55 research outputs found

    Unquenching the scalar glueball

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    Computations in the quenched approximation on the lattice predict the lightest glueball to be a scalar in the 1.5-1.8 GeV region. Here we calculate the dynamical effect the coupling to two pseudoscalars has on the mass, width and decay pattern of such a scalar glueball. These hadronic interactions allow mixing with the qqq \overline q scalar nonet, which is largely fixed by the well-established K_0^*(1430). This non-perturbative mixing means that, if the pure gluestate has a width to two pseudoscalar channels of ~100 MeV as predicted on the lattice, the resulting hadron has a width to these channels of only ~30 MeV with a large eta-eta component. Experimental results need to be reanalyzed in the light of these predictions to decide if either the f_0(1500) or an f_0(1710) coincides with this dressed glueball.Comment: 12 pages, LaTex, 3 Postscript figure

    Strange Decays of Nonstrange Baryons

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    The strong decays of excited nonstrange baryons into the final states Lambda K, Sigma K, and for the first time into Lambda(1405) K, Lambda(1520) K, Sigma(1385) K, Lambda K*, and Sigma K*, are examined in a relativized quark pair creation model. The wave functions and parameters of the model are fixed by previous calculations of N pi and N pi pi, etc., decays. Our results show that it should be possible to discover several new negative parity excited baryons and confirm the discovery of several others by analyzing these final states in kaon production experiments. We also establish clear predictions for the relative strengths of certain states to decay to Lambda(1405) K and Lambda(1520) K, which can be tested to determine if a three-quark model of the Lambda(1405) K is valid. Our results compare favorably with the results of partial wave analyses of the limited existing data for the Lambda K and Sigma K channels. We do not find large Sigma K decay amplitudes for a substantial group of predicted and weakly established negative-parity states, in contrast to the only previous work to consider decays of these states into the strange final states Lambda K and Sigma K.Comment: 25 pages, 8 figures, RevTe

    On the Mechanism of Open-Flavor Strong Decays

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    Open-flavor strong decays are mediated by qqˉq\bar q pair production, which is known to occur dominantly with \3p0 quantum numbers. The relation of the phenomenological \3p0 model of these decays to ``microscopic" QCD decay mechanisms has never been clearly established. In this paper we investigate qqˉq\bar q meson decay amplitudes assuming pair production from the scalar confining interaction (sKs) and from one gluon exchange (OGE). sKs pair production predicts decay amplitudes of approximately the correct magnitude and D/S amplitude ratios in b1ωπb_1\to\omega\pi and a1ρπa_1\to\rho\pi which are close to experiment. The OGE decay amplitude is found to be subdominant in most cases, a notable exception being 3^3P01_0\to{}^1S0+1_0+{}^1S0_0. The full sKs~+~OGE amplitudes differ significantly from \3p0 model predictions in some channels and can be distinguished experimentally, for example through an accurate comparison of the D/S amplitude ratios in b1ωπb_1\to\omega\pi and a1ρπa_1\to\rho\pi.Comment: 44 pages, 22 eps figures, RevTex, complete postscript file available at http://csep2.phy.ornl.gov/theory_group/people/barnes/pubs/abs.p

    Quark--antiquark states and their radiative transitions in terms of the spectral integral equation. {\Huge II.} Charmonia

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    In the precedent paper of the authors (hep-ph/0510410), the bbˉb\bar b states were treated in the framework of the spectral integral equation, together with simultaneous calculations of radiative decays of the considered bottomonia. In the present paper, such a study is carried out for the charmonium (ccˉ)(c\bar c) states. We reconstruct the interaction in the ccˉc\bar c-sector on the basis of data for the charmonium levels with JPC=0+J^{PC}=0^{-+}, 11^{--}, 0++0^{++}, 1++1^{++}, 2++2^{++}, 1+1^{+-} and radiative transitions ψ(2S)γχc0(1P)\psi(2S)\to\gamma\chi_{c0}(1P), γχc1(1P)\gamma\chi_{c1}(1P), γχc2(1P)\gamma\chi_{c2}(1P), γηc(1S)\gamma\eta_{c}(1S) and χc0(1P)\chi_{c0}(1P), χc1(1P)\chi_{c1}(1P), χc2(1P)γJ/ψ\chi_{c2}(1P)\to\gamma J/\psi. The ccˉc\bar c levels and their wave functions are calculated for the radial excitations with n6n\le 6. Also, we determine the ccˉc\bar c component of the photon wave function using the e+ee^+e^- annihilation data: e+eJ/ψ(3097)e^+e^- \to J/\psi(3097), ψ(3686)\psi(3686), ψ(3770)\psi(3770), ψ(4040)\psi(4040), ψ(4160) \psi(4160), ψ(4415)\psi(4415) and perform the calculations of the partial widths of the two-photon decays for the n=1n=1 states: ηc0(1S)\eta_{c0}(1S), χc0(1P)\chi_{c0}(1P), χc2(1P)γγ\chi_{c2}(1P)\to\gamma\gamma, and n=2n=2 states: ηc0(2S)γγ\eta_{c0}(2S)\to\gamma\gamma, χc0(2P)\chi_{c0}(2P), χc2(2P)γγ\chi_{c2}(2P)\to \gamma\gamma. We discuss the status of the recently observed ccˉc\bar c states X(3872) and Y(3941): according to our results, the X(3872) can be either χc1(2P)\chi_{c1}(2P) or ηc2(1D)\eta_{c2}(1D), while Y(3941) is χc2(2P)\chi_{c2}(2P).Comment: 24 pages, 9 figure

