Speaker
Giorgio Di Russo
(Hangzhou Institute for Advanced Study)
Description
The renormalized angular momentum appearing in the time-honored Mano–Suzuki–Takasugi (MST) method, which is useful for solving the confluent Heun equation as an infinite expansion of hypergeometric functions, is a fundamental quantity that arises in almost every black hole perturbation theory context, such as quasi-normal mode computations, tidal Love numbers, and waveforms. The appearance of this quantity is discussed both in the MST and in the Seiberg–Witten approaches, and some recent post-Minkowskian resummation properties in the eikonal regime are also examined.
Author
Giorgio Di Russo
(Hangzhou Institute for Advanced Study)