12 research outputs found

    Effects of the K+→π+ννˉK^+\to\pi^+\nu\bar{\nu} and of other processes on the mixing hierarchies in the four-generation model

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    We analyze in the four-generation model the first measurement of the branching ratio of rare kaon decay K+→π+νnuˉK^+\to\pi^+\nu\bar{nu}, along with the other processes of KL−KSK_L-K_S mass difference ΔmK\Delta m_K, CP-violating parameter ϵK,Bd−Bdˉ\epsilon_K, B_d-\bar{B_d} mixing, Bs−BsˉB_s-\bar{B_s} mixing, B(KL→μμˉ)B(K_L\to\mu\bar{\mu}), and the upper bound values of D0−D0ˉD^0-\bar{D^0} mixing and B(KL→π0ννˉ)B(K_L\to\pi^0\nu\bar{\nu}), and try to search for mixing of the fourth generation in the hierarchical mixing scheme of the Wolfenstein parametrization. Using the results for the mixing of the fourth generation, we discuss predictions of the D0−D0ˉD^0-\bar{D^0} mixing (ΔmD\Delta m_D) and the branching ratio of directly CP-violating decay process KL→π0ννˉK_L\to\pi^0\nu\bar{\nu}, and the effects on the CP asymmetry in neutral B meson decays and the unitarity triangle.Comment: 29 pages written in LaTex. 6 figures(drawn on LaTeX). Revised from "K+→π+ννˉK^+\to\pi^+\nu\bar{\nu} in the four-generation model" of the same Authors(TOKUSHIMA 99-1, January 1999). A minor chang

    CP violation effect in long-baseline neutrino oscillation in the four-neutrino model

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    We investigate CP-violation effect in the long-baseline neutrino oscillation in the four-neutrino model with mass scheme of the two nearly degenerate pairs separated with the order of 1 eV, by using the data from the solar neutrino deficit, the atmospheric neutrino anomaly and the LSND experiments along with the other accelerator and reactor experiments. By use of the most general parametrization of the mixing matrix with six angles and six phases, we show that the genuine CP-violation effect could attain as large as 0.3 for ΔP(νμ→ντ)≡P(νμ→ντ)−P(νμˉ→ντˉ)\Delta P(\nu_\mu\to\nu_\tau) \equiv P(\nu_\mu\to\nu_\tau) - P(\bar{\nu_\mu}\to\bar{\nu_\tau}) and that the matter effect is negligibly small such as at most 0.01 for ΔP(νμ→ντ)\Delta P(\nu_\mu\to\nu_\tau) for Δm2=(1−5)×10−3eV2\Delta m^2 = (1-5)\times 10^{-3} {\rm eV}^2, which is the mass-squared difference relevant to the long-baseline oscillation.Comment: 21 pages in LaTeX, 9 ps figures. Some changes in the Introduction and Reference
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