Exploration of mass splitting and muon/tau mixing parameters for an eV-scale sterile neutrino with IceCube
R. Abbasi, M. Ackermann, J. Adams, S. K. Agarwalla, J. A. Aguilar, M., Ahlers, J.M. Alameddine, N. M. Amin, K. Andeen, C. Arg\"uelles, Y. Ashida, S., Athanasiadou, L. Ausborm, S. N. Axani, X. Bai, A. Balagopal V., M. Baricevic,, S. W. Barwick, S. Bash, V. Basu, R. Bay

TL;DR
This paper presents the first three-parameter fit to an eV-scale sterile neutrino model using IceCube data, constraining mass splitting and mixing parameters with implications for sterile neutrino searches.
Contribution
It introduces the first comprehensive 3+1 sterile neutrino parameter space mapping using IceCube data, focusing on mass splitting and muon/tau mixing parameters.
Findings
Consistent with no sterile neutrino hypothesis (4.3% probability)
Constraints on $\Delta m_{41}^2$ between 2.4 and 9.6 eV$^2$
Limits on $|U_{ au4}|^2$ below 0.035
Abstract
We present the first three-parameter fit to a 3+1 sterile neutrino model using 7.634 years of data from the IceCube Neutrino Observatory on charged-current interactions in the energy range 500--9976 GeV. Our analysis is sensitive to the mass-squared splitting between the heaviest and lightest mass state (), the mixing matrix element connecting muon flavor to the fourth mass state (), and the element connecting tau flavor to the fourth mass state (). Predicted propagation effects in matter enhance the signature through a resonance as atmospheric neutrinos from the Northern Hemisphere traverse the Earth to the IceCube detector at the South Pole. The remaining sterile neutrino matrix elements are left fixed, with and , as they have a negligible effect, and is set to…
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