Heavy quarkonia in a contact interaction and an algebraic model: mass spectrum, decay constants, charge radii and elastic and transition form factors

TL;DR

This paper models heavy quarkonia, specifically bottomonia, using a contact interaction within a symmetry-preserving framework to compute masses, decay constants, charge radii, and form factors, aligning well with experimental data.

Contribution

It extends previous charmonia studies to bottomonia using a Schwinger-Dyson equations approach with a contact interaction, providing comprehensive spectral and form factor predictions.

Findings

Masses of bottomonia states agree with experimental data.

Calculated decay constants and charge radii match existing models.

Form factor predictions offer new insights into heavy quarkonia structure.

Abstract

For the flavor-singlet heavy quark system of bottomonia, we compute the masses of the ground state mesons in four different channels, namely, pseudo-scalar ($\eta_{b}(1S)$), vector ($\Upsilon(1S)$), scalar ($\chi_{b_0}(1P)$) and axial vector ($\chi_{b_{1}}(1P)$). We also calculate the weak decay constants of the $\eta_{b}(1S)$ and $\Upsilon(1S)$ as well as the charge radius of $\eta_{b}(1S)$. It complements our previous study of the corresponding charmonia systems: $\eta_c(1S)$, $J/\Psi(1S)$, $\chi_{c_0}(1P)$) and ($\chi_{c_{1}}(1P)$). The unified formalism for this analysis is provided by a symmetry-preserving Schwinger-Dyson equations treatment of a vector$\times$vector contact interaction. Whenever a comparison is possible, our results are in fairly good agreement with experimental data and model calculations based upon Schwinger-Dyson and Bethe-Salpeter equations involving sophisticated interaction kernels. Within the same framework, we also report the elastic and transition form factors to two photons for the pseudo-scalar channels $\eta_{c}(1S)$ and $\eta_{b}(1S)$ in addition to the elastic form factors for the vector mesons $J/\Psi$ and $\Upsilon$ for a wide range of photon momentum transfer squared ($Q^2$). For $\eta_{c}(1S)$ and $\eta_{b}(1S)$, we also provide predictions of an algebraic model which correlates remarkably well between the known infrared and ultraviolet limits of these form factors.