Abstract
We study one loop quantum gravitational corrections to the long range force induced by the exchange of a massless scalar between two massive scalars. The various diagrams contributing to the flat space matrix are evaluated in a general covariant gauge, and we show that dependence on the gauge parameters cancels at a point considerably before forming the full matrix, which is unobservable in cosmology. It is possible to interpret our computation as a solution to the effective field equations—which could be done even in cosmology—but taking account of quantum gravitational corrections from the source and from the observer.
- Received 22 August 2017
DOI:https://doi.org/10.1103/PhysRevD.96.104029
© 2017 American Physical Society