Abstract
We report in detail on searches for eV-scale sterile neutrinos, in the context of a 3+1 model, using eight years of data from the IceCube Neutrino Telescope. By analyzing the reconstructed energies and zenith angles of 305,735 atmospheric ππ and
ππbar events we construct confidence intervals in two analysis spaces: sin2β‘(2β’π24) vs Ξβ’π2 41 under the conservative assumption π34 =0; and sin2β‘(2β’π24) vs sin2β‘(2β’π34) given sufficiently large Ξβ’π2 41 that fast oscillation features are unresolvable. Detailed discussions of the event selection, systematic uncertainties, and fitting procedures are presented. No strong evidence for sterile neutrinos is found, and the best-fit likelihood is consistent with the no sterile neutrino hypothesis with a π value of 8% in the first analysis space and 19% in the second.
ππbar events we construct confidence intervals in two analysis spaces: sin2β‘(2β’π24) vs Ξβ’π2 41 under the conservative assumption π34 =0; and sin2β‘(2β’π24) vs sin2β‘(2β’π34) given sufficiently large Ξβ’π2 41 that fast oscillation features are unresolvable. Detailed discussions of the event selection, systematic uncertainties, and fitting procedures are presented. No strong evidence for sterile neutrinos is found, and the best-fit likelihood is consistent with the no sterile neutrino hypothesis with a π value of 8% in the first analysis space and 19% in the second.
| Original language | English |
|---|---|
| Pages (from-to) | 052009 |
| Journal | Physical Review D: Particles, Fields, Gravitation and Cosmology |
| Volume | 102 |
| DOIs | |
| Publication status | Published - 2021 |
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