Astrophysical Signatures of Einstein-Skyrme Anti-de Sitter Black Holes: Epicyclic Frequencies and QPO Constraints
This paper investigates the geodesic motion and epicyclic oscillations of particles around Einstein-Skyrme Anti-de Sitter black holes, revealing a unique signature where the radial frequency overtakes the orbital frequency at large distances, and demonstrates through MCMC analysis of X-ray binary and galactic center QPO data that this model consistently fits observations with a Skyrme charge parameter of approximately 0.6.