Charge conservation in a gravitational field in the scalar ether theory
Mayeul Arminjon

TL;DR
This paper investigates charge conservation in a scalar ether theory with gravity, showing that modified Maxwell equations predict charge non-conservation, but standard equations with an interaction tensor restore conservation and may relate to dark matter.
Contribution
The work introduces an asymptotic scheme for electromagnetic fields in weak gravitational fields and demonstrates that standard Maxwell equations with an interaction tensor are compatible with the scalar ether theory.
Findings
Modified Maxwell equations predict charge non-conservation.
Standard Maxwell equations with an interaction tensor restore charge conservation.
Interaction energy could contribute to dark matter.
Abstract
A modification of the Maxwell equations due to the presence of a gravitational field was formerly proposed for a scalar theory with a preferred reference frame. With this modification, the electric charge is not conserved. The aim of the present work was to numerically assess the amount of charge production or destruction. We propose an asymptotic scheme for the electromagnetic field in a weak and slowly varying gravitational field. This scheme is valid independently of the theory and the "gravitationally-modified" Maxwell equations. Then we apply this scheme to plane waves and to a group of Hertzian dipoles in the scalar ether theory. The predicted amounts of charge production/destruction discard the formerly proposed gravitationally-modified Maxwell equations. The theoretical reason for that is the assumption that the total energy tensor is the sum of the energy tensor of the medium…
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.
