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    Progress of Theoretical Physics

    Progress of Theoretical Physics

    JournalISSN 0033-068XeISSN 1347-4081

    年发文量

    研究主题

    论文(16324)

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    1Measurements of $\overline{\nu}_{\mu}$ and $\overline{\nu}_{\mu} + \nu_{\mu}$ Charged-Current Cross-Sections Without Detected Pions or Protons on Water and Hydrocarbon at a Mean Anti-Neutrino Energy of 0.86 GeV
    Kanji Abe,N. Akhlaq,R. Akutsu,Y. Takeuchi,C. Alt,C Andreopoulos,C. Andreopoulos,M. Antonova, S. Aoki,A. Ariga,T. Arihara,Y. Asada,

    We report measurements of the flux-integrated $\overline{\nu}_\mu$ and $\overline{\nu}_\mu+\nu_\mu$ charged-current cross-sections on water and hydrocarbon targets using the T2K anti-neutrino beam with a mean beam energy of 0.86 GeV. The signal is defined as the (anti-)neutrino charged-current interaction with one induced $\mu^\pm$ and no detected charged pion or proton. These measurements are performed using a new WAGASCI module recently added to the T2K setup in combination with the INGRID Proton Module. The phase space of muons is restricted to the high-detection efficiency region, $p_{\mu}>400~{\rm MeV}/c$ and $\theta_{\mu}<30^{\circ}$, in the laboratory frame. An absence of pions and protons in the detectable phase spaces of $p_{\pi}>200~{\rm MeV}/c$, $\theta_{\pi}<70^{\circ}$ and $p_{\rm p}>600~{\rm MeV}/c$, $\theta_{\rm p}<70^{\circ}$ is required. In this paper, both the $\overline{\nu}_\mu$ cross-sections and $\overline{\nu}_\mu+\nu_\mu$ cross-sections on water and hydrocarbon targets and their ratios are provided by using the D’Agostini unfolding method. The results of the integrated $\overline{\nu}_\mu$ cross-section measurements over this phase space are $\sigma_{\rm H_{2}O}=(1.082\pm0.068(\rm stat.)^{+0.145}_{-0.128}(\rm syst.)) \times 10^{-39}\,{\rm cm^{2} / nucleon}$, $\sigma_{\rm CH}=(1.096\pm0.054(\rm stat.)^{+0.132}_{-0.117}(\rm syst.)) \times 10^{-39}\,{\rm cm^{2} / nucleon}$, and $\sigma_{\rm H_{2}O}/\sigma_{\rm CH} = 0.987\pm0.078(\rm stat.)^{+0.093}_{-0.090}(\rm syst.)$. The $\overline{\nu}_\mu+\nu_\mu$ cross-section is $\sigma_{\rm H_{2}O} = (1.155\pm0.064(\rm stat.)^{+0.148}_{-0.129}(\rm syst.)) \times 10^{-39}\,{\rm cm^{2} / nucleon}$, $\sigma_{\rm CH}=(1.159\pm0.049(\rm stat.)^{+0.129}_{-0.115}(\rm syst.)) \times 10^{-39}\,{\rm cm^{2} / nucleon}$, and $\sigma_{\rm H_{2}O}/\sigma_{\rm CH}=0.996\pm0.069(\rm stat.)^{+0.083}_{-0.078}(\rm syst.)$.

    2021
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    2Measurement of the Τ Michel Parameters Η¯ and Ξκ in the Radiative Leptonic Decay Τ−→ℓ−ντν¯ℓγ
    N. Shimizu et al.,R Kulasiri
    2018引用:23
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    3KL -> 0 Formula Decay Correlating with K in High-Scale SUSY
    M. Tanimoto,K. Yamamoto

    We have studied the contribution of high-scale SUSY to the |$K_L \to \pi ^0 \nu {\bar {\nu }}$| and |$K^+ \to \pi ^+ \nu {\bar {\nu }}$| processes by correlating with the CP-violating parameter |$\epsilon _K$|⁠. Taking account of the recent LHC results for Higgs discovery and SUSY searches, we consider high-scale SUSY at the |$10$|–|$50$|TeV scale in the framework of non-minimal squark (slepton) flavor mixing. The Z penguin mediated chargino dominates the SUSY contribution for these decays. At the |$10$|TeV SUSY scale, the chargino contribution can enhance the branching ratio of |$K_L \to \pi ^0 \nu {\bar {\nu }}$| by eight times compared with SM predictions, whereas the predicted branching ratio |${\textit {BR}}(K^+ \to \pi ^+ \nu {\bar {\nu }})$| increases by up to three times that of the SM. The gluino box diagram dominates the SUSY contribution of |$\epsilon _K$| up to |$30{\%}$|⁠. If down-squark mixing is neglected compared with up-squark mixing, the Z penguin mediated chargino dominates both SUSY contributions of |${\textit {BR}}(K_L \to \pi ^0 \nu {\bar {\nu }})$| and |$\epsilon _K$|⁠. Then, a correlation between them is found, but the chargino contribution to |$\epsilon _K$| is at most |$3{\%}$|⁠. Even if the SUSY scale is |$50$|TeV, the chargino process still enhances the branching ratio of |$K_L \to \pi ^0 \nu {\bar {\nu }}$| from the SM prediction by a factor of two, and |$\epsilon _K$| is deviated from the SM prediction by |$\mathcal {O}(10{\%})$|⁠. We also discuss the chargino contribution to the |$K_L \to \pi ^0 e^+e^-$| process.

    2015引用:10
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    4Backward-angle Photoproduction of \omega and \eta{’} Mesons from Protons in the Photon Energy Range
    A. K. Mohanty,Y. Nakatsugawa, Mamoru Yosoi,M. Niiyama,D. S. Ahn,J. K. Ahn,S. Ajimura,W. C. Chang,J.Y. Chen,S. Daté,H. Fujimura,S. Fukui,
    2015引用:22
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    5Langmuir Waves in Semi-Relativistic Spinless Quantum Plasmas
    A. Yu. Ivanov,P. A. Andreev

    Many particle quantum hydrodynamics based on the Darwin Hamiltonian (the Hamiltonian corresponding to the Darwin Lagrangian) is considered. A force field appearing in corresponding Euler equation is considered in details. Contributions from different terms of the Darwin Hamiltonian in the Euler equation are traced. For example, the relativistic correction to the kinetic energy of particles leads to several terms in the Euler equation, these terms have different form. One of them has a form similar to a term appearing from the Darwin term. Hence, the two different mechanisms give analogous contributions in wave dispersion. Microscopic analog of the Biot-Savart law, called the current-current interaction and describing an interaction of moving charges via the magnetic field, is also included in our description. The semi-relativistic generalization of the quantum Bohm potential is obtained. Contribution of the relativistic effects in the spectrum of plasma collective excitations is considered.

    2015引用:15
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    高被引作者

    作者引用发文
    Toshihide Maskawa1991029
    Shoichi Sakata80608
    Ziro Maki781729
    Masami Nakagawa781331
    Misao Sasaki538250
    Hideo Kodama524237
    Tsutomu Yanagida508932
    Yoshiki Kuramoto503237
    Takeo Matsubara425457
    Chushiro Hayashi421929

    高产作者

    作者引用发文
    Ryozo Tamagaki265099
    Shoichiro Otsuki136082
    Yasuhiko Tsue58478
    Hisashi Horiuchi335068
    Taichiro Kugo316662
    Kiyomi Ikeda351761
    Shigeo Minami25060
    Shin Ishida114260
    M Yamamura51159
    Takeo Matsubara425457

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