Baryon transition form factors at the pole
L. Tiator, M. D\"oring, R. L. Workman, M. Had\v{z}imehmedovi\'c, H., Osmanovi\'c, R. Omerovi\'c, J. Stahov, A. \v{S}varc

TL;DR
This paper discusses the definition of baryon transition form factors at the resonance pole, compares different form factor relations, and analyzes experimental data to extract and compare these form factors at various energy scales.
Contribution
It generalizes the relations for nucleon to baryon transition form factors to virtual photons and compares form factors at Breit-Wigner and pole positions using experimental data.
Findings
Form factors differ between Breit-Wigner and pole positions.
The $G_M$, $G_E$, and $G_C$ form factors are analyzed up to $Q^2=5$ GeV$^2$.
Ratios $E/M$ and $S/M$ are studied as functions of $Q^2$.
Abstract
Electromagnetic resonance properties are uniquely defined at the pole and do not depend on the separation of the resonance from background or the decay channel. Photon-nucleon branching ratios are nowadays often quoted at the pole, and we generalize the considerations to the case of virtual photons. We derive and compare relations for nucleon to baryon transition form factors both for the Breit-Wigner and the pole positions. Using the MAID2007 and SAID SM08 partial wave analyses of pion electroproduction data, we compare the , , and form factors for the resonance excitation at the Breit-Wigner resonance and pole positions up to GeV. We also explore the and ratios as functions of . For pole and residue extraction, we apply the Laurent + Pietarinen method.
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