Journal article

Publication year: 2016

Journal: Physical Review D

Volume number: 93

Issue number: 3

ISSN: 2470-0010

eISSN: 2470-0029

Open access status: Green

DOI Link: https://doi.org/10.1103/PhysRevD.93.033004

Publisher: American Physical Society

Abstract: 
The Delta(1232) -> gamma*N magnetic dipole form factor (G*(M)) 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 parametrized 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 -> gamma N transition, the Dalitz decay (Delta -> e(+)e(-)N), and the Delta mass distribution function. The impact of the model on dilepton spectra in pp collisions is also discussed.

Harvard Citation style: Ramalho, G., Pena, M., Weil, J., van Hees, H. and Mosel, U. (2016) Role of the pion electromagnetic form factor in the Δ(1232) → γ*N timelike transition, Physical Review D, 93(3), Article 033004. https://doi.org/10.1103/PhysRevD.93.033004

APA Citation style: Ramalho, G., Pena, M., Weil, J., van Hees, H., & Mosel, U. (2016). Role of the pion electromagnetic form factor in the Δ(1232) → γ*N timelike transition. Physical Review D. 93(3), Article 033004. https://doi.org/10.1103/PhysRevD.93.033004