Abstract
We compute the hereditary part of the third post-Newtonian accurate gravitational energy radiation from hyperbolic scatterings (and parabolic scatterings) of nonspinning compact objects. We employ large angular momentum () expansion, and compute it to the relative order (so the first 12 terms). For the parabolic scattering case, the exact solution is computed. At the end, the completely collected expression of the energy radiation up to the third post-Newtonian and from to order, is presented including the instantaneous contribution.
- Received 21 March 2022
- Accepted 26 April 2022
DOI:https://doi.org/10.1103/PhysRevD.105.104035
© 2022 American Physical Society
Physics Subject Headings (PhySH)
Gravitation, Cosmology & Astrophysics