Variations of the Fine Structure Constant in Space and Time
D.F. Mota (Cambridge Univ., DAMTP)

TL;DR
This thesis investigates how matter inhomogeneities influence the evolution of the fine structure constant in the universe, using the BSBM theory, through analytical solutions, perturbation analysis, and non-linear regime studies.
Contribution
It provides a comprehensive analysis of the space-time variations of the fine structure constant considering matter inhomogeneities and dark energy effects within the BSBM framework.
Findings
Derived exact solutions for the fine structure constant in homogeneous universes.
Analyzed the evolution of inhomogeneous perturbations on different scales.
Explored the impact of matter coupling and dark energy on the constant's variation.
Abstract
This thesis describes a detailed investigation of the effects of matter inhomogeneities on the cosmological evolution of the fine structure constant using the Bekenstein-Sandvik-Barrow-Magueijo (BSBM) theory. We briefly review the observational and theoretical motivations to this work, together with the standard cosmological model. We start by analysing the phase space of the system of equations that describes a time-varying fine structure constant, in a homogeneous and isotropic background universe. We classify all the possible behaviours of the fine structure constant in ever-expanding universes and find exact solutions for it. Using a gauge-invariant formalism, we derive and solve the linearly perturbed Einstein cosmological equations for the BSBM theory. We calculate the time evolution of inhomogeneous perturbations of the fine structure constant on small and large scales with…
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Taxonomy
TopicsCosmology and Gravitation Theories · Galaxies: Formation, Evolution, Phenomena · Black Holes and Theoretical Physics
