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Gravitational memory contributions to waveform and effective action

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arxiv 2410.10565 v2 pith:IVOQJDR2 submitted 2024-10-14 gr-qc

Gabriel Luz Almeida , Alan Müller , Stefano Foffa , Riccardo Sturani This is my paper · ORCID
classification gr-qc
keywords effectivegravitationalactionagreementbalanceradiationwaveformaffect
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We use Effective Field Theory techniques to derive the quadrupole-quadrupole part of the gravitational wave, obtaining a waveform in agreement with previous results found within the multipolar-post-Minkowskian method. In particular we emphasize the role of radiation-reaction terms, which affect the energy-momentum balance between source and radiation. An in-in effective action is then derived along the same principles and it is shown to provide energy and angular momentum balance equations in agreement with the corresponding fluxes carried at infinity by gravitational radiation.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Matching Tidal Deformability (Wilson) Coefficients to Black Hole Love Numbers in Higher-Curvature Gravity

    gr-qc 2026-04 accept novelty 7.0 of 10

    Wilson coefficients in higher-curvature EFTs equal point-particle counterterms plus finite-size Love-number pieces; standard GR matching fails and is corrected for cubic gravity.

  2. Local-in-Time Conservative Binary Dynamics at Fifth Post-Minkowskian and First Self-Force Orders

    hep-th 2025-06 conditional novelty 7.0 of 10

    The authors isolate the nonlocal tail part of the 5PM/1SF scattering angle and reconstruct a local-in-time Hamiltonian for generic bound orbits.

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