Confinement Phenomena in Topological Stars

TL;DR

This paper investigates how Quantum Chromodynamics (QCD) phenomena, especially confinement, influence the physics and spacetime structure of topological stars under extreme density conditions.

Contribution

It provides a novel analysis of QCD effects on the energy-momentum tensor in the context of topological stars, linking particle physics to astrophysical phenomena.

Findings

QCD effects significantly impact the energy-momentum tensor near topological stars

QCD confinement influences the spacetime fabric around these celestial bodies

Insights into the interplay between strong force physics and astrophysical environments

Abstract

Quantum Chromodynamics (QCD) is the fundamental theory describing the strong nuclear force and the interactions among quarks and gluons. Topological stars, characterized by extreme density conditions, offer a unique environment where QCD phenomena play a crucial role due to the confinement of fundamental particles. Understanding these phenomena is essential for unraveling the behavior and properties of these celestial bodies. In this study, we explore the implications of QCD within extreme density regimes, focusing on its contribution to the energy-momentum tensor ($T^{\mu\nu}_{\text{QCD}}$) within the framework of Quantum Chromodynamics. Our analysis sheds light on how these QCD effects influence the fabric of spacetime in the vicinity of topological stars, providing valuable insights into their underlying physics.