DAEMONFLUX: DAta-drivEn MuOn-calibrated atmospheric Neutrino Flux
arXiv:2303.00022 · doi:10.1103/PhysRevD.107.123037
Abstract
In this paper, we present a refined calculation of the atmospheric neutrino flux spanning from GeV to PeV energies. Our method, Daemonflux, utilizes data-driven inputs and incorporates adjustable parameters to take their uncertainties into account. By optimizing these parameters using a combination of muon data and constraints from fixed-target experiments, we achieve uncertainties in the calculated neutrino fluxes of less than 10% up to 1 TeV, with neutrino ratios constrained to below 10%. Our model performs particularly well at energies below 100 GeV, where the smallest errors are obtained. We make our model available as a software package that provides access to predictions of fluxes, ratios, and errors, including the covariance matrix obtained from the fit.
21 pages, 23 figures
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- A search for an eV-scale sterile neutrino using improved high-energy event reconstruction in IceCube
- Evidence for a Spectral Break or Curvature in the Spectrum of Astrophysical Neutrinos from 5 TeV--10 PeV
- Sibyll
- Improved measurements of the TeV-PeV extragalactic neutrino spectrum from joint analyses of IceCube tracks and cascades
- Cosmic Ray Muons in Laboratories Deep Underground
- Methods and stability tests associated with the sterile neutrino search using improved high-energy event reconstruction in IceCube
- Constraints on non-unitary neutrino mixing in light of atmospheric and reactor neutrino data
- Beyond first light: Global monitoring for high-energy neutrino astronomy
- Measurement of the mean number of muons with energies above 500 GeV in air showers detected with the IceCube Neutrino Observatory
- Cosmogenic Muon Background Characterization for the Colorado Underground Research Institute (CURIE)
- Seasonal Variations of the Atmospheric Muon Neutrino Spectrum measured with IceCube
- Measurement of the inelasticity distribution of neutrino-nucleon interactions for with IceCube DeepCore