The nucleon as a test case to calculate vector-isovector form factors at low energies
Stefan Leupold (UU)

TL;DR
This paper uses dispersion theory and chiral perturbation theory to calculate nucleon vector-isovector form factors at low energies, highlighting the importance of including Delta baryons for accurate results.
Contribution
It extends hyperon form factor methods to nucleons, comparing two pion rescattering approaches and emphasizing the necessity of Delta baryons in the calculations.
Findings
Including Delta baryons yields more reasonable form factor results.
Adjusting low-energy constants improves agreement with Roy-Steiner equations.
Different rescattering methods produce significantly different results.
Abstract
Extending a recent suggestion for hyperon form factors to the nucleon case, dispersion theory is used to relate the low-energy vector-isovector form factors of the nucleon to the pion vector form factor. The additionally required input, i.e. the pion-nucleon scattering amplitudes are determined from relativistic next-to-leading-order (NLO) baryon chiral perturbation theory including the nucleons and optionally the Delta baryons. Two methods how to include pion rescattering are compared: (a) solving the Muskhelishvili-Omnes (MO) equation and (b) using an N/D approach. It turns out that the results differ strongly from each other. Furthermore the results are compared to a fully dispersive calculation of the (subthreshold) pion-nucleon amplitudes based on Roy-Steiner (RS) equations. In full agreement with the findings from the hyperon sector it turns out that the inclusion of Delta baryons…
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