Dimensionless cosmology
Ali Narimani, Adam Moss, Douglas Scott

TL;DR
This paper emphasizes the importance of using dimensionless parameters in cosmology, illustrating how to properly analyze variations in fundamental constants like G and alpha through a dimensionless framework, with applications to Big Bang Nucleosynthesis and CMB data.
Contribution
It introduces a dimensionless formulation of cosmological parameters and demonstrates how to analyze variations in fundamental constants without inconsistencies, including implications for future CMB experiments.
Findings
Dimensionless parameters clarify the physics of cosmological epochs.
Misinterpretation of G variations can occur if not properly dimensionless.
Future experiments can constrain fine structure constants with high precision.
Abstract
Although it is well known that any consideration of the variations of fundamental constants should be restricted to their dimensionless combinations, the literature on variations of the gravitational constant is entirely dimensionful. To illustrate applications of this to cosmology, we explicitly give a dimensionless version of the parameters of the standard cosmological model, and describe the physics of Big Bang Neucleosynthesis and recombination in a dimensionless manner. The issue that appears to have been missed in many studies is that in cosmology the strength of gravity is bound up in the cosmological equations, and the epoch at which we live is a crucial part of the model. We argue that it is useful to consider the hypothetical situation of communicating with another civilization (with entirely different units), comparing only dimensionless constants, in order to decide if…
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