The Redshift of Recombination Under a Bounce-Modified Expansion History: A Sub-Percent Calculation

Recombination, the formation of neutral hydrogen at a redshift near 1090, is located by the microwave background with remarkable precision: the standard value carries an uncertainty of about a quarter of a unit in redshift. With the stated sensitivity, a one percent residual change in the expansion rate would move the last-scattering redshift to 1093.2, a shift of 3.3 units, more than ten times the observational uncertainty of 0.25. Conversely, the spin term predicted at recombination for bounce temperatures above the nucleosynthesis bound corresponds to a shift orders of magnitude below the uncertainty. The instrument is sharp; the predicted signal on the allowed branch is far beneath it; and stating both numbers together is the correct, complete result. Computed from stated assumptions, not measured.

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Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-11-11
DOI
https://doi.org/10.5281/zenodo.24125954
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
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article

The Redshift of Recombination Under a Bounce-Modified Expansion History: A Sub-Percent Calculation

William Alexander Aldred
Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
article

The Redshift of Recombination Under a Bounce-Modified Expansion History: A Sub-Percent Calculation

William Alexander Aldred
article en

Abstract

Recombination, the formation of neutral hydrogen at a redshift near 1090, is located by the microwave background with remarkable precision: the standard value carries an uncertainty of about a quarter of a unit in redshift. With the stated sensitivity, a one percent residual change in the expansion rate would move the last-scattering redshift to 1093.2, a shift of 3.3 units, more than ten times the observational uncertainty of 0.25. Conversely, the spin term predicted at recombination for bounce temperatures above the nucleosynthesis bound corresponds to a shift orders of magnitude below the uncertainty. The instrument is sharp; the predicted signal on the allowed branch is far beneath it; and stating both numbers together is the correct, complete result. Computed from stated assumptions, not measured.

Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
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