Extracting the three- and four-graviton vertices from binary pulsars and coalescing binaries
Umberto Cannella, Stefano Foffa, Michele Maggiore, Hillary Sanctuary, and Riccardo Sturani

TL;DR
This paper explores how measurements from binary pulsars and coalescing binaries can test the three- and four-graviton vertices predicted by General Relativity, using a Feynman graph-based post-Newtonian approach.
Contribution
It introduces a Feynman graph formulation of the post-Newtonian expansion to connect gravitational vertices with observable tests of GR, providing bounds from pulsar timing and lunar laser ranging.
Findings
Binary pulsar timing constrains three-graviton vertex deviations at 0.1%.
Lunar laser ranging bounds the three-graviton vertex at 0.02%.
Coalescing binaries cannot effectively constrain vertex deviations due to parameter degeneracies.
Abstract
Using a formulation of the post-Newtonian expansion in terms of Feynman graphs, we discuss how various tests of General Relativity (GR) can be translated into measurement of the three- and four-graviton vertices. In problems involving only the conservative dynamics of a system, a deviation of the three-graviton vertex from the GR prediction is equivalent, to lowest order, to the introduction of the parameter beta_{PPN} in the parametrized post-Newtonian formalism, and its strongest bound comes from lunar laser ranging, which measures it at the 0.02% level. Deviation of the three-graviton vertex from the GR prediction, however, also affects the radiative sector of the theory. We show that the timing of the Hulse-Taylor binary pulsar provides a bound on the deviation of the three-graviton vertex from the GR prediction at the 0.1% level. For coalescing binaries at interferometers we find…
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