Gravitational Waves, relativistic celestial mechanics and black hole physics
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Full text | |
Author(s): |
Adamo, Tim
;
Gonzo, Riccardo
;
Ilderton, Anton
Total Authors: 3
|
Document type: | Journal article |
Source: | Journal of High Energy Physics; v. N/A, n. 5, p. 54-pg., 2024-05-03. |
Abstract | |
With the aim of computing bound waveforms from scattering amplitudes, we explore gravitational two-body dynamics using the Schwinger-Dyson equations and Bethe-Salpeter recursion. We show that the tree-level scattering waveform admits a natural analytic continuation, in rapidity, to the bound waveform, which we confirm from an independent calculation, in the Post-Newtonian expansion, of the time-domain multipoles at large eccentricity. We demonstrate consistency of this scattering-to-bound map with the Damour-Deruelle prescription for orbital elements in the quasi-Keplerian parametrization (which enters into the evaluation of the multipoles) and with the analytic continuation, in the binding energy, of radiated energy and angular momentum at 3PM. (AU) | |
FAPESP's process: | 21/14335-0 - ICTP South American Institute for Fundamental Research: a regional center for Theoretical Physics |
Grantee: | Nathan Jacob Berkovits |
Support Opportunities: | Special Projects |