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1.
The charged current neutrino production of φ and D s + mesons is studied, using the data obtained with the SKAT bubble chamber exposed to the Serpukhov accelerator neutrino beam. It is found that the φ production occurs predominantly in the forward hemisphere of the hadronic c.m.s. (at x F > 0, x F being the Feynman variable), with the mean yield strongly exceeding the expected yield of directly produced φ mesons and varying from 〈n φ(x F s 0)〉 = (0.92 ± 0.34) × 10?2 at W > 2 GeV up to (1.23 ± 0.53) × 10?2 at W > 2.6 GeV and (1.44 ± 0.69) × 10?2 at W > 2.9 GeV, W being the invariant mass of the hadronic system. For the first time, the inclusive yield of leading D s + mesons carrying more than z = 0.85 of the current c-quark energy is estimated: 〈n D s + (z > 0.85, W > 2.9 GeV)〉 = (6.64 ± 1.91) × 10?2. It is shown that the shape of measured φ meson differential spectrum on xF is reproduced by that expected from the D s + φX decays. An indication was obtained that this expected spectrum underestimates the measured φ yield.  相似文献   

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The hyperfine splittings in heavy quarkonia are studied in a model-independent way using experimental data on dielectron widths. Relativistic correlations are taken into account together with the smearing of spin-spin interaction. The radius of smearing is fixed by known G/ψ−η c(1S), ψ(2S)−η c′(2S) splittings, which appears to be small, r ss ≅ 0.06 fm. Nevertheless, even with such a small radius, substantial suppression of hyperfine splittings (∼50%) is observed in bottomonium. For nS b states (n = 1, 2, ..., 6), our predicted splittings (in MeV) are 28, 12, 10, 5, 6, 3. For the 3S and 4S charmonium states, the splittings 16(2) and 12(4) MeV are obtained. The text was submitted by the authors in English.  相似文献   

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In this paper, we calculate the branching ratio and direct CP asymmetry parameter of B c ±D 0 K ± in the framework of a perturbative QCD approach based on k T factorization. Besides the usual factorizable diagrams, both nonfactorizable and annihilation type contributions are taken into account. We find that (a) the branching ratio is at the order of 10−5; (b) the tree annihilation diagrams and the penguin diagrams dominate the total contribution; and (c) the direct CP asymmetry is about 7%, which can be tested in the Large Hadron Collider beauty experiments (LHC-b) at CERN.  相似文献   

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We investigate the inclusive photoproduction of J/ψ mesons at HERA within the framework of the k T -factorization QCD approach. Our study is based on the color singlet model supplemented with the relevant off-shell matrix elements and the CCFM and KMR unintegrated gluon densities in a proton and in a photon. Both the direct and resolved photon contributions are taken into account. Our predictions are compared with the recent experimental data taken by the H1 and ZEUS collaborations. Special attention is put on the J/ψ polarization parameters λ and ν, which are sensitive to the production dynamics.  相似文献   

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We consider the π+π?π0γ final state in electron-positron annihilation at c.m.s. energies not far from the threshold. Both initial-and final-state radiations of the hard photon are considered, but without interference between them. The amplitude for the final-state radiation is obtained by using the effective Wess-Zumino-Witten Lagrangian for pion-photon interactions valid for low energies. In real experiments, energies are never so small that ρ and ω mesons would have a negligible effect. So a phenomenological Breit-Wigner factor is introduced in the final-state radiation amplitude to account for the vector mesons' influence. Using radiative 3π production amplitudes, a Monte Carlo event generator was developed which could be useful in experimental studies.  相似文献   

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The Mellin-Barnes representation is used to improve the theoretical estimate of mass corrections to the width of a light pseudoscalar meson decay into a lepton pair, Pl + l . The full resummation of the terms ln(m l 22)(m l 22) n and (m l 22) n to the decay amplitude is performed, where m l is the lepton mass and Λ ≈ m ρ is the characteristic scale of the P → γ*γ* form factor. The total effect of the mass corrections for the e + e channel is negligible and, for the μ+μchannel, its order is of a few percent. The text was submitted by the authors in English.  相似文献   

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In this article, we assume that there exist hidden charmed tetraquark states with spin–parity J P=1, and we calculate their masses with the QCD sum rules. The numerical result indicates that the masses of the vector hidden charmed tetraquark states are about M Z =(5.12±0.15) GeV or M Z =(5.16±0.16) GeV, which are inconsistent with the experimental data on the π + χ c1 invariant-mass distribution. The hidden charmed mesons Z 1, Z 2 or Z may be scalar hidden charmed tetraquark states, hadro-charmonium resonances or molecular states.  相似文献   

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The importance of taking into account the mixing of the heavy cascade baryons Ξ and Ξ′ that have new quantum numbers in analyzing their properties is shown. The Ono quark model is considered by way of example. The masses of the new baryons and the Ξ-Ξ′ mixing angles are obtained. The same approach is applied to the interpolating currents of these baryons within QCD sum rules.  相似文献   

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Om diagnostic is a good geometric method to differentiate one dark energy model from LCDM. We apply three different two-parameter equation of state ω σ (EOS) to Dilaton Dark energy (DDE) model and investigate the Om diagnostic for these cases. We obtain that DDE model can be easily distinguished from LCDM no matter which case is considered. We also investigate the influence of coupled parameter α on the evolutive behavior of Omz. According to the numerical result of Om, we get the current value of equation of state ω σ0=−0.939 which fits the observational data well.  相似文献   

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In a hydrodynamic model, we have studied J/ψ production in Au+Au/Cu+Cu collisions at RHIC energy, GeV. At the initial time, J/ψ’s are randomly distributed in the fluid. As the fluid evolves in time, the free streaming J/ψ’s are dissolved if the local fluid temperature exceeds a threshold temperature T J/ψ . Sequential melting of charmonium states (χ c , ψ and J/ψ), with melting temperatures , T J/ψ ≈2T c and feed-down fraction F≈0.3, explains the PHENIX data on the centrality dependence of J/ψ suppression in Au+Au collisions. J/ψ p T spectra and the nuclear modification factor in Au+Au collisions are also well explained in the model. The model however overpredicts the centrality dependence of J/ψ suppression in Cu+Cu collisions by 20–30%. The J/ψ p T spectra are underpredicted by 20–30%. The model predicts that in central Pb+Pb collisions at LHC energy,  GeV, J/ψ’s are suppressed by a factor of ∼10. The model predicted a J/ψ p T distribution in Pb+Pb collisions at LHC is similar to that in Au+Au collisions at RHIC.  相似文献   

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New relations between Borel QCD sum rules for the strong couplings of baryons to kaons are derived. It is shown that, on the basis of the sum rules for the coupling constants g πΣΣ and g πΣΛ, the corresponding sum rules can be directly obtained for the coupling constants g KYN and g KYΞ, Y = Σ,Λ. The values of these coupling constants are calculated in the fiducial interval 1.0 ≤ M 2 ≤ 1.4 GeV2 at t = ?1.  相似文献   

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The decay η′ → ηπ 0 π 0 is studied in the framework of isobar model. It is shown, that good agreement with the experiment is achieved if α 0- and σ-meson contributions are taken into account. The contribution of α 0-meson is dominant, but σ-meson is necessary to reproduce the form of the Dalitz plot. Instead of the usual Breit-Wigner form of σ-meson propagator we use parametrization of the ππ-amplitude, which satisfies analyticity, crossing, unitarity and chirality constraints. This amplitude has a pole in the complex plane, which corresponds to σ-meson and describe experimental data on ππ-scattering in K e4 decay.  相似文献   

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The possibility of describing experimental data on the astrophysical S factor for radiative proton capture on a 13C nucleus at energies in the range 0.03–0.8 MeV is considered within the potential cluster model involving forbidden states. It is shown that the energy dependence of this astrophysical S factor can be reasonably explained on the basis of the E1 transition to the 3 P 1-wave bound state of the 14N nucleus in the p 13C channel from the 3 S 1 wave of p 13C scattering in the resonance energy region around 0.55 MeV in the laboratory frame.  相似文献   

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