Abstract
Neutrino oscillations, in a two neutrino mixing scenario, are the most likely solution for the atmospheric neutrino problem [1]. Underground experiments unfold the mass difference Δm 2 = m 2 v2 and the mixing angle θ from the measurement of the survival probability P(v μ → v μ) = 1 − sin 22 θ sin 2(1.27Δm 2 l v /E v ) .
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Bakari, D., Becherini, Y., Spurio, M. (2001). Estimate of the Energy of Upgoing Muons with Multiple Coulomb Scattering. In: Giacomelli, G., Spurio, M., Derkaoui, J.E. (eds) Cosmic Radiations: From Astronomy to Particle Physics. NATO Science Series, vol 42. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0634-7_12
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DOI: https://doi.org/10.1007/978-94-010-0634-7_12
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