A simple model of pointlike spacetime defects and implications for photon propagation
M. Schreck, F. Sorba, S. Thambyahpillai

TL;DR
This paper models pointlike spacetime defects in Minkowski space to investigate potential Lorentz violation effects on photon propagation, finding that a dense, homogeneous, and isotropic defect distribution preserves Lorentz invariance.
Contribution
It introduces a Lorentz-invariant spacetime defect model and demonstrates through perturbation theory that photon dispersion remains conventional under certain conditions.
Findings
Photon dispersion law remains unchanged with dense, isotropic defects
Lorentz invariance can be preserved despite small-scale spacetime structure
Direct computation supports theoretical predictions of Lorentz invariance preservation
Abstract
A model in which pointlike defects are randomly embedded in Minkowski spacetime is considered. The distribution of spacetime defects is constructed to be Lorentz-invariant. It does not introduce a preferred reference frame, because it is based on a sprinkling process. A field-theoretic action for the photon and a fermion is set up, in which the photon is assumed not to couple to the defects directly, but via a scalar field. We are interested in signs for Lorentz violation caused by the spacetime defects, which are expected to reveal themselves in the photon sector. A modification of the photon dispersion relation may result as a quantum effect and we compute it at leading order perturbation theory. The outcome of the calculation is that the photon dispersion law remains conventional, if the defect distribution is dense, homogeneous, and isotropic. This result sheds some new light on…
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