A note on the absence of corrections to Newton's potential
arXiv:1911.10108 · doi:10.1103/PhysRevD.101.046011
Abstract
We consider Einstein gravity with the addition of and interactions in the context of effective field theory, and the corresponding scattering amplitudes of gravitons and minimally-coupled heavy scalars. First, we recover the known fact that graviton amplitudes are the same as in Einstein gravity. Then we show that all amplitudes with two heavy scalars and an arbitrary number of gravitons are also not affected by these interactions. We prove this by direct computations, using field redefinitions known from earlier applications in string theory, and with a combination of factorisation and power-counting arguments. Combined with unitarity, these results imply that, in an effective field theory approach, the Newtonian potential receives neither classical nor quantum corrections from terms quadratic in the curvature.
15 pages
References in corpus (5)
- Scattering Amplitudes and the Conservative Hamiltonian for Binary Systems at Third Post-Minkowskian Order
- Aspects of general higher-order gravities
- Structure of the MHV-rules Lagrangian
- Curvature-Squared Multiplets, Evanescent Effects and the U(1) Anomaly in N = 4 Supergravity
- Graviton Bending in Quantum Gravity from One-Loop Amplitudes
Cited by in corpus (15)
- Gravitational Bremsstrahlung and Hidden Supersymmetry of Spinning Bodies
- One-loop Gravitational Bremsstrahlung and Waveforms from a Heavy-Mass Effective Field Theory
- Eikonal phase matrix, deflection angle and time delay in effective field theories of gravity
- From amplitudes to gravitational radiation with cubic interactions and tidal effects
- The 2PM Hamiltonian for binary Kerr to quartic in spin
- Resummed spinning waveforms from five-point amplitudes
- Scalar QED as a toy model for higher-order effects in classical gravitational scattering
- Large Gauge Effects and the Structure of Amplitudes
- Radiative Classical Gravitational Observables at from Scattering Amplitudes
- Spin supplementary condition in quantum field theory: covariant SSC and physical state projection
- Bootstrapping spinning two body problem in dynamical Chern-Simons gravity using worldline QFT
- On the equivalence between theories and Einstein gravity
- The Eikonal Approximation and the Gravitational Dynamics of Binary Systems
- Scattering Amplitudes for Binary Systems beyond GR
- Unitarity, Causality, and Solar System Bounds May Significantly Limit the Use of Gravitational Waves to Test General Relativity