Charged Black-Hole Binary Evolution at Second Post-Newtonian Order
Andrea Placidi, Elisa Grilli, Marta Orselli, Matteo Pegorin, Nicola Bartolo, Pierpaolo Mastrolia
TL;DR
This work extends the PN description of binary black holes to include electric charge at $2\mathrm{PN}$ order within an EFT framework. It delivers a complete conservative Lagrangian in harmonic coordinates, an ADM-type Hamiltonian with center-of-mass transformations, and gauge-invariant observables (binding energy, periastron advance, scattering angle), plus the leading $1.5\mathrm{PN}$ dissipative dipolar effects. The results reproduce known neutral GR limits, agree with recent post-Minkowskian Einstein–Maxwell findings, and establish a solid foundation for incorporating charge-physics into GW waveform models. The analysis sets the stage for future refinements including energy flux, extremal-charge regimes, and spin/finite-size effects relevant for gravitational-wave data analysis.
Abstract
We study the dynamics of electrically charged black-hole binaries and their gravitational-wave emission during the inspiral phase. Within the post-Newtonian framework, we derive the conservative and dissipative dynamics up to second order (2PN), combining Effective Field Theory and classical methods. We compute the NNLO conservative Lagrangian, LO dissipative effects in harmonic and Lorenz gauges, and provide the equations of motion, center-of-mass transformations, and the Lagrangian/Hamiltonian in ADM-type coordinates. We also obtain gauge-invariant expressions for the binding energy, periastron advance in quasi-circular orbits, and the scattering angle in unbound orbits. Our results extend previous analyses and are fully consistent with recent post-Minkowskian findings.
