Mechanical properties of the $\Omega^-$ baryon from gravitational form factors
Zeinab Dehghan, K. Azizi

TL;DR
This paper analyzes the gravitational form factors of the $^-$ baryon using QCD sum rules to reveal its internal mechanical structure, including energy, pressure, and shear distributions, providing new insights into spin-3/2 hadrons.
Contribution
First determination of mechanical radii and quadrupole contributions to the pressure and shear force distributions of the $^-$ baryon using gravitational form factors.
Findings
Quadrupole contributions are generally subdominant to monopole components.
Mechanical radii and D-terms are extracted for the first time.
The internal force distributions support the mechanical stability of the $^-$ baryon.
Abstract
We present a comprehensive investigation of the mechanical properties of the baryon by analyzing its gravitational form factors (GFFs) within the framework of QCD sum rules. These form factors encode rich information about the internal structure of hadrons and offer deep insights into the dynamics that govern their stability. The spin-3/2 nature of the baryon manifests in its gravitational form factors as intricate multipole structures, which encapsulate higher-order deformations and demonstrate the influence of intrinsic spin on internal dynamics. We extract the GFFs of the baryon and apply their specific multipole combinations, gravitational multipole form factors (GMFFs), to quantify key mechanical observables-including energy density, angular momentum, pressure and shear force distributions, mass and mechanical radii, and D-terms-associated with…
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Taxonomy
TopicsQuantum Chromodynamics and Particle Interactions · High-Energy Particle Collisions Research · Pulsars and Gravitational Waves Research
