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

Abstract

Extending our recent work (which focussed on the even-parity quadrupolar part of the waveform), we compute the even-parity octupolar contribution, U3, to the gravitational waveform W ≡ (c4 r)/4G m̅i m̅j hi j emitted during the scattering of two masses. We work within the Multipolar Post-Minkowskian (MPM) formalism, and use the 3.5 Post-Newtonian (PN) accurate radiation-reacted quasi-Keplerian representation of the hyperbolic motion. We explicitly evaluate the frequency-domain value Û3(ω, θ,ϕ) of U3 up to the 2-loop level, i.e. $ O(G^4)$ contributions to hij(ω, θ,ϕ), corresponding to O(G3) contributions to Û3(ω, θ,ϕ). As a crucial partial confirmation of our result, we find that the 1-loop truncation of our 3.5 PN frequency-domain MPM waveform agrees with corresponding existing Effective Field Theory (EFT) results when taking into account exactly the {\it same} (2.5PN-level) difference in the definitions of the center-of-mass origins within the two formalisms that was deduced from our previous quadrupolar comparison.

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BibTeX
@misc{bini2026octupolar,
  title = {{Octupolar bremsstrahlung waveform up to the two-loop level and the third-and-a-half post-Newtonian accuracy}},
  author = {Donato Bini and Thibault Damour and Andrea Geralico},
  howpublished = {HAL},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2609.11835},
  eprint = {2609.11835},
  archivePrefix = {arXiv},
  url = {https://hal.science/hal-05761200v1},
}
RIS
TY  - UNPB
TI  - Octupolar bremsstrahlung waveform up to the two-loop level and the third-and-a-half post-Newtonian accuracy
AU  - Donato Bini
AU  - Thibault Damour
AU  - Andrea Geralico
PY  - 2026
DA  - 2026/09/10
PB  - HAL
DO  - 10.48550/arxiv.2609.11835
UR  - https://hal.science/hal-05761200v1
AB  - Extending our recent work (which focussed on the even-parity quadrupolar part of the waveform), we compute the even-parity octupolar contribution, U_3, to the gravitational waveform W ≡ (c^4 r)/4G m̅^i m̅^j  h_i j emitted during the scattering of two masses. We work within the Multipolar Post-Minkowskian (MPM) formalism, and use the 3.5 Post-Newtonian (PN) accurate radiation-reacted quasi-Keplerian representation of the hyperbolic motion. We explicitly evaluate the frequency-domain value Û_3(ω, θ,ϕ) of U_3 up to the 2-loop level, i.e. $ O(G^4)$ contributions to h_ij(ω, θ,ϕ), corresponding to O(G^3) contributions to Û_3(ω, θ,ϕ). As a crucial partial confirmation of our result, we find that the 1-loop truncation of our 3.5 PN frequency-domain MPM waveform agrees with corresponding existing Effective Field Theory (EFT) results when taking into account exactly the {\it same} (2.5PN-level) difference in the definitions of the center-of-mass origins within the two formalisms that was deduced from our previous quadrupolar comparison.
ER  -