Varying fine-structure constant cosmography

Cosmography is a phenomenological and relatively model-independent approach to cosmology, where physical quantities are expanded as a Taylor series in the cosmological redshift, or in related variables. Here we apply this methodology to constrain possible cosmological variations of the fine-structure constant, alpha. Two peculiarities of this case are the existence of high-redshift data, and the fact that one term in the series is directly and tightly constraint by local laboratory tests with atomic clocks. We use this atomic clock data, together with direct model-independent high-resolution astrophysical spectroscopy measurements of alpha up to redshift z similar to 7 and additional model-dependent constraints on alpha from the cosmic microwave background and big bang nucleosynthesis, to place stringent (parts per million level) constraints on the first two terms in the alpha cosmographic series. (c) 2022 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/). Funded by SCOAP(3).

Automated summary

Cosmography is used to constrain cosmological variations of the fine-structure constant α, with limitations imposed by high-redshift data and local laboratory tests. Strict constraints are obtained through a combination of atomic clock data, high-resolution astrophysical spectroscopy measurements, and model-dependent constraints.