Microwave Background Spectral Distortions from Bounce-Era Dissipation: A Limit on Small-Scale Power

Energy released into the early photon bath leaves a characteristic distortion in the microwave background spectrum, of the kind parameterised by a chemical potential when the release is early. For a cutoff at one thousand per megaparsec the predicted distortion falls to 1.02e-08, with a surviving power fraction of 0.511; at two hundred per megaparsec it falls further, to 4.34e-09; the standard value is 2.00e-08, and the firm observational limit from past measurement is 9 in a hundred thousand. A future instrument reaching the standard prediction could therefore detect the absence of power the cutoff implies, turning a null result at the expected level into positive evidence about the initial spectrum at scales no other probe reaches. 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.24125705
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
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article

Microwave Background Spectral Distortions from Bounce-Era Dissipation: A Limit on Small-Scale Power

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

Microwave Background Spectral Distortions from Bounce-Era Dissipation: A Limit on Small-Scale Power

William Alexander Aldred
article en

Abstract

Energy released into the early photon bath leaves a characteristic distortion in the microwave background spectrum, of the kind parameterised by a chemical potential when the release is early. For a cutoff at one thousand per megaparsec the predicted distortion falls to 1.02e-08, with a surviving power fraction of 0.511; at two hundred per megaparsec it falls further, to 4.34e-09; the standard value is 2.00e-08, and the firm observational limit from past measurement is 9 in a hundred thousand. A future instrument reaching the standard prediction could therefore detect the absence of power the cutoff implies, turning a null result at the expected level into positive evidence about the initial spectrum at scales no other probe reaches. Computed from stated assumptions, not measured.

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