2006/12/22 by Chikara Fuji, Yasumasa Matsuura, Fuji, Chikara +6 · 1 citation
Physics and Astronomy · #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #Neutrino Physics Research #Particle physics theoretical and experimental studies #hep-ph
paper · pdf · doi:10.48550/arxiv.hep-ph/0612300
25 pages
arxiv created 2006/12/22 · openalex publication_date 2006/12/22 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
Kinematical aspects of pion decay π→ μν is studied, with neutrino mixing taken into account. An attempt is made to derive the transition probability for such a sequence of processes: a π+ produced at (xπ,tπ) with momentum pπ decays into a μ+ and a νμ somewhere in space-time and then the μ+ is detected at (xμ,tμ) with momentum pμ and a να (a neutrino with flavor α= e, μ, ...) is detected at (xν,tν) with momentum pν. It is shown that (1) if all the particles involved are treated as plane-waves, the energy-momentum conservation would eliminate the neutrino oscillating terms, leaving each mass-eigenstate to contribute separately to the transition probability; (2) if one treats all the particles involved as wave-packets, the neutrino oscillating terms would appear and would be multiplied by two suppression factors, which result from distinction in velocity and in energy between the two interfering neutrino mass-eigenstates. An approximate treatment which takes account of the two complementary features, each of the particles involved propagates along its classical trajectory on the one hand and energies and momenta of the particles involved are conserved during the decay on the other hand, is proposed and similarity and difference between our approach and that of Dolgov et al. are discussed.