R\^ole of the pion electromagnetic form factor in the $\Delta(1232) \to \gamma^\ast N$ timelike transition

TL;DR

This paper introduces a covariant model for the $\Delta(1232) o \gamma^* N$ transition form factor, incorporating pion cloud effects, and demonstrates improved predictions for timelike regions relevant to particle collisions.

Contribution

The paper presents a new covariant model that combines valence quark core and pion cloud contributions, improving timelike transition form factor predictions over previous models.

Findings

Model predicts a peak at the $ ho$ mass pole in the timelike region.

Improved agreement with experimental data for dilepton spectra.

Provides calculations for $\Delta o \gamma N$ and Dalitz decays.

Abstract

The $\Delta(1232) \to \gamma^\ast N$ magnetic dipole form factor ($G_M^\ast$) is described here within a new covariant model that combines the valence quark core together with the pion cloud contributions. The pion cloud term is parameterized by two terms: one connected to the pion electromagnetic form factor, the other to the photon interaction with intermediate baryon states. The model can be used in studies of pp and heavy ion collisions. In the timelike region this new model improves the results obtained with a constant form factor model fixed at its value at zero momentum transfer. At the same time, and in contrast to the Iachello model, this new model predicts a peak for the transition form factor at the expected position, i.e. at the $\rho$ mass pole. We calculate the decay of the $\Delta \to \gamma N$ transition, the Dalitz decay ($\Delta \to e^+ e^- N$), and the $\Delta$ mass distribution function. The impact of the model on dilepton spectra in pp collisions is also discussed.