Cosmology in the presence of diffeomorphism-violating, nondynamical background fields

TL;DR

This paper explores how nondynamical background fields violating diffeomorphism invariance influence cosmological evolution, potentially causing accelerated expansion without exotic matter, and provides initial insights into their phenomenological effects.

Contribution

It introduces the application of the Standard-Model Extension to cosmology, analyzing background field configurations that induce accelerated expansion without exotic matter.

Findings

Identified background configurations leading to accelerated expansion

Demonstrated how background fields modify cosmological evolution equations

Provided initial understanding of phenomenological impacts of diffeomorphism violation

Abstract

We consider diffeomorphism violation, which is parameterized by nondynamical background fields of the gravitational Standard-Model Extension (SME), and study its effects on the time evolution of the Universe. Our goal is to identify background field configurations that imply stages of accelerated expansion without exotic forms of matter and radiation present. Although our approach gives rise to a set of restrictive conditions, configurations are encountered that exhibit this property or show other interesting behaviors. The findings of our article, which is among the first to apply the SME to a cosmological setting, provide an initial understanding of how to technically incorporate background fields into the cosmological evolution equations and what their phenomenological impact may be.