File:Atmosheric neutrino numu to nue oscillation probability for NH.png
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![File:Atmosheric neutrino numu to nue oscillation probability for NH.png](https://upload.wikimedia.org/wikipedia/commons/thumb/c/c1/Atmosheric_neutrino_numu_to_nue_oscillation_probability_for_NH.png/618px-Atmosheric_neutrino_numu_to_nue_oscillation_probability_for_NH.png?20220105160317)
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Atmospheric neutrino νμ → νe (ν̄μ → ν̄e) oscillation probabilities in case of the normal (inverted) mass hierarchy.
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[edit]DescriptionAtmosheric neutrino numu to nue oscillation probability for NH.png |
English: Atmospheric neutrino oscillation probabilities as a function of energy and cosine of the neutrino zenith angle (−1 corresponds to upward-going). The plot shows the νμ → νe probability in case of the normal mass hierarchy or ν̄μ → ν̄e in case of the inverted mass hierarchy. |
Date | |
Source | "Physics potentials with the second Hyper-Kamiokande detector in Korea", PTEP 2018 (2018) 6, 063C01, Prog Theor Exp Phys (2018), https://arxiv.org/abs/1611.06118, https://doi.org/10.1093/ptep/pty044 |
Author | Hyper-Kamiokande Collaboration (K. Abe et al.) |
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current | 16:03, 5 January 2022 | ![]() | 796 × 772 (228 KB) | Batmann (talk | contribs) | Uploaded a work by Hyper-Kamiokande Collaboration (K. Abe et al.) from "Physics potentials with the second Hyper-Kamiokande detector in Korea", PTEP 2018 (2018) 6, 063C01, Prog Theor Exp Phys (2018), https://arxiv.org/abs/1611.06118, https://doi.org/10.1093/ptep/pty044 with UploadWizard |
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20 June 2018
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