Gravitational closure of weakly birefringent electrodynamics
Jonas Schneider, Frederic P. Schuller, Nadine Stritzelberger, Florian, Wolz

TL;DR
This paper derives a new family of gravitational field equations based on the causal structure of weakly birefringent electrodynamics, enabling predictions of vacuum birefringence phenomena.
Contribution
It introduces a gravitational closure method to derive tensorial gravitational dynamics from the most general linear electrodynamics with weak birefringence.
Findings
Eleven-parameter family of weak gravitational field equations
Predicts conditions for vacuum birefringence occurrence
Links electrodynamics properties to gravitational dynamics
Abstract
We derive the gravitational dynamics of the tensorial geometry which underlies the most general linear theory of electrodynamics that features weak birefringence in vacuo. This derivation is performed by way of gravitational closure, which is a mechanism that employs the causal structure of any canonically quantizable matter dynamics on some tensorial spacetime geometry in order to derive canonical dynamics for the latter. The resulting eleven-parameter family of weak gravitational field equations allows to predict where vacuum birefringence will occur, if there is any.
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Quantum Electrodynamics and Casimir Effect
