High-Precision Ringdown Surrogate Model for Non-Precessing Binary Black Holes<\/p>\n\n\n\n
arXiv:2408.05300<\/a><\/p>\n\n\n\n Adding higher-order spherical harmonics in non-spinning eccentric binary black hole merger waveform models<\/p>\n\n\n\n arXiv:2408.02762<\/a><\/p>\n\n\n\n Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity<\/p>\n\n\n\n arXiv:2407.18319<\/a><\/p>\n\n\n\n Gravitational waves from black hole emission<\/p>\n\n\n\n arXiv:2407.16989<\/a><\/p>\n\n\n\n Non-Axisymmetric Gravitational “Hair” for Extremal Black Holes<\/p>\n\n\n\n arXiv:2407.06926<\/a><\/p>\n\n\n\n Phenomenology and origin of late-time tails in eccentric binary black hole mergers<\/p>\n\n\n\n arXiv:2407.04682<\/a><\/p>\n\n\n\n Testing eccentric corrections to the radiation-reaction force in the test-mass limit of effective-one-body models<\/p>\n\n\n\n arXiv:2405.19006<\/a><\/p>\n\n\n\n Optimizing post-Newtonian parameters and fixing the BMS frame for numerical-relativity waveform hybridizations<\/p>\n\n\n\n arXiv:2403.10278<\/a><\/p>\n\n\n\n Real-time gravitational-wave inference for binary neutron stars using machine learning<\/p>\n\n\n\n arXiv:2407.09602<\/a><\/p>\n\n\n\n Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA<\/p>\n\n\n\n