35,416 research outputs found

    Intrinsic Charm Flavor and Helicity Content in the Proton

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    Contributions to the quark flavor and spin observables from the intrinsic charm in the proton are discussed in the SU(4) quark meson fluctuation model. Our results suggest that the probability of finding the intrinsic charm in the proton is less than 1%. The intrinsic charm helicity is small and negative, Δc≃−(0.003∼0.015)\Delta c \simeq -(0.003\sim 0.015). The fraction of the total quark helicity carried by the intrinsic charm is less than 2%, and c_\up/c_\dw=35/67.Comment: 4 pages, 2 tables (revised version

    3D structure of hadrons by generalized distribution amplitudes and gravitational form factors

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    Generalized distribution amplitudes (GDAs) are one type of three-dimensional structure functions, and they are related to the generalized distribution functions (GPDs) by the ss-tt crossing of the Mandelstam variables. The GDA studies provide information on three-dimensional tomography of hadrons. The GDAs can be investigated by the two-photon process γ∗γ→hhˉ\gamma^* \gamma \to h\bar h, and the GPDs are studied by the deeply virtual Compton scattering γ∗h→γh\gamma^* h \to \gamma h. The GDA studies had been pure theoretical topics, although the GPDs have been experimentally investigated, because there was no available experimental measurement. Recently, the Belle collaboration reported their measurements on the γ∗γ→π0π0\gamma^* \gamma \to \pi^0 \pi^0 differential cross section, so that it became possible to find the GDAs from their measurements. Here, we report our analysis of the Belle data for determining the pion GDAs. From the GDAs, the timelike gravitational form factors Θ1(s)\Theta_1 (s) and Θ2(s)\Theta_2 (s) can be calculated, which are mechanical (pressure, shear force) and mass (energy) form factors, respectively. They are converted to the spacelike form factors by using the dispersion relation, and then gravitational radii are evaluated for the pion. The mass and mechanical radii are obtained from Θ2\Theta_2 and Θ1\Theta_1 as ⟨r2⟩mass=0.56∼0.69\sqrt {\langle r^2 \rangle_{\text{mass}}} =0.56 \sim 0.69 fm and ⟨r2⟩mech=1.45∼1.56\sqrt {\langle r^2 \rangle_{\text{mech}}} =1.45 \sim 1.56 fm, whereas the experimental charge radius is ⟨r2⟩charge=0.672±0.008\sqrt {\langle r^2 \rangle_{\text{charge}}} =0.672 \pm 0.008 fm for the charged pion. Future developments are expected in this new field to explore gravitational physics in the quark and gluon level.Comment: 6 pages, LaTeX, 1 style file, 8 figure files, Proceedings of the XXV International Workshop on Deep-Inelastic Scattering and Related Subjects, April 3-7, 2017, University of Birmingham, U

    Light pseudoscalar eta and H->eta eta decay in the simplest little Higgs mode

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    The SU(3) simplest little Higgs model in its original framework without the so-called mu term inevitably involves a massless pseudoscalar boson eta, which is problematic for b-physics and cosmological axion limit. With the mu term introduced by hand, the eta boson acquires mass m_eta ~ mu, which can be lighter than half the Higgs boson mass in a large portion of the parameter space. In addition, the introduced mu term generates sizable coupling of H-eta-eta. The Higgs boson can dominantly decay into a pair of eta's especially when mH below the WW threshold. Another new decay channel of H->Z+eta can be dominant or compatible with H -> WW for mH above the Z+eta threshold. We show that the LEP bound on the Higgs boson mass is loosened to some extent due to this new H->eta eta decay channel as well as the reduced coupling of H-Z-Z. The Higgs boson mass bound falls to about 110 GeV for f=3-4 TeV. Since the eta boson decays mainly into a bb pair, H-> eta eta -> 4b and H-> Z eta -> Z bb open up other interesting search channels in the pursuit of the Higgs boson in the future experiments. We discuss on these issues.Comment: major modification considering the simplest little Higgs model with the mu ter

    Measuring Consensus in Binary Forecasts: NFL Game Predictions

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    Previous research on defining and measuring consensus (agreement) among forecasters has been concerned with evaluation of forecasts of continuous variables. This previous work is not relevant when the forecasts involve binary decisions: up-down or win-lose. In this paper we use Cohen¡¯s kappa coefficient, a measure of inter-rater agreement involving binary choices, to evaluate forecasts of National Football League games. This statistic is applied to the forecasts of 74 experts and 31 statistical systems that predicted the outcomes of games during two NFL seasons. We conclude that the forecasters, particularly the systems, displayed significant levels of agreement and that levels of agreement in picking game winners were higher than in picking against the betting line. There is greater agreement among statistical systems in picking game winners or picking winners against the line as the season progresses, but no change in levels of agreement among experts. High levels of consensus among forecasters are associated with greater accuracy in picking game winners, but not in picking against the line.binary forecasts, NFL, agreement, consensus, kappa coefficient
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