activity
20102026
most citedPost-1-Newtonian tidal effects in the gravitational waveform from binary inspirals

344 citations · 2.8k across the 40 of their papers we have counts for

collaborators

40 papers

gr-qc2026

Generalized Carter & Rüdiger Constants of

Christopher de Firmian, Justin Vines

We consider the motion of a charged spinning test/probe particle -- governed by the Mathisson-Papapetrou-Dixon equations with generic, adiabatic, and conservative spin- and field-i…

gr-qc2024★ 1 cited

Post-Newtonian observables for aligned-spin binaries to sixth order in spin from gravitational self-force and Compton amplitudes

Yilber Fabian Bautista, Mohammed Khalil, Matteo Sergola +2

Accurate modeling of compact binaries is essential for gravitational-wave detection and parameter estimation, with spin being an important effect to include in waveform models. In…

gr-qc2023★ 2 cited

Dynamical Implications of the Kerr Multipole Moments for Spinning Black Holes

Trevor Scheopner, Justin Vines

Previously the linearized stress tensor of a stationary Kerr black hole has been used to determine some of the values of gravitational couplings for a spinning black hole to linear…

hep-th2023

Quantum Field Theory, Worldline Theory, and Spin Magnitude Change in Orbital Evolution

Zvi Bern, Dimitrios Kosmopoulos, Andres Luna +4

A previous paper~\cite{Bern:2022kto} identified a puzzle stemming from the amplitudes-based approach to spinning bodies in general relativity: additional Wilson coefficients appear…

gr-qc2023★ 21 cited

Generalized Carter constant for quadrupolar test bodies in Kerr spacetime

Geoffrey Compère, Adrien Druart, Justin Vines

We establish the existence of a deformation of the usual Carter constant which is conserved along the motion in a fixed Kerr background of a spinning test body possessing the spin-…

gr-qc2023★ 54 cited

Modeling horizon absorption in spinning binary black holes using effective worldline theory

M. V. S. Saketh, Jan Steinhoff, Justin Vines +1

The mass and spin of black holes (BHs) in binary systems may change due to the infall of gravitational-wave (GW) energy down the horizons. For spinning BHs, this effect enters at 2…