Meson cloud contributions to baryon axial form factors
arXiv:1406.7633 · doi:10.1103/PhysRevD.91.034022
Abstract
The axial form factor as well as the axial charge of octet baryons are studied in the perturbative chiral quark model (PCQM) with the quark wave functions predetermined by fitting the theoretical results of the proton charge form factor to experimental data. The theoretical results are found, based on the predetermined quark wave functions, in good agreement with experimental data and lattice values. This may indicate that the electric charge and axial charge distributions of the constituent quarks are the same. The study reveals that the meson cloud plays an important role in the axial charge of octet baryons, contributing 30%-40% to the total values, and strange sea quarks have a considerable contribution to the axial charge of the and .
6 pages, 4 figures, 5 tables
References in corpus (11)
- Nucleon electromagnetic form factors
- First Calculation of Hyperon Axial Couplings from Lattice QCD
- Octet baryon electromagnetic form factors in nuclear medium
- Electromagnetic form factors of the baryon octet in the perturbative chiral quark model
- Nucleon Form Factors of the Isovector Axial-Vector Current: Situation of Experiments and Theory
- Axial charges of octet and decuplet baryons
- Covariant spectator quark model description of the transition
- Hyperon Axial Charges in Two-Flavor Chiral Perturbation Theory
- Chiral Corrections and the Axial Charge of the Delta
- Isovector axial-vector form factors of octet baryons in QCD
- Dependence of nucleon properties on pseudoscalar meson masses