Omega Meson Cloud and the Proton's Light Anti-Quark Distribution
Mary Alberg (1, 2), Ernest M. Henley (1, 3), and Gerald A., Miller (1) ((1) University of Washington, (2) Seattle University, (3), Institute for Nuclear Theory)

TL;DR
This paper employs the meson cloud model, including omega mesons, to calculate and explain the proton's light anti-quark distributions, aligning well with experimental data.
Contribution
It introduces the omega meson cloud into the meson cloud model to improve the understanding of proton anti-quark asymmetries.
Findings
Omega meson cloud improves data fit
Calculations match observed anti-quark distributions
Supports meson cloud model validity
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.
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