Using the cosmological recombination radiation to probe early dark energy and fundamental constant variations
Luke Hart, Jens Chluba

TL;DR
This paper explores how the cosmological recombination radiation (CRR) can be used to investigate early dark energy and variations in fundamental constants, providing a potential new probe of the pre-recombination universe despite small signal levels.
Contribution
It computes the effects of early dark energy and fundamental constant variations on the CRR and assesses the sensitivity of future spectrometers to these signals.
Findings
CRR depends on changes in expansion history and recombination physics.
Futuristic sensitivities are needed for competitive constraints.
CRR measurements can access otherwise unreachable early Universe phases.
Abstract
The cosmological recombination radiation (CRR) is one of the guaranteed spectral distortion signals from the early Universe. The CRR photons from hydrogen and helium pre-date the last scattering process and as such allow probing physical phenomena in the pre-recombination era. Here we compute the modifications to the CRR caused by early dark energy models and varying fundamental constants. These new physics examples have seen increased recent activity in connection with the Hubble tension, motivating the exploratory study presented here. The associated CRR responses are spectrally-rich but the level of the signals is small. We forecast the possible sensitivity of future spectrometers to these effects. Our estimates demonstrate that the CRR directly depends to changes in the expansion history and recombination physics during the pre-recombination era. However, futuristic sensitivities…
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Taxonomy
TopicsCosmology and Gravitation Theories · Galaxies: Formation, Evolution, Phenomena · Dark Matter and Cosmic Phenomena
