key role in the appearance probability, yet the effect on the disappearance probability is surprisingly small for these experiments. Here we investigate both exactly how small the effect is and show that it just begins to become relevant in the high statistics regime of DUNE.
arXiv comment9 pages, 6 figures, 1 table, comments welcome! v2: appendix added, matches published version
References in corpus (17)
- Golden measurements at a neutrino factory
- Analytic Approximations for Three Neutrino Oscillation Parameters and Probabilities in Matter
- Series expansions for three-flavor neutrino oscillation probabilities in matter
- Another possible way to determine the Neutrino Mass Hierarchy
- Compact Perturbative Expressions For Neutrino Oscillations in Matter
- Large-Theta(13) Perturbation Theory of Neutrino Oscillation for Long-Baseline Experiments
- Two modes of searching for new neutrino interactions at MINOS
- Simple and Compact Expressions for Neutrino Oscillation Probabilities in Matter
- Analytical Approximation of the Neutrino Oscillation Matter Effects at large
- Large Matter Effects in Oscillations
- Neutrino oscillation probabilities through the looking glass
- Eigenvalues: the Rosetta Stone for Neutrino Oscillations in Matter
- Matter Density Profile Shape Effects at DUNE
- Rotations Versus Perturbative Expansions for Calculating Neutrino Oscillation Probabilities in Matter
- The Impact of Different Parameterizations on the Interpretation of CP Violation in Neutrino Oscillations
- Here Comes the Sun: Solar Parameters in Long-Baseline Accelerator Neutrino Oscillations
- An Effective Two-Flavor Approximation for Neutrino Survival Probabilities in Matter