    Relativistic two-photon and two-gluon decay rates of heavy quarkonia

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    The decay rates of ccˉc\bar{c} and bbˉb\bar{b} through two-photon or two-gluon annihilations are obtained by using totally relativistic decay amplitudes and a sophisticated quantum-chromodynamic potential model for heavy quarkonia. Our results for the photonic and gluonic widths of the 1S0, 3P0, and the 3P2 states are in excellent agreement with the available experimental data. The procedures and mathematical techniques used by us for the treatment of the fermion-antifermion bound states are also applicable to other decay processes.Comment: 15 pages, RevTeX, PostScript available at http://gluon.physics.wayne.edu/wsuhep/jim/predecay.p

    Pseuduscalar Heavy Quarkonium Decays With Both Relativistic and QCD Radiative Corrections

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    We estimate the decay rates of ηc2γ\eta_c\rightarrow 2\gamma, ηc2γ\eta_c'\rightarrow 2\gamma, and J/ψe+eJ/\psi\rightarrow e^+ e^-, ψe+e\psi^\prime\rightarrow e^+e^-, by taking into account both relativistic and QCD radiative corrections. The decay amplitudes are derived in the Bethe-Salpeter formalism. The Bethe-Salpeter equation with a QCD-inspired interquark potential are used to calculate the wave functions and decay widths for these ccˉc\bar{c} states. We find that the relativistic correction to the ratio RΓ(ηc2γ)/Γ(J/ψe+e)R\equiv \Gamma (\eta_c \rightarrow 2\gamma)/ \Gamma (J/ \psi \rightarrow e^+ e^-) is negative and tends to compensate the positive contribution from the QCD radiative correction. Our estimate gives Γ(ηc2γ)=(67) keV\Gamma(\eta_c \rightarrow 2\gamma)=(6-7) ~keV and Γ(ηc2γ)=2 keV\Gamma(\eta_c^\prime \rightarrow 2\gamma)=2 ~keV, which are smaller than their nonrelativistic values. The hadronic widths Γ(ηc2g)=(1723) MeV\Gamma(\eta_c \rightarrow 2g)=(17-23) ~MeV and Γ(ηc2g)=(57) MeV\Gamma(\eta_c^\prime \rightarrow 2g)=(5-7)~MeV are then indicated accordingly to the first order QCD radiative correction, if αs(mc)=0.260.29\alpha_s(m_c)=0.26-0.29. The decay widths for bbˉb\bar b states are also estimated. We show that when making the assmption that the quarks are on their mass shells our expressions for the decay widths will become identical with that in the NRQCD theory to the next to leading order of v2v^2 and αs\alpha_s.Comment: 14 pages LaTex (2 figures included

    Radiative Decays of Excited Vector Mesons

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    Radiative decays of the 13S11^3S_1 radial and 13D11^3D_1 orbital excitations of the ρ\rho, ω\omega and ϕ\phi are calculated in the quark model, using wave functions obtained variationally from the Hamiltonian with standard quark-model parameters. The larger radiative widths should be measurable at new high-intensity facilities being proposed, and in some cases may be measurable in data from existing experiments. The radiative decays are a strong discriminator between the 13S11^3S_1 and 13D11^3D_1 excitations, and can also be used to provide unique information about the decay products.Comment: 23 pages, 6 figure

    Application of Jain and Munczek's bound-state approach to gamma gamma-processes of pi0, eta_c and eta_b

