activity
20032026
most citedNovel approach to binary dynamics: application to the fifth post-Newtonian level

152 citations · 2.5k across the 136 of their papers we have counts for

collaborators

141 papers

gr-qc2026

Binary black hole scattering in the extreme-mass-ratio limit: time-domain waveform

Andrea Geralico

The time-domain gravitational waveform emitted during the scattering of two nonspinning compact bodies is computed in the extreme-mass-ratio limit. It provides a time-domain descri…

gr-qc2026

Octupolar bremsstrahlung waveform up to the two-loop level and the third-and-a-half post-Newtonian accuracy

Donato Bini, Thibault Damour, Andrea Geralico

Extending our recent work (which focussed on the even-parity quadrupolar part of the waveform), we compute the even-parity octupolar contribution, , to the gravitational wavef…

gr-qc2026

Radiation-reaction driven dynamics at the third-and-a-half post-Newtonian order in different gauges

Donato Bini, Andrea Geralico, Sara Rufrano Aliberti

We consider the coordinate-dependent definition of the radiation-reaction force at the third-and-a-half post-Newtonian order for general orbits. In order to (partially) determine i…

gr-qc2026

Gravitational bremsstrahlung waveform at the eighth post-Minkowskian order in the extreme-mass-ratio limit

Andrea Geralico

The gravitational waveform generated by the scattering of two nonspinning bodies is computed in the frequency domain in the extreme-mass-ratio limit at the eighth post-Minkowskian…

gr-qc2026

Radiated Energy Spectrum, Radiated Angular Distribution and Non-linear Memory from the One-loop Gravitational Bremsstrahlung Waveform

Donato Bini, Thibault Damour, Stefano De Angelis +1

The frequency-domain gravitational waveform emitted by the scattering of two non-spinning massive particles has recently been derived at next-to-leading, \textit{i.e.} one-loop, po…

gr-qc2026

Quadrupolar bremsstrahlung waveform at the third-and-a-half post-Newtonian accuracy

Donato Bini, Thibault Damour, Andrea Geralico

We study the quadrupolar part of the gravitational waveform (encoded in the helicity-( radiative quadrupole moment $U_2 = \frac{1}{2!} \bar m^{i} \bar m^{j } U_{i j}…