94 research outputs found

    Production of the PP-Wave Excited BcB_c-States through the Z0Z^0 Boson Decays

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    In Ref.[7],we have dealt with the production of the two color-singlet SS-wave (cbˉ)(c\bar{b})-quarkonium states Bc((cbˉ)1[1S0]>)B_c(|(c\bar{b})_{\bf 1}[^1S_0]>) and Bc((cbˉ)1[3S1]>)B^*_c(|(c\bar{b})_{\bf 1}[^3S_1]>) through the Z0Z^0 boson decays. As an important sequential work, we make a further discussion on the production of the more complicated PP-wave excited (cbˉ)(c\bar{b})-quarkonium states, i.e. (cbˉ)1[1P1]>|(c\bar{b})_{\bf 1}[^1P_1]> and (cbˉ)1[3PJ]>|(c\bar{b})_{\bf 1}[^3P_J]> (with J=(1,2,3)J=(1,2,3)). More over, we also calculate the channel with the two color-octet quarkonium states (cbˉ)8[1S0]g>|(c\bar{b})_{\bf 8}[^1S_0]g> and (cbˉ)8[3S1]g>|(c\bar{b})_{\bf 8}[^3S_1]g>, whose contributions to the decay width maybe at the same order of magnitude as that of the color-singlet PP-wave states according to the naive nonrelativistic quantum chromodynamics scaling rules. The PP-wave states shall provide sizable contributions to the BcB_c production, whose decay width is about 20% of the total decay width ΓZ0Bc\Gamma_{Z^0\to B_c}. After summing up all the mentioned (cbˉ)(c\bar{b})-quarkonium states' contributions, we obtain ΓZ0Bc=235.9122.0+352.8\Gamma_{Z^0\to B_c} =235.9^{+352.8}_{-122.0} KeV, where the errors are caused by the main uncertainty sources.Comment: 8 pages, 5 figures and 2 tables. basic formulae in the appendix are cut off to match the published version, which can be found in v1. to be published in Eur.Phys.J.

    Principle of Balance and the Sea Content of the Proton

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    In this study, the proton is taken as an ensemble of quark-gluon Fock states. Using the principle of balance that every Fock state should be balanced with all of the nearby Fock states (denoted as the balance model), instead of the principle of detailed balance that any two nearby Fock states should be balanced with each other (denoted as the detailed balance model), the probabilities of finding every Fock state of the proton are obtained. The balance model can be taken as a revised version of the detailed balance model, which can give an excellent description of the light flavor sea asymmetry (i.e., uˉdˉ\bar{u}\not= \bar{d}) without any parameter. In case of gggg\Leftrightarrow gg sub-processes not considered, the balance model and the detailed balance model give the same results. In case of gggg\Leftrightarrow gg sub-processes considered, there is about 10 percent difference between the results of these models. We also calculate the strange content of the proton using the balance model under the equal probability assumption.Comment: 32 latex pages, 4 ps figures, to appear in PR

    Z0Z_0 Boson Decays to Bc()B^{(*)}_c Meson and Its Uncertainties

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    The programming new e+ee^{+}e^- collider with high luminosity shall provide another useful platform to study the properties of the doubly heavy BcB_c meson in addition to the hadronic colliders as LHC and TEVATRON. Under the `New Trace Amplitude Approach', we calculate the production of the spin-singlet BcB_c and the spin-triplet BcB^*_c mesons through the Z0Z^0 boson decays, where uncertainties for the production are also discussed. Our results show Γ(1S0)=81.440.5+102.1\Gamma_{(^1S_0)}= 81.4^{+102.1}_{-40.5} KeV and Γ(3S1)=116.462.8+163.9\Gamma_{(^3S_1)}=116.4^{+163.9}_{-62.8} KeV, where the errors are caused by varying mbm_b and mcm_c within their reasonable regions.Comment: 11 pages, 5 figures, 2 tables. To be published in Eur.Phys.J.

    News from the Muon (g-2) Experiment at BNL

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    The magnetic moment anomaly a_mu = (g_mu - 2) / 2 of the positive muon has been measured at the Brookhaven Alternating Gradient Synchrotron with an uncertainty of 0.7 ppm. The new result, based on data taken in 2000, agrees well with previous measurements. Standard Model evaluations currently differ from the experimental result by 1.6 to 3.0 standard deviations.Comment: Talk presented at RADCOR - Loops and Legs 2002, Kloster Banz, Germany, September 8-13 2002, to be published in Nuclear Physics B (Proc. Suppl.); 5 pages, 3 figure

    Effect of general risk on trust, satisfaction, and recommendation intention for halal food

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    The purpose of this empirical study is to investigate the effect of general risk, a multidimensional factor, on halal customer trust, satisfaction and intention to recommend halal food. The study also calculates the mean comparison of trust, satisfaction and intention recommendation across the demographic variables of halal customers. Our results from the structural analysis revealed that general risk has significant and positive effects on trust, satisfaction, and intention to recommend halal food. In addition, the results of the mean difference test advised that satisfaction and intention to recommend halal food are significantly different between male and female customers and that trust significantly varies across halal customers with different educations and marital status backgrounds. This study added a valuable contribution to the current literature of halal food consumption by performing a set of symmetric analytical approaches to assess desired responses from halal food customers

    Use of SMS texts for facilitating access to online alcohol interventions: a feasibility study

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    A41 Use of SMS texts for facilitating access to online alcohol interventions: a feasibility study In: Addiction Science & Clinical Practice 2017, 12(Suppl 1): A4

    Experimental progress in positronium laser physics

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    Measurement of the νe and total 8B solar neutrino fluxes with the Sudbury Neutrino Observatory phase-III data set

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    This paper details the solar neutrino analysis of the 385.17-day phase-III data set acquired by the Sudbury Neutrino Observatory (SNO). An array of 3He proportional counters was installed in the heavy-water target to measure precisely the rate of neutrino-deuteron neutral-current interactions. This technique to determine the total active 8B solar neutrino flux was largely independent of the methods employed in previous phases. The total flux of active neutrinos was measured to be 5.54-0.31+0.33(stat.)-0.34+0.36(syst.)×106 cm-2 s-1, consistent with previous measurements and standard solar models. A global analysis of solar and reactor neutrino mixing parameters yielded the best-fit values of Δm2=7.59-0.21+0.19×10 -5eV2 and θ=34.4-1.2+1.3degrees
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