The HADES seminar on Tuesday, April 7th, will be at 3:30pm in Room 740.
Speaker: Tyler Guo
Abstract: Quasi-normal modes (QNM) of black holes are supposed to describe the ringdown of decaying gravitational waves. This ringdown is dominated by the modes closest to the real axis but the overdamped modes (deeper in the complex) remain of interest to physicists and mathematicians.
In this talk, I will give a rigorous definition of QNM as scattering resonances. I will then explain how, in the Schwarzschild case, the problem of finding QNM can be reduced to a study of eigenvalues of a family of non-self-adjoint 1D operators using the method of complex scaling. To explain the structure of the resulting spectral problems I will consider the simpler self-adjoint case and give a proof of the emergence of Bohr–Sommerfeld quantisation rules. If time permits, I will discuss the modifications needed to treat the non-self-adjoint case.