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Classroom Contents
Testing General Relativity with Gravitational Waves - Black Holes as Perfect Laboratories
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- 1 Intro
- 2 Uniqueness: the Kerr solution
- 3 Singularities & Censorship
- 4 Energy source?
- 5 The simplicity slide: BHs as perfect laboratories
- 6 Fundamental questions
- 7 I. Inspiralling compact objects
- 8 Parametrized tests
- 9 Challenges
- 10 II. Spectroscopy: testing the Kerr nature
- 11 When is a linear ringdown description valid?
- 12 One and two-mode estimates: the start of spectroscopy
- 13 Addenda i. Nonlinearities in ringdown?
- 14 Addenda ii. Spectral stability
- 15 Addenda iii. Environmental effects
- 16 Particle detectors in the sky: dark matter II
- 17 Fundamental fields: particle detectors in the sky
- 18 Bounding the boson mass with EM observations
- 19 Wonderful sources for different detectors
- 20 Constraints on fundamental fields via superradiance
- 21 Couplings to Standard Model
