Electrodynamics and spacetime geometry: Astrophysical applications
Francisco Cabral, Francisco S. N. Lobo

TL;DR
This paper investigates how spacetime curvature influences electromagnetic phenomena in astrophysical contexts, considering non-homogeneous and anisotropic vacuum properties, and explores implications like field decay, gravitomagnetism effects, and variable light speed.
Contribution
It introduces models of vacuum electromagnetic properties that depend on spacetime geometry, relaxing traditional assumptions of homogeneity and isotropy, and analyzes their astrophysical consequences.
Findings
Electromagnetic field decay is affected by gravitational fields.
Gravitomagnetism induces magnetic terms in Gauss's law.
Spacetime curvature can cause spatial variability in the speed of light.
Abstract
After a brief review of the foundations of (pre-metric) electromagnetism, we explore some physical consequences of electrodynamics in curved spacetime. In general, new electromagnetic couplings and related phenomena are induced by the spacetime curvature. The applications of astrophysical interest considered here correspond essentially to the following geometries: the Schwarzschild spacetime and the spacetime around a rotating spherical mass in the weak field and slow rotation regime. In the latter, we use the Parameterised Post-Newtonian (PPN) formalism. We also explore the hypothesis that the electric and magnetic properties of vacuum reflect the spacetime isometries. Therefore, the permittivity and permeability tensors should not be considered homogeneous and isotropic a priori. For spherical geometries we consider the effect of relaxing the homogeneity assumption in the constitutive…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
