Black Holes in Einstein-scalar-Gauss-Bonnet model probed with scattering amplitudes
arXiv:2311.01756 · doi:10.1103/PhysRevD.110.046025
Abstract
We examined the quantum properties of scalar-tensor gravity with a coupling to the Gauss-Bonnet term in the low energy limit, exploring both linear and quadratic couplings. We calculated the leading-order corrections to the non-relativistic one-body gravitational potential and the metric by studying the gravitational field of a point-like scalar particle. We studied light-like scattering and compared it with the classical theory. We found that the non-minimal coupling does not contribute to the small-angle scattering for the quadratic coupling but does in the case of linear coupling. The results provide an opportunity to constrain the linear non-minimal coupling to the Gauss-Bonnet term with forthcoming observational data.
28 pages, 4 figures
References in corpus (9)
- Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models
- First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
- The Confrontation between General Relativity and Experiment
- The SAGEX Review on Scattering Amplitudes
- Post-Newtonian expansion for Gauss-Bonnet Gravity
- Scattering Amplitudes in Quantum Field Theory
- Graviton Bending in Quantum Gravity from One-Loop Amplitudes
- FeynGrav 2.0
- FeynMG: a FeynRules extension for scalar-tensor theories of gravity