Testing General Relativity with Gravitational Waves - Black Holes as Perfect Laboratories
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Overview
Syllabus
Intro
Uniqueness: the Kerr solution
Singularities & Censorship
Energy source?
The simplicity slide: BHs as perfect laboratories
Fundamental questions
I. Inspiralling compact objects
Parametrized tests
Challenges
II. Spectroscopy: testing the Kerr nature
When is a linear ringdown description valid?
One and two-mode estimates: the start of spectroscopy
Addenda i. Nonlinearities in ringdown?
Addenda ii. Spectral stability
Addenda iii. Environmental effects
Particle detectors in the sky: dark matter II
Fundamental fields: particle detectors in the sky
Bounding the boson mass with EM observations
Wonderful sources for different detectors
Constraints on fundamental fields via superradiance
Couplings to Standard Model
Taught by
Harvard CMSA