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    We point out the problems affecting most quark--antiquark bound state approaches when they are faced with the electromagnetic processes dominated by Abelian axial anomaly. However, these problems are resolved in the consistently coupled Schwinger-Dyson and Bethe-Salpeter approach. Using one of the most successful variants of this approach, we find the dynamically dressed propagators of the light u and d quarks, as well as the heavy c and b quarks, and find the Bethe-Salpeter amplitudes for their bound states pi0, eta_c and \eta_b. Thanks to incorporating the dynamical chiral symmetry breaking, the pion simultaneously appears as the (pseudo)Goldstone boson. We give the theoretical predictions for the gamma-gamma decay widths of pi0, eta_c and eta_b, and for the pi0 gamma* -> gamma transition form factor, and compare them with experiment. In the chiral limit, the axial-anomaly result for pi0->gamma-gamma is reproduced analytically in the consistently coupled Schwinger-Dyson and Bethe-Salpeter approach, provided that the quark-photon vertex is dressed consistently with the quark propagator, so that the vector Ward-Takahashi identity of QED is obeyed. On the other hand, the present approach is also capable of quantitatively describing systems of heavy quarks, concretely eta_c and possibly eta_b, and their gamma-gamma decays. We discuss the reasons for the broad phenomenological success of the bound-state approach of Jain and Munczek.Comment: RevTeX, 37 pages, 7 eps figures, submitted to Int. J. Mod. Phys.

    The newly observed open-charm states in quark model

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    Comparing the measured properties of the newly observed open-charm states D(2550), D(2600), D(2750), D(2760), D_{s1}(2710), D_{sJ}(2860), and D_{sJ}(3040) with our predicted spectroscopy and strong decays in a constituent quark model, we find that: (1) the D(2\,^1S_0) assignment to D(2550) remains open for its too broad width determined by experiment; (2) the D(2600) and Ds1(2710)D_{s1}(2710) can be identified as the 2\,^3S_1-1\,^3D_1 mixtures; (3) if the D(2760) and D(2750) are indeed the same resonance, they would be the D(1\,^3D_3); otherwise, they could be assigned as the D(1\,^3D_3) and D2(1D)D^\prime_2(1D), respectively; (4) the DsJ(2860)D_{sJ}(2860) could be either the Ds1(2710)D_{s1}(2710)'s partner or the D_s(1\,^3D_3); and (5) both the Ds1(2P)D_{s1}(2P) and Ds1(2P)D^\prime_{s1}(2P) interpretations for the DsJ(3040)D_{sJ}(3040) seem likely. The E1E1 and M1M1 radiative decays of these sates are also studied. Further experimental efforts are needed to test the present quarkonium assignments for these new open-charm states.Comment: 26 pages,7 figures, journal versio

    The Decay ηcγγ\eta_c \rightarrow \gamma \gamma : A Test for Potential Models

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    We use a simple perturbation theory argument and measurements of charmonium leptonic widths Γ(ψNSe+e)\Gamma (\psi_{NS} \rightarrow e^+e^-) to estimate the ratio \mbox{RΨηc1S(0)2/Ψψ1S(0)2R_\circ \equiv {\vert \Psi _{\eta_{c1S}}(0) \vert}^2 /{\vert\Psi_{\psi_{1 S}}(0)\vert}^2} in the general context of non- relativistic potential models. We obtain R=1.4±0.1R_\circ = 1.4 \pm 0.1. We then apply well known potential model formulas, which include lowest order QCD corrections, to find Γ(ηcγγ)/Γ(ψ1Se+e)2.2±0.2\Gamma (\eta_c \rightarrow \gamma \gamma )/\Gamma (\psi_{1S} \rightarrow e^+e^-) \approx 2.2\pm 0.2. The central value for Γ(ψ1Se+e)\Gamma (\psi_{1S} \rightarrow e^+ e^-)in the 1992 Particle Data Tables then leads to a (non relativistic) prediction Γ(ηcγγ)11.8±0.8\Gamma (\eta_c \rightarrow \gamma \gamma )\approx 11.8\pm 0.8 keV. This prediction is in good agreement with a recent measurement by the ARGUS collaboration, is consistent with a recent measurement by the L3 collaboration but is significantly higher than several earlier measurements and than previous theoretical estimates, which usually assume R=1R_\circ =1. The correction to R=1R_\circ =1 is estimated to be smaller but nonnegligible for the bbˉb\bar b system. Using the current central measurement for Γ(Υ1Se+e)\Gamma (\Upsilon_{1S}\rightarrow e^+e^-) we find Γ(ηbγγ)0.58±0.03\Gamma (\eta_b\rightarrow \gamma \gamma )\approx 0.58\pm 0.03 keV. A rough estimate of relativistic corrections reduces the expected two photon rates to about 8.8 keV and 0.52 keV for the ηc\eta_c and ηb\eta_b mesons respectively. Such correctionsComment: Estimates of likely relativistic corrections to the results have been adde
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