11 research outputs found

    Discovery of naked charm particles and lifetime differences among charm species using nuclear emulsion techniques innovated in Japan

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    This is a historical review of the discovery of naked charm particles and lifetime differences among charm species. These discoveries in the field of cosmic-ray physics were made by the innovation of nuclear emulsion techniques in Japan. A pair of naked charm particles was discovered in 1971 in a cosmic-ray interaction, three years prior to the discovery of the hidden charm particle, J/Ψ, in western countries. Lifetime differences between charged and neutral charm particles were pointed out in 1975, which were later re-confirmed by the collaborative Experiment E531 at Fermilab. Japanese physicists led by K.Niu made essential contributions to it with improved emulsion techniques, complemented by electronic detectors. This review also discusses the discovery of artificially produced naked charm particles by us in an accelerator experiment at Fermilab in 1975 and of multiple-pair productions of charm particles in a single interaction in 1987 by the collaborative Experiment WA75 at CERN

    Measurement of B(D_s+ -> mu+ nu_mu)/B(D_s+ -> phi mu+ nu_mu) and Determination of the Decay Constant f_{D_s}

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    We have observed 23.2±6.00.9+1.023.2 \pm 6.0_{-0.9}^{+1.0} purely-leptonic decays of Ds+>μ+νμD_s^+ -> \mu^+ \nu_\mu from a sample of muonic one prong decay events detected in the emulsion target of Fermilab experiment E653. Using the Ds+>ϕμ+νμD_s^+ -> \phi \mu^+ \nu_\mu yield measured previously in this experiment, we obtain B(Ds+>μ+νμ)/B(Ds+>ϕμ+νμ)=0.16±0.06±0.03B(D_s^+ --> \mu^+ \nu_\mu) / B(D_s^+ --> \phi \mu^+ \nu_\mu) =0.16 \pm 0.06 \pm 0.03. In addition, we extract the decay constant fDs=194±35±20±14MeVf_{D_s}=194 \pm 35 \pm 20 \pm 14 MeV.Comment: 15 pages including one figur

    Observation of D+ -> rho0(770) mu+ nu

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    We report the first observation of the Cabibbo disfavored semileptonic decay mode D+ -> rho0(770) mu+ nu, and measure its decay rate relative to the Cabibbo favored mode D+ -> K*0(892) mu+ nu to be Gamma(D+ -> rho0(770) mu+ nu) / Gamma(D+ -> K*0(892) mu+ nu) = 0.044 +0.031 -0.025 (stat.) +/- 0.014 (sys). The results are compared to theoretical predictions and to previous experimental upper limits.Comment: 15 pgs., OKHEP-93-0
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