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- W2897978978 abstract "Abstract This chapter begins by finding the field created by compact objects in the post-linear approximation of general relativity. The second quadrupole formula is then completely proven. Next, the chapter finds the equations of motion of the bodies in the field which they create to second order in the perturbations, assuming that their velocities are small. It shows that, to correctly describe the radiation reaction at 2.5 PN order, it will prove necessary to iterate Einstein equations a third time. This leads the discussion to the equations of motion, which generalize to order 1/c5 the EIH equations of order 1/c. Finally, the chapter studies the effect of the radiation reaction force on the sources, and shows that there is an energy balance at 2.5 PN order between the energy radiated to infinity and the mechanical energy lost by the system." @default.
- W2897978978 created "2018-10-26" @default.
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- W2897978978 date "2018-08-30" @default.
- W2897978978 modified "2023-09-24" @default.
- W2897978978 title "The two-body problem and radiative losses" @default.
- W2897978978 doi "https://doi.org/10.1093/oso/9780198786399.003.0055" @default.
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