The SARAS 3 Non-Detection as a Bound on Early X-ray Heating in the Bounce Frame

Where EDGES reported a deep feature, the SARAS 3 experiment reported no such feature and rejected the EDGES best-fitting profile at stated confidence. Using the stated cosmology and the brightness-temperature relations described in the Methods, the calculