Omega Meson Cloud and the Proton's Light Anti-Quark Distribution
arXiv:hep-ph/9907417 · doi:10.1016/S0370-2693(99)01419-7
Abstract
We use the meson cloud model of the nucleon to calculate distribution functions for and in the proton. Including the effect of the omega meson cloud, with a coupling constant , allows a reasonably good description of the data.
6 pages, 2 figures, LaTex
References in corpus (6)
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Cited by in corpus (19)
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- The quark - antiquark asymmetry of the strange sea of the nucleon
- Nucleon sea in the effective chiral quark model
- Chiral Light Front Perturbation Theory and the Flavor Dependence of the Light-Quark Nucleon Sea
- Parton Distribution of Proton in a Simple Statistical Model
- Sea quark contents of octet baryons
- Quark sea asymmetries of the octet baryons
- Collinear parton distributions and the structure of the nucleon sea in a light-front meson-cloud model
- Parton distributions in the proton and pion
- Sigma Meson Cloud and Proton's Light Flavor Sea Quarks
- Nucleon structure functions and longitudinal spin asymmetries in the chiral quark constituent model
- Sea Quark Flavor Asymmetry of Hadrons in Statistical Balance Model
- Quark flavor distribution functions for the octet baryons in the chiral quark constituent model
- Pion-Exchange and Fermi-Motion Effects on the Proton-Deuteron Drell-Yan Process
- Electromagnetic and Axial-Vector Form Factors of the Quarks and Nucleon
- Multi-quark components in baryons
- Coordinate Space Distributions of Antiquark Flavor Asymmetries in the Proton