Title: Complete mode decomposition of Green’s functions and bouncing singularities
Speaker: Paolo Arnaudo
Based on: 2605.16489
Abstract: Quasinormal modes are the characteristic damped oscillations of black holes and are central to the theory of ringdown. However, the quasinormal mode expansion of the retarded Green’s function provides a convergent representation only in a late-time region. In this talk, I will describe how to complete this mode decomposition by including a set of Matsubara modes, which reconstruct the Green’s function in the earlier-time region where the quasinormal mode sum fails. The main focus will be the Schwarzschild case. I will show that the boundary of the quasinormal mode convergence region has a precise geometric origin. It is controlled by singularities of the Green’s function at complex times, produced by null geodesics that bounce from the black-hole singularity. These bouncing singularities determine the radius of convergence of the quasinormal mode sum and explain the otherwise mysterious bounce radius appearing in the complete mode decomposition.