432 research outputs found

    On P-wave meson decay constants in the heavy quark limit of QCD

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    In previous work it has been shown that, either from a sum rule for the subleading Isgur-Wise function ξ3(1)\xi_3(1) or from a combination of Uraltsev and Bjorken SR, one infers for PP-wave states τ1/2(1)τ3/2(1)|\tau_{1/2}(1)| \ll |\tau_{3/2}(1)|. This implies, in the heavy quark limit of QCD, a hierarchy for the {\it production} rates of PP-states Γ(BˉdD(12)ν)Γ(BˉdD(32)ν)\Gamma(\bar{B}_d \to D ({1 \over 2}) \ell \nu) \ll \Gamma(\bar{B}_d \to D ({3 \over 2}) \ell \nu) that seems at present to be contradicted by experiment. It was also shown that the decay constants of j=32j = {3 \over 2} PP-states vanish in the heavy quark limit of QCD, f3/2(n)=0f_{3/2}^{(n)} = 0. Assuming the {\it model} of factorization in the decays BˉdDˉsD\bar{B}_d \to \bar{D}_s^{**}D, one expects the opposite hierarchy for the {\it emission} rates Γ(BˉdDˉs(32)D)Γ(BˉdDˉs(12)D)\Gamma(\bar{B}_d \to \bar{D}_s ({3 \over 2}) D) \ll \Gamma(\bar{B}_d \to \bar{D}_s ({1 \over 2}) D), since j=12j = {1 \over 2} PP-states are coupled to vacuum. Moreover, using Bjorken SR and previously discovered SR involving heavy-light meson decay constants and IW functions, one can prove that the sums n(f(n)f(0))2\sum\limits_n ({f^{(n)} \over f^{(0)}})^2, n(f1/2(n)f(0))2\sum\limits_n ({f_{1/2}^{(n)} \over f^{(0)}})^2 (where f(n)f^{(n)} and f1/2(n)f_{1/2}^{(n)} are the decay constants of SS-states and j=12j = {1\over 2} PP-states) are divergent. This situation seems to be realized in the relativistic quark models \`a la Bakamjian and Thomas, that satisfy HQET and predict decays constants f(n)f^{(n)} and f1/2(n)f_{1/2}^{(n)} that do not decrease with the radial quantum number nn.Comment: 7 pages, Late

    Sum rules in the heavy quark limit of QCD

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    In the leading order of the heavy quark expansion, we propose a method within the OPE and the trace formalism, that allows to obtain, in a systematic way, Bjorken-like sum rules for the derivatives of the elastic Isgur-Wise function ξ(w)\xi(w) in terms of corresponding Isgur-Wise functions of transitions to excited states. A key element is the consideration of the non-forward amplitude, as introduced by Uraltsev. A simplifying feature of our method is to consider currents aligned along the initial and final four-velocities. As an illustration, we give a very simple derivation of Bjorken and Uraltsev sum rules. On the other hand, we obtain a new class of sum rules that involve the products of IW functions at zero recoil and IW functions at any ww. Special care is given to the needed derivation of the projector on the polarization tensors of particles of arbitrary integer spin. The new sum rules give further information on the slope ρ2=ξ(1)\rho^2 = - \xi '(1) and also on the curvature σ2=ξ(1)\sigma^2 = \xi '' (1), and imply, modulo a very natural assumption, the inequality σ254ρ2\sigma^2 \geq {5\over 4} \rho^2, and therefore the absolute bound σ21516\sigma^2 \geq {15 \over 16}.Comment: 64 pages, Late

    DsJ(2860)D_{sJ}(2860) and DsJ(2715)D_{sJ}(2715)

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    Recently Babar Collaboration reported a new csˉc\bar{s} state DsJ(2860)D_{sJ}(2860) and Belle Collaboration observed DsJ(2715)D_{sJ}(2715). We investigate the strong decays of the excited csˉc\bar{s} states using the 3P0^{3}P_{0} model. After comparing the theoretical decay widths and decay patterns with the available experimental data, we tend to conclude: (1) DsJ(2715)D_{sJ}(2715) is probably the 1(13D1)1^{-}(1^{3}D_{1}) csˉc\bar{s} state although the 1(23S1)1^{-}(2^{3}S_{1}) assignment is not completely excluded; (2) DsJ(2860)D_{sJ}(2860) seems unlikely to be the 1(23S1)1^{-}(2^{3}S_{1}) and 1(13D1)1^{-}(1^{3}D_{1}) candidate; (3) DsJ(2860)D_{sJ}(2860) as either a 0+(23P0)0^{+}(2^{3}P_{0}) or 3(13D3)3^{-}(1^{3}D_{3}) csˉc\bar{s} state is consistent with the experimental data; (4) experimental search of DsJ(2860)D_{sJ}(2860) in the channels DsηD_s\eta, DKDK^{*}, DKD^{*}K and DsηD_{s}^{*}\eta will be crucial to distinguish the above two possibilities.Comment: 18 pages, 7 figures, 2 tables. Some discussions added. The final version to appear at EPJ

    Angular analysis of B -> J/psi K1 : towards a model independent determination of the photon polarization with B-> K1 gamma

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    We propose a model independent extraction of the hadronic information needed to determine the photon polarization of the b-> s gamma process by the method utilizing the B -> K1 gamma -> K pi pi gamma angular distribution. We show that exactly the same hadronic information can be obtained by using the B -> J/psi K1 -> J/psi K pi pi channel, which leads to a much higher precision.Comment: 12 pages, 1 figur

    Equation of state of strongly coupled Hamiltonian lattice QCD at finite density

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    We calculate the equation of state of strongly coupled Hamiltonian lattice QCD at finite density by constructing a solution to the equation of motion corresponding to an effective Hamiltonian using Wilson fermions. We find that up to and beyond the chiral symmetry restoration density the pressure of the quark Fermi sea can be negative indicating its mechanical instability. This result is in qualitative agreement with continuum models and should be verifiable by future numerical simulations.Comment: 14 pages, 2 EPS figures. Revised version - added discussion on the equation of stat

    Critical Analysis of Theoretical Estimates for BB to Light Meson Form Factors and the BψK(K)B \to \psi K(K^{\ast}) Data

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    We point out that current estimates of form factors fail to explain the non-leptonic decays BψK(K)B \to \psi K(K^{\ast}) and that the combination of data on the semi-leptonic decays DK(K)νD \to K(K^{\ast})\ell \nu and on the non-leptonic decays BψK(K)B \to \psi K(K^{\ast}) (in particular recent po\-la\-ri\-za\-tion data) severely constrain the form (normalization and q2q^2 dependence) of the heavy-to-light meson form factors, if we assume the factorization hypothesis for the latter. From a simultaneous fit to \bpsi and \dk data we find that strict heavy quark limit scaling laws do not hold when going from DD to BB and must have large corrections that make softer the dependence on the masses. We find that A1(q2)A_1(q^2) should increase slower with \qq than A2,V,f+A_2, V, f_+. We propose a simple parametrization of these corrections based on a quark model or on an extension of the \hhs laws to the \hl case, complemented with an approximately constant A1(q2)A_1(q^2). We analyze in the light of these data and theoretical input various theoretical approaches (lattice calculations, QCD sum rules, quark models) and point out the origin of the difficulties encountered by most of these schemes. In particular we check the compatibility of several quark models with the heavy quark scaling relations.Comment: 48 pages, DAPNIA/SPP/94-24, LPTHE-Orsay 94/1
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