6533b82afe1ef96bd128ca15

RESEARCH PRODUCT

Isovector and isoscalar meson cloud contributions to the nucleon electromagnetic form factors

R. TegenR. Tegen

subject

Quantum chromodynamicsPhysicsNuclear and High Energy PhysicsParticle physicsIsovectorMesonIsoscalarHadronForm factor (quantum field theory)Order (ring theory)Nucleon

description

We have calculated the nucleon form factors ${G}_{E,M}^{(p,n)}{(q}^{2})$ in the linear \ensuremath{\sigma} model to one-meson-loop order plus (two-loop) $\ensuremath{\gamma}\ensuremath{\pi}\ensuremath{\pi}\ensuremath{\pi}$ anomaly. The previously derived $\ensuremath{\gamma}\ensuremath{\pi}\ensuremath{\pi}\ensuremath{\pi}$ anomaly generally reduces the nucleon radii and produces a shift of the magnetic moments of order 0.1 ${\ensuremath{\mu}}_{N}$ or less. We present analytical results for ${G}_{E,M}^{p,n}(0)$ which display explicitly their dependence on hadron masses and coupling constants. Analytical results for the radii are also given and the chiral singularities they contain $(\mathrm{ln}{m}_{\ensuremath{\pi}}$ and ${m}_{\ensuremath{\pi}}^{\ensuremath{-}1})$ are exposed. These come from the $\ensuremath{\pi}\ensuremath{\pi}$ intermediate state contribution to the form factors and not from the chiral quark substructure of nucleons or mesons. The leading chiral singularity has a universal strength while the chiral log (next-to-leading singularity) picks up a model (or approximation) dependence in terms of ${g}_{A}$ and the threshold behavior of the $\ensuremath{\pi}N$ amplitude ${A}^{(\ensuremath{-})}(\ensuremath{\nu},0)$. The chiral singularities appear only in the isovector nucleon radii $〈{r}_{1,2}^{2}{〉}^{I=1}$, the leading ${m}_{\ensuremath{\pi}}^{\ensuremath{-}1}$ term appears only in $〈{r}_{2}^{2}{〉}^{I=1}$ due to a peculiar cancellation between two independent form factor combinations ${\ensuremath{\Gamma}}_{1,3}{(q}^{2})$. The isoscalar anomaly $\ensuremath{\gamma}\ensuremath{\pi}\ensuremath{\pi}\ensuremath{\pi}$ is finite for ${m}_{\ensuremath{\pi}}\ensuremath{\rightarrow}0$.

https://doi.org/10.1103/physrevc.57.329