Abstract
We compute the variation of the Fokker-Wheeler-Feynman total linear and angular momentum of a
gravitationally interacting binary system under the second post-Minkowskian retarded dynamics. The
resulting OðG2Þ equations-of-motion-based, total change in the system's angular momentum is found to
agree with existing computations that assumed balance with angular momentum fluxes in the radiation zone.
Anno
2022
Autori IAC
Tipo pubblicazione
Altri Autori
Donato Bini, Thibault Damour
Editore
American Physical Society,
Rivista
Physical review. D. Particles, fields, gravitation, and cosmology (Online)