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.
Recent Posts
The Geometry of Hamiltonian Monte Carlo
Applying symplectic geometry to understand and refine Hamiltonian MC.
Bumpy Black Holes in Alternative Theories of Gravity
Parametrizing deviations from purely GR, vacuum black holes.
Nonspinning Black Holes in Alternative Theories of Gravity
The deformation to spherically symmetric black holes under a class of corrections to general relativity.
Effective Gravitational Wave Stress-energy Tensor in Alternative Theories of Gravity
Computing how much energy and momentum gravitational waves carry in a very broad class of almost-GR theories.