Early Universe Cosmology in Internal Relativity
Olaf Dreyer

TL;DR
This paper proposes a new early universe cosmology model where a phase transition creates matter and geometry simultaneously, predicting a nearly flat, slightly tilted spectrum of metric perturbations consistent with observations, and suggests discreteness of spacetime.
Contribution
It introduces a phase transition-based cosmology replacing inflation, linking the tilt of the perturbation spectrum to critical exponents, implying a discrete underlying structure of spacetime.
Findings
Spectrum of metric perturbations is flat and tilted due to phase transition dynamics.
Tilt of the spectrum is related to critical exponent η, between 0.03 and 0.06.
Observed tilt may indicate spacetime discreteness.
Abstract
We present a new approach to early universe cosmology. Inflation is replaced by a phase transition in which both matter and geometry are created simultaneously. We calculate the spectrum of metric perturbations and show that it is flat. We then argue that as a consequence of the dynamic nature of the phase transition the spectrum is likely not completely flat but tilted. We argue that the tilt is related to , one of the critical exponents characterizing the phase transition. This exponent generically lies between 0.03 and 0.06. It thus coincides with the observed tilt of the perturbation spectrum. Because the critical exponent is related to the presence of an additional small length scale we argue that the deviation of the observed spectrum from flatness might be an experimental indication that our world is in fact discrete.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Relativity and Gravitational Theory
