Numerical relativity simulation of GW150914 beyond general relativity
The first astrophysically-relevant numerical simulation of merging black holes in a higher-curvature theory beyond GR.
The first astrophysically-relevant numerical simulation of merging black holes in a higher-curvature theory beyond GR.
The generalized harmonic formulation can be derived by adding a gauge-fixing term to the Einstein-Hilbert action
Interactive toy for understanding Poincaré sections and chaos
The dividing line between bound and plunging orbits is an algebraic variety
qnm is an open-source Python package for computing the Kerr quasinormal mode frequencies, angular separation constants, and spherical-spheroidal mixing coeff...