457 research outputs found

    Isgur-Wise form factors of heavy baryons within a light-front constituent quark model

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    The space-like elastic form factors of baryons containing a heavy quark are investigated within a light-front constituent quark model in the limit of infinite heavy-quark mass, adopting a gaussian-like ansatz for the three-quark wave function. The results obtained for the Isgur-Wise form factors corresponding both to a spin-0 and a spin-1 light spectator pair are presented. It is found that the Isgur-Wise functions depend strongly on the baryon structure, being sharply different in case of diquark-like or collinear-type configurations in the three-quark system. It is also shown that the relativistic effects lead to a saturation property of the form factors as a function of the baryon size. Our results are compared with those of different models as well as with recent predictions from QCD sum rules and lattice QCD simulations; the latter ones seem to suggest the dominance of collinear-type configurations, in which the heavy-quark is sitting close to the center-of-mass of the light quark pair.Comment: latex, 15 pp., 6 figures with epsfig.st

    The light-quark contribution to the leading HVP term of the muon g−2g - 2 from twisted-mass fermions

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    We present a lattice calculation of the leading Hadronic Vacuum Polarization (HVP) contribution of the light u- and d-quarks to the anomalous magnetic moment of the muon, aμHVP(ud)a_\mu^{\rm HVP}(ud), adopting the gauge configurations generated by the European Twisted Mass Collaboration with Nf=2+1+1N_f = 2+1+1 dynamical quarks at three values of the lattice spacing with pion masses in the range 210 - 450 MeV. Thanks to several lattices at fixed values of the light-quark mass and scale but with different sizes we perform a careful investigation of finite-volume effects (FVEs). In order to remove FVEs we develop an analytic representation of the vector correlator, which describes the lattice data for time distances larger than ≃0.2\simeq 0.2 fm. The representation is based on quark-hadron duality at small and intermediate time distances and on the two-pion contributions in a finite box at larger time distances. After extrapolation to the physical pion point and to the continuum limit we obtain aμHVP(ud)=619.0 (17.8)⋅10−10a_\mu^{\rm HVP}(ud) = 619.0~(17.8) \cdot 10^{-10}. Adding the contribution of strange and charm quarks, obtained by ETMC, and an estimate of the isospin-breaking corrections and quark-disconnected diagrams from the literature we get aμHVP(udsc)=683 (19)⋅10−10a_\mu^{\rm HVP}(udsc) = 683~(19) \cdot 10^{-10}, which is consistent with recent results based on dispersive analyses of the experimental cross section data for e+e−e^+ e^- annihilation into hadrons. Using our analytic representation of the vector correlator, taken at the physical pion mass in the continuum and infinite volume limits, we provide the first eleven moments of the polarization function and we compare them with recent results of the dispersive analysis of the π+π−\pi^+ \pi^- channels. We estimate also the light-quark contribution to the missing part of aμHVPa_\mu^{\rm HVP} not covered in the MUonE experiment.Comment: 34 pages, 20 figures, 7 tables. Version to appear in PR

    Electromagnetic and strong isospin-breaking corrections to the muon g−2g - 2 from Lattice QCD+QED

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    We present a lattice calculation of the leading-order electromagnetic and strong isospin-breaking corrections to the hadronic vacuum polarization (HVP) contribution to the anomalous magnetic moment of the muon. We employ the gauge configurations generated by the European Twisted Mass Collaboration (ETMC) with Nf=2+1+1N_f = 2+1+1 dynamical quarks at three values of the lattice spacing (a≃0.062,0.082,0.089a \simeq 0.062, 0.082, 0.089 fm) with pion masses between ≃210\simeq 210 and ≃450\simeq 450 MeV. The results are obtained adopting the RM123 approach in the quenched-QED approximation, which neglects the charges of the sea quarks. Quark disconnected diagrams are not included. After the extrapolations to the physical pion mass and to the continuum and infinite-volume limits the contributions of the light, strange and charm quarks are respectively equal to δaμHVP(ud)=7.1 (2.5)⋅10−10\delta a_\mu^{\rm HVP}(ud) = 7.1 ~ (2.5) \cdot 10^{-10}, δaμHVP(s)=−0.0053 (33)⋅10−10\delta a_\mu^{\rm HVP}(s) = -0.0053 ~ (33) \cdot 10^{-10} and δaμHVP(c)=0.0182 (36)⋅10−10\delta a_\mu^{\rm HVP}(c) = 0.0182 ~ (36) \cdot 10^{-10}. At leading order in αem\alpha_{em} and (md−mu)/ΛQCD(m_d - m_u) / \Lambda_{QCD} we obtain δaμHVP(udsc)=7.1 (2.9)⋅10−10\delta a_\mu^{\rm HVP}(udsc) = 7.1 ~ (2.9) \cdot 10^{-10}, which is currently the most accurate determination of the isospin-breaking corrections to aμHVPa_\mu^{\rm HVP}.Comment: 23 pages, 7 figures, 5 tables. Version to appear in PRD. A bug in the update of the strange and charm contributions is removed and an extended discussion on the identification of the ground-state is included. arXiv admin note: text overlap with arXiv:1808.00887, arXiv:1707.0301

    Lattice study of semileptonic form factors with twisted boundary conditions

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    We apply twisted boundary conditions to lattice QCD simulations of three-point correlation functions in order to access spatial components of hadronic momenta different from the integer multiples of 2 pi / L. We calculate the vector and scalar form factors relevant to the K -> pi semileptonic decay and consider all the possible ways of twisting one of the quark lines in the three-point functions. We show that the momentum shift produced by the twisted boundary conditions does not introduce any additional noise and easily allows to determine within a few percent statistical accuracy the form factors at quite small values of the four-momentum transfer, which are not accessible when periodic boundary conditions are considered. The use of twisted boundary conditions turns out to be crucial for a precise determination of the form factor at zero-momentum transfer, when a precise lattice point sufficiently close to zero-momentum transfer is not accessible with periodic boundary conditions.Comment: latex 15 pages, 4 figures and 3 tables; modified intro and discussions of the results; version to appear in PR

    The nucleon Drell-Hearn-Gerasimov sum rule within a relativistic constituent quark model

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    The Drell-Hearn-Gerasimov sum rule for the nucleon is investigated within a relativistic constituent quark model formulated on the light-front. The contribution of the N - Delta(1232) transition is explicitly evaluated using different forms for the baryon wave functions and adopting a one-body relativistic current for the constituent quarks. It is shown that the N - Delta(1232) contribution to the sum rule is sharply sensitive to the introduction of anomalous magnetic moments for the constituent quarks, at variance with the findings of non-relativistic and relativized quark models. The experimental value of the isovector-isovector part of the sum rule is almost totally reproduced by the N - Delta(1232) contribution, when the values of the quark anomalous magnetic moments are fixed by fitting the experimental nucleon magnetic moments. Our results are almost independent of the adopted form of the baryon wave functions and only slightly sensitive to the violation of the angular condition caused by the use of a one-body current. The calculated average slope of the generalized sum rule around the photon point results to be only slightly negative at variance with recent predictions of relativized quark models
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