Deuterium Survival Through the Bottleneck in a Bounced Cosmology: A Yield and a Sensitivity Coefficient

Deuterium is the most fragile of the light nuclei and the most informative. The scan gives a logarithmic sensitivity of 0.15 for the deuterium abundance with respect to the bounce temperature in the range examined. A bounce at 0.2 MeV would leave a residue of 2.16e-05, well below the observed value, while a bounce at 1 MeV leaves 2.52e-05, close to the standard 2.53e-05. Deuterium therefore excludes a low bounce more firmly, per unit of observational effort, than any other single light element considered in isolation. Computed from stated assumptions, not measured.

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-11-11
DOI
https://doi.org/10.5281/zenodo.24125749
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
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article

Deuterium Survival Through the Bottleneck in a Bounced Cosmology: A Yield and a Sensitivity Coefficient

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

Deuterium Survival Through the Bottleneck in a Bounced Cosmology: A Yield and a Sensitivity Coefficient

William Alexander Aldred
article en

Abstract

Deuterium is the most fragile of the light nuclei and the most informative. The scan gives a logarithmic sensitivity of 0.15 for the deuterium abundance with respect to the bounce temperature in the range examined. A bounce at 0.2 MeV would leave a residue of 2.16e-05, well below the observed value, while a bounce at 1 MeV leaves 2.52e-05, close to the standard 2.53e-05. Deuterium therefore excludes a low bounce more firmly, per unit of observational effort, than any other single light element considered in isolation. Computed from stated assumptions, not measured.

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