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Nonlinear Gravitational Memory in the Post-Minkowskian Expansion
Alessandro Georgoudis1, Vasco Goncalves2, Carlo Heissenberg3
1Queen Mary University of London, Centre for Theoretical Physics, Department of Physics and Astronomy, Mile End Road, London E1 4NS, United Kingdom.
This study computes the nonlinear gravitational memory waveform for compact object scattering using a novel amplitude-based method. This provides a crucial benchmark for gravitational wave research.
Area of Science:
- Gravitational Wave Physics
- General Relativity
- High-Energy Astrophysics
Background:
- The gravitational memory effect is a crucial prediction of general relativity, representing a permanent distortion of spacetime after a gravitational wave event.
- Previous calculations of the nonlinear gravitational memory waveform have been limited in scope or computational approach.
Purpose of the Study:
- To compute the leading-order nonlinear gravitational memory waveform for the scattering of two compact objects within the post-Minkowskian expansion.
- To utilize a scattering-amplitude-based approach to naturally incorporate the nonlinear memory as a soft graviton contribution.
Main Methods:
- Employing a scattering-amplitude-based representation of the gravitational waveform.
- Applying multipolar decomposition to the waveform.
- Utilizing the reverse unitarity method for exact-in-velocity predictions.
Main Results:
- The first computation of the nonlinear gravitational memory waveform for compact object scattering at leading order in the post-Minkowskian expansion.
- Explicit exact-in-velocity predictions derived from the reverse unitarity method.
- Validation of results through agreement with velocity-expanded post-Newtonian multipoles.
Conclusions:
- The study successfully computes the gauge-invariant, nonanalytic-in-frequency part of the O(G^{3}) multipolar waveform.
- The findings provide a valuable benchmark for future theoretical and observational studies of gravitational waves and compact object mergers.
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