Gravitational-wave generation beyond General Relativity
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If you have a question about this talk, please contact Scott Melville.
I will motivate why and how General Relativity can be classically
extended and how the generation of gravitational waves can be
modified. I will review how these differences can be perturbative or
non-perturbative according to the
specific theory under scrutiny, and show how non-linearities can
become important in the merger of
compact objects. I will discuss the future prospects of testing
General relativity with next generation interferometers
This talk is part of the Theoretical Physics Colloquium series.
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