Rapidly Rotating Black Holes in Dynamical Chern-Simons Gravity: Decoupling Limit Solutions and Breakdown
Numerical solutions for rapidly-rotating dCS black holes show where the weak-coupling expansion breaks down.
Recent Posts
Note on Legendre Decomposition of the Pontryagin Density in Kerr
Short note simplifying a calculation in the literature.
Three-Hair Newtonian Relations for Rotating Stars
Universal relations between the Newtonian multipole moments of rotating stars.
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.