Relativity and gravitational theory Definition
Gravitational radiation reaction
Builds on Post-Newtonian expansionQuadrupole formulaGravitational wave
Definition
Consider a slowly moving, weakly self-gravitating source of mass density and reduced quadrupole moment , as in the quadrupole formula. Consider the post-Newtonian expansion of the equations of motion of the source. The gravitational radiation reaction is the leading part of the force that is odd under time reversal. It appears at order relative to the Newtonian force. In Burke–Thorne gauge it is given by the potential with summation over , which adds the force density to the Newtonian equations.
Remarks
The work done by this force on the source is , using the continuity equation. After integration by parts in time and averaging over several periods it equals . This is minus the power carried by the gravitational waves, so the energy balance holds.
Example: for two point masses on a circular orbit of separation , energy balance with gives So decreases linearly in time and the bodies collide after a finite time.
Non-example: the first post-Newtonian corrections to the force, at order , are even under time reversal. They are conservative, cause effects such as perihelion precession, and are not part of radiation reaction.
Reading path
To understand this page from the ground up, read these 5 pages in order. The foundations come first.
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- no evidence level
- Gravitational wave concept
- Linearized gravity concept
- Post-Newtonian expansion concept
- Quadrupole formula statement
- Gravitational radiation reaction definition
Further reading
About this page
| Tag | 7QPQ1AHD5H |
|---|---|
| URI | m2://7QPQ1AHD5H |
| Kind | definition |
| Writing | W0 stub |
| MSC | 83C35, 83C10, 83C25 |
| Defines | Gravitational radiation reaction |
| Uses | Post-Newtonian expansion, Quadrupole formula, Gravitational wave |
| Changed | 3 November 2026 |
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