Measurement of Atmospheric Neutrino Mixing with Improved IceCube DeepCore Calibration and Data Processing
Physics - Instrumentation and Detectors
Neutrino: flavor
neutrino: flux
Physics, Particles & Fields
High Energy Physics - Experiment
IceCube
Subatomär fysik
High Energy Physics - Experiment (hep-ex)
Astronomi, astrofysik och kosmologi
neutrino: atmosphere
Subatomic Physics
Neutrino: mixing angle: measured
Astronomy, Astrophysics and Cosmology
info:eu-repo/classification/ddc/530
physics.ins-det
Physics
ddc:530
Instrumentation and Detectors (physics.ins-det)
mass difference: measured
STATISTICS
INVARIANCE
Neutrino: atmosphere
Calibration
Physical Sciences
neutrino: flavor
Neutrino: oscillation
numerical calculations: Monte Carlo
BEHAVIOR
neutrino: mixing angle: measured
accelerator
neutrino: mass difference
Accelerator
FOS: Physical sciences
ISING-MODEL
Astronomy & Astrophysics
530
info:eu-repo/classification/ddc/500.2
neutrino: energy
Experimental results
Science & Technology
hep-ex
Numerical calculations: Monte Carlo
Neutrino: mixing
Neutrino: flux
calibration
Neutrino: mass difference
Physics and Astronomy
13. Climate action
neutrino: oscillation
Mass difference: measured
neutrino: mixing
Neutrino: energy
GAUGE-THEORY
experimental results
DOI:
10.48550/arxiv.2304.12236
Publication Date:
2023-07-20
AUTHORS (225)
ABSTRACT
Published by Inst., Woodbury, NY<br/>Physical review / D 108(1), 012014 (2023). doi:10.1103/PhysRevD.108.012014<br/>We describe a new data sample of IceCube DeepCore and report on the latest measurement of atmospheric neutrino oscillations obtained with data recorded between 2011–2019. The sample includes significant improvements in data calibration, detector simulation, and data processing, and the analysis benefits from a sophisticated treatment of systematic uncertainties, with significantly greater level of detail since our last study. By measuring the relative fluxes of neutrino flavors as a function of their reconstructed energies and arrival directions we constrain the atmospheric neutrino mixing parameters to be sin2θ23=0.51±0.05 and Δm322=2.41±0.07×10-3 eV2, assuming a normal mass ordering. The errors include both statistical and systematic uncertainties. The resulting 40% reduction in the error of both parameters with respect to our previous result makes this the most precise measurement of oscillation parameters using atmospheric neutrinos. Our results are also compatible and complementary to those obtained using neutrino beams from accelerators, which are obtained at lower neutrino energies and are subject to different sources of uncertainties.<br/>
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