Abstract
The angular distribution of upward-going muons produced by atmospheric neutrinos in the rock below the MACRO detector shows anomalies in good agreement with two flavor vμ → vτ oscillations with maximum mixing and Δm2 around 0.0024 eV2. Exploiting the dependence of magnitude of the matter effect on oscillation channel, and using a set of 809 upward-going muons observed in MACRO, we show that the two flavor vμ → vs oscillation is disfavored with 99% C.L. with respect to vμ → vτ.
| Lingua originale | Inglese |
|---|---|
| pagine (da-a) | 59-66 |
| Numero di pagine | 8 |
| Rivista | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics |
| Volume | 517 |
| Numero di pubblicazione | 1-2 |
| DOI | |
| Stato di pubblicazione | Pubblicato - 27 set 2001 |
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