Photon propagation in Einstein and Higher Derivative Gravity
arXiv:gr-qc/9804017 · doi:10.1016/S0550-3213(98)00275-2
Abstract
In the wave equation obeyed by electromagnetic fields in curved spacetime there are Riemann and Ricci curvature coupling terms to the photon polarisation, which result in a polarisation dependent deviation of the photon trajectories from null geodesics. Photons are found to have an effective mass in an external gravitational field and their velocity in an inertial frame is in general less than . A consequence of this is that the curvature corrections to the propagation of electromagnetic radiation keep the velocities subluminal provided the strong energy condition is satisfied. We further show that the claims of superluminal velocities in higher derivative gravity theories are erroneous and arise due to the neglect of Riemann and Ricci coupling terms in the wave equation, which exists in Einstein's gravity itself.
12 page Latex. To appear in Nuclear Physics B
Cited by in corpus (14)
- How does the electromagnetic field couple to gravity, in particular to metric, nonmetricity, torsion, and curvature?
- Strong deflection gravitational lensing by a modified Hayward black hole
- Gauge Invariant Wave Equations in Curved Space-Times and Primordial Magnetic Fields
- Non-minimal coupling of photons and axions
- Strong gravitational field time delay for photons coupled to Weyl tensor in a Schwarzschild black hole
- Wave propagation in linear electrodynamics
- One-loop corrections to the photon propagator in the curved-space QED
- Superluminality, Black Holes and Effective Field Theory
- Anisotropic cosmological models with non-minimally coupled magnetic field
- Nonminimal isotropic cosmological model with Yang-Mills and Higgs fields
- Light propagation with non-minimal couplings in a two-component cosmic dark fluid with an Archimedean-type force and unlighted cosmological epochs
- Motion of a Vector Particle in a Curved Spacetime. I. Lagrangian Approach
- Motion of a Vector Particle in a Curved Spacetime. II First Order Correction to a Geodesic in a Schwarzschild Background
- General Relativistic Contribution to Polarization of the Cosmic Microwave Background Anisotropy