Slowly evolving early universe and a phenomenological model for time-dependent fundamental constants and the leptonic masses
Dara Faroughy

TL;DR
This paper proposes a phenomenological model where fundamental constants and leptonic masses vary over cosmic time, suggesting a very slowly expanding early universe with negligible light speed at t=0, impacting cosmological theories.
Contribution
It introduces a novel phenomenological model that accurately describes the time variation of fundamental constants and leptonic masses in the early universe, emphasizing a slowly evolving initial phase.
Findings
Model achieves extreme accuracy in describing constant variations.
Suggests a negligibly small light speed at early times.
Impacts cosmological understanding of universe expansion.
Abstract
A phenomenological model with an extreme accuracy is proposed for the cosmic time variation of the primordial fundamental constants (e, h, G and c) and the leptonic masses. The model is purely exploratory in that at the very early times the light speed is purposely modeled to be negligibly small, indicating a very slowly expanding universe around t=0. The impact of this idea in cosmology and its modeling is overwhelming.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Relativity and Gravitational Theory
