## Post-Newtonian, Quasicircular Binary Inspirals in Quadratic Modified Gravity

The post-Newtonian calculation scheme applied to binary inspirals in a broad class of almost-GR theories.

The post-Newtonian calculation scheme applied to binary inspirals in a broad class of almost-GR theories.

Applying symplectic geometry to understand and refine Hamiltonian MC.

Parametrizing deviations from purely GR, vacuum black holes.

The deformation to spherically symmetric black holes under a class of corrections to general relativity.

Computing how much energy and momentum gravitational waves carry in a very broad class of almost-GR theories.