Spacetime structure and asymmetric metric from the premetric formulation of electromagnetism
Wei-Tou Ni

TL;DR
This paper investigates how the spacetime metric can be derived from premetric electrodynamics, examining the role of skewons and antisymmetric components, and constraining their effects through observational data on birefringence and polarization rotation.
Contribution
It provides new constraints on skewon and antisymmetric metric components in premetric electrodynamics, linking theoretical structures to observational limits.
Findings
Type I skewon constrained to < 10^(-35)
Type II skewon constrained to 10^(-19) by birefringence
Antisymmetric metric part constrained by cosmic polarization rotation
Abstract
After reviewing the construction of metric from premetric electrodynamics with empirical improvement of accuracy in the skewonless case, we explore the role of skewons in the construction of spacetime metric in the full premetric electrodynamics. For metric principal part plus skewon part, we have shown that the Type I skewon part is constrained to < a few x 10^(-35) in the weak field/weak EEP violation limit. Type II skewon part is not constrained in the first order. However, in the second order it induces birefringence; the nonbirefringence observations constrain the Type II skewon part to 10^(-19). Nevertheless, an additional nonmetric induced second-order contribution to the principal part constitutive tensor compensates the Type II skewon birefringence and makes it nonbirefringent. This second-order contribution is just the extra piece to the core-metric principal constitutive…
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