Light-Front Transverse Nucleon Charge and Magnetisation Densities
Z.-N. Xu, Z.-Q. Yao, P. Cheng, C. D. Roberts, J. Rodriguez-Quintero, J. Segovia

TL;DR
This paper calculates light-front transverse charge and magnetisation densities of nucleons using two models, revealing detailed flavor separation and polarization effects consistent with experimental data.
Contribution
It provides a comparative analysis of three-body and quark-diquark models to predict nucleon transverse densities, highlighting flavor-specific and polarization-dependent features.
Findings
Valence u- and d-quark Dirac radii are nearly identical.
d-quark Pauli radius is about 10% larger than u-quark.
Transverse charge densities shift in polarized nucleons, breaking rotational symmetry.
Abstract
Nucleon elastic electromagnetic form factors obtained using both the three-body and quark + fully-interacting-diquark pictures of nucleon structure are employed to calculate an array of light-front transverse densities for the proton and neutron and their dressed valence-quark constituents, viz. flavour separations of the proton and neutron results. These two complementary descriptions of nucleon structure deliver mutually compatible predictions, which match expectations based on modern parametrisations of available data, where such are available. Amongst other things, it is found that transverse-plane valence - and -quark Dirac radii are practically indistinguishable; but regarding kindred Pauli radii, the quark value is roughly 10% greater than that of the -quark. Moreover, magnetically, the valence quark is far more active than the valence quark, probably because…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsNuclear physics research studies · Quantum Chromodynamics and Particle Interactions · Pulsars and Gravitational Waves Research
