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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