A bstract Using a heavy-mass effective field theory (HEFT), we study gravitational-wave
emission in the scattering of two spinless black holes or neutron stars of arbitrary masses at …

We describe a systematic framework for computing the conservative potential of a compact
binary system using modern tools from scattering amplitudes and effective field theory. Our …

Using the recently established formalism of a worldline quantum field theory description of
the classical scattering of two spinless black holes, we compute the far-field time-domain …

Using the spinning worldline quantum field theory formalism we calculate the quadratic-in-
spin momentum impulse Δ pi μ and spin kick Δ ai μ from a scattering of two arbitrarily …

The recently established formalism of a worldline quantum field theory, which describes the
classical scattering of massive bodies (black holes, neutron stars, or stars) in Einstein …

A bstract Picture yourself in the wave zone of a gravitational scattering event of two massive,
spinning compact bodies (black holes, neutron stars or stars). We show that this system of …

A bstract We introduce a—somewhat holographic—dictionary between gravitational
observables for scattering processes (measured at the boundary) and adiabatic invariants …

A bstract We develop an Effective Field Theory (EFT) formalism to solve for the conservative
dynamics of binary systems in gravity via Post-Minkowskian (PM) scattering data. Our …

A bstract We continue to investigate correspondences between, on the one hand, scattering
amplitudes for massive higher-spin particles and gravitons in appropriate quantum-to …

We develop a general formalism for computing classical observables for relativistic
scattering of spinning particles, directly from on-shell amplitudes. We then apply this …