Three-Hair Newtonian Relations for Rotating Stars
Universal relations between the Newtonian multipole moments of rotating stars.
Recent Posts
Parametrizing and Constraining Scalar Corrections to General Relativity
Connecting observables (pulsar binary pericenter precession and gravitational wave phase) to the parameters and structure of theoretical models.
Isolated and Binary Neutron Stars in Dynamical Chern-Simons Gravity
Chern-Simons corrections to 1) internal structure (including mass shift) and 2) binary dynamics (including pericenter precession) of neutron stars.
Probes of Strong-field Gravity (PhD Thesis) External link
MIT PhD thesis of Leo C. Stein
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.