Gravitational form factors of the proton in the improved holographic QCD model
Antti Hippeläinen, Niko Jokela, Matti Järvinen
TL;DR
The paper analyzes the gluonic contributions to the proton's gravitational form factors within the improved holographic QCD framework, modeling the proton as bulk Dirac fermions and extracting the form factors $\mathcal{A}(t)$ and $\mathcal{D}(t)$ from holographic couplings to metric fluctuations. By fitting $\mathcal{A}(t)$ to lattice data, the authors predict $\mathcal{D}(t)$, uncovering an infrared pole in the forward limit but showing that observable mechanical properties remain finite due to cancellations. Using these form factors, they derive the proton's mechanical structure, computing pressure and shear distributions and two radii, $\rho_{\text{mech}}$ and $\rho_{\text{mass}}$, finding $\rho_{\text{mech}} = 0.95$ fm and $\rho_{\text{mass}} = 0.61$ fm, in line with nonperturbative studies. The work illustrates how holographic methods yield nonperturbative insights into gluonic observables and motivates extensions to include quark degrees of freedom and connections to generalized parton distributions.
Abstract
We compute the gluonic contribution to the gravitational form factors of the proton using the improved holographic QCD model, in which the proton is described in terms of bulk Dirac fermions. Model parameters are constrained using lattice and phenomenological input, allowing us to obtain estimates for the gravitational form factors and to compare them with results from other approaches. The resulting $\mathcal{D}(t)$ form factor is found to exhibit an infrared pole in our framework. Using the extracted form factors, we analyze mechanical properties of the proton, including pressure and shear distributions. We obtain estimates of $ρ_\text{mech} = 0.95$ fm and $ρ_\text{mass} = 0.61$ fm for the mechanical and the mass radii of the proton, respectively, which are similar to values in other nonperturbative studies.
