Quasinormal modes and grey-body factors of axial gravitational perturbations of regular black holes in asymptotically safe gravity
This paper investigates the axial gravitational perturbations of regular black holes in asymptotically safe gravity by employing the Bernstein spectral method and asymptotic iteration method to compute quasinormal modes, revealing that while the fundamental mode remains largely unaffected by the deviation parameter, higher overtones exhibit significant deviations from the Schwarzschild case, alongside a strong agreement between grey-body factors and quasinormal modes for larger multipole numbers.