Abstract

In the partonic (or light-front) description of relativistic systems the electromagnetic form factors are expressed in terms of frame-independent charge and magnetization densities in transverse space. This formulation allows one to identify the chiral components of nucleon structure as the peripheral densities at transverse distances b = O(M_pi^{-1}) and compute them in a parametrically controlled manner. A dispersion relation connects the large-distance behavior of the transverse charge and magnetization densities to the spectral functions of the Dirac and Pauli form factors near the two-pion threshold at timelike t = 4 M_pi^2. Using relativistic chiral effective field theory in the leading-order approximation, we (a) derive the asymptotic behavior (Yukawa tail) of the isovector transverse densities in the "chiral" region b = O(M_pi^{-1}) and the "molecular" region b = O(M_N^2/M_pi^3); (b) perform the heavy-baryon expansion; (c) explain the relative magnitude of the peripheral charge and magnetization densities in a simple mechanical picture; (d) include Delta intermediate states and study the densities in the large-N_c limit of QCD; (e) quantify the spatial region where the chiral components are numerically dominant; (f) calculate the chiral divergences of the b^2-weighted moments of the transverse densities (charge and magnetic radii) and determine their spatial support. Our approach provides a concise formulation of the spatial structure of the nucleon's chiral component and offers new insights into basic properties of the chiral expansion. It relates the information extracted from low-t elastic form factors to the generalized parton distributions probed in peripheral high-energy scattering processes.

Highlights

  • Understanding the spatial structure of hadrons and their interactions is one of the main objectives of modern strong interaction physics

  • It is important to realize that the light-front formulation of relativistic dynamics can be used when describing hadron structure in terms of the fundamental theory of QCD, and in effective theories based on hadronic degrees of freedom

  • We describe the dispersion representation of the transverse densities and its usage, discuss the behavior of the spectral functions near threshold based on general principles, and introduce the parametric regions of transverse distances

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Summary

Introduction

Understanding the spatial structure of hadrons and their interactions is one of the main objectives of modern strong interaction physics. In this formulation the densities are expressed as overlap integrals of the peripheral πN light-cone wave functions of the physical nucleon, which are calculable directly from the chiral Lagrangian This formulation will reveal several new aspects, such as the role of orbital angular momentum in chiral counting, the longitudinal structure of the configurations contributing to the densities at given b, and the connection with chiral contributions to the nucleon’s parton densities and high-energy scattering processes. Higher-order calculations of the spectral functions of the nucleon form factors have been performed in relativistic [31] and heavy-baryon chiral EFT [29, 32] and could be adapted for our purposes This extension, requires new physical considerations regarding the regularization of chiral loops in coordinate space and will be left to a future study

Definition and interpretation
Dispersion representation
Spectral functions near threshold
Parametric regions of transverse distance
Two-pion spectral functions
Chiral component of transverse densities
Heavy-baryon expansion
Contact terms and pseudoscalar πN coupling
Delta isobar and large-Nc limit
N only
Transverse densities in large-Nc QCD
Two-pion component in large-Nc limit
Spectral functions from vector mesons
Mπ2 ρ pole t
Moments of transverse densities
Chiral divergence of moments
Summary and outlook
Methodological aspects
Experimental tests
A Cutting rule for t-channel discontinuity
Findings
B Dispersion integral in heavy-baryon expansion
Full Text
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