4,032 research outputs found

    VcbV_{cb} from the semileptonic decay B→DℓνˉℓB\to D \ell \bar{\nu}_{\ell} and the properties of the DD meson distribution amplitude

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    The improved QCD light-cone sum rule (LCSR) provides an effective way to deal with the heavy-to-light transition form factors (TFFs). Firstly, we adopt the improved LCSR approach to deal with the Bβ†’DB\to D TFF f+(q2)f^{+}(q^2) up to twist-4 accuracy. Due to the elimination of the most uncertain twist-3 contribution and the large suppression of the twist-4 contribution, the obtained LCSR shall provide us a good platform for testing the DD-meson leading-twist DA. For the purpose, we suggest a new model for the DD-meson leading-twist DA (Ο•3D\phi_{3D}), whose longitudinal behavior is dominantly determined by a parameter BB. Moreover, we find its second Gegenbauer moment a2D∼Ba^D_2\sim B. Varying BB within certain region, one can conveniently mimic the DD-meson DA behavior suggested in the literature. Inversely, by comparing the estimations with the experimental data on the DD-meson involved processes, one can get a possible range for the parameter BB and a determined behavior for the DD-meson DA. Secondly, we discuss the Bβ†’DB\to D TFF at the maximum recoil region and present a detailed comparison of it with the pQCD estimation and the experimental measurements. Thirdly, by applying the LCSR on f+(q2)f^{+}(q^2), we study the CKM matrix element \Vcb together with its uncertainties by adopting two types of processes, i.e. the B0/BΛ‰0B^0/\bar{B}^0-type and the BΒ±B^{\pm}-type. It is noted that a smaller Bβ‰Ύ0.20B \precsim 0.20 shows a better agreement with the experimental value on \Vcb. For example, for the case of B=0.00B=0.00, we obtain ∣Vcb∣(B0/BΛ‰0βˆ’type)=(41.28βˆ’4.82+5.68βˆ’1.16+1.13)Γ—10βˆ’3|V_{cb}|(B^0/\bar{B}^0-{\rm type})=(41.28 {^{+5.68}_{-4.82}} {^{+1.13}_{-1.16}}) \times 10^{-3} and ∣Vcb∣(BΒ±βˆ’type)=(40.44βˆ’4.72+5.56βˆ’1.00+0.98)Γ—10βˆ’3|V_{cb}|(B^{\pm}-{\rm type})=(40.44 {^{+5.56}_{-4.72}} {^{+0.98}_{-1.00}}) \times 10^{-3}, whose first (second) uncertainty comes from the squared average of the mentioned theoretical (experimental) uncertainties.Comment: 13 pages, 10 figures. Reference updated and discussion improved. To be published in Nucl.Phys.

    Twist-3 light-cone distribution amplitudes of the scalar mesons within the QCD sum rules and their application to the B→SB \to S transition form factors

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    We investigate the twist-3 light-cone distribution amplitudes (LCDAs) of the scalar mesons a0a_0, K0βˆ—K^{\ast}_0 and f0f_0 within the QCD sum rules. The QCD sum rules are improved by a consistent treatment of the sizable ss-quark mass effects within the framework of the background field approach. Adopting the valence quark component (qΛ‰1q2)(\bar{q}_1 q_2) as the dominant structure of the scalar mesons, our estimation for their masses are close to the measured a0(1450)a_0(1450), K0βˆ—(1430)K^{\ast}_0(1430) and f0(1710)f_0(1710). From the sum rules, we obtain the first two non-zero moments of the twist-3 LCDAs Ο•a0s,Οƒ\phi^{s,\sigma}_{a_0}: ⟨ξs,a02(4)⟩=0.369β€…β€Š(0.245)\langle \xi_{s,a_0}^{2(4)} \rangle=0.369 \;(0.245) and βŸ¨ΞΎΟƒ,a02(4)⟩=0.203β€…β€Š(0.093)\langle \xi_{\sigma,a_0}^{2(4)} \rangle=0.203 \;(0.093); those of the twist-3 LCDAs Ο•K0βˆ—s,Οƒ\phi_{K^*_0}^{s,\sigma}: ⟨ξs,K0βˆ—1(2)⟩=0.004β€…β€Š(0.355)\langle \xi_{s,K^{\ast}_0}^{1(2)} \rangle =0.004\;(0.355) and βŸ¨ΞΎΟƒ,K0βˆ—1(2)⟩=0.018β€…β€Š(0.207)\langle \xi_{\sigma,K^{\ast}_0}^{1(2)} \rangle =0.018\;(0.207); and those of the twist-3 LCDAs Ο•f0s,Οƒ\phi_{f_0}^{s,\sigma}: ⟨ξs,f02(4)⟩=0.335β€…β€Š(0.212)\langle \xi_{s,f_0}^{2(4)} \rangle=0.335 \;(0.212) and βŸ¨ΞΎΟƒ,f02(4)⟩=0.196β€…β€Š(0.088)\langle \xi_{\sigma,f_0}^{2(4)} \rangle=0.196 \; (0.088), respectively. As an application of those twist-3 LCDAs, we study the Bβ†’SB \to S transition form factors by introducing proper chiral currents into the correlator, which is constructed such that the twist-3 LCDAs give dominant contribution and the twist-2 LCDAs make negligible contribution. Our results of the Bβ†’SB \to S transition form factors at the large recoil region q2≃0q^2 \simeq 0 are consistent with those obtained in the literature, which inversely shows the present twist-3 LCDAs are acceptable.Comment: 14 pages, 12 figures, 7 table

    The ρ\rho-meson longitudinal leading-twist distribution amplitude

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    In the present paper, we suggest a convenient model for the vector ρ\rho-meson longitudinal leading-twist distribution amplitude Ο•2;ρβˆ₯\phi_{2;\rho}^\|, whose distribution is controlled by a single parameter B2;ρβˆ₯B^\|_{2;\rho}. By choosing proper chiral current in the correlator, we obtain new light-cone sum rules (LCSR) for the B→ρB\to\rho TFFs A1A_1, A2A_2 and VV, in which the Ξ΄1\delta^1-order Ο•2;ρβˆ₯\phi_{2;\rho}^\| provides dominant contributions. Then we make a detailed discussion on the Ο•2;ρβˆ₯\phi_{2;\rho}^\| properties via those B→ρB\to\rho TFFs. A proper choice of B2;ρβˆ₯B^\|_{2;\rho} can make all the TFFs agree with the lattice QCD predictions. A prediction of ∣Vub∣|V_{\rm ub}| has also been presented by using the extrapolated TFFs, which indicates that a larger B2;ρβˆ₯B^{\|}_{2;\rho} leads to a larger ∣Vub∣|V_{\rm ub}|. To compare with the BABAR data on ∣Vub∣|V_{\rm ub}|, the longitudinal leading-twist DA Ο•2;ρβˆ₯\phi_{2;\rho}^\| prefers a doubly-humped behavior.Comment: 7 pages, 3 figures. Discussions improved and references updated. To be published in Phys.Lett.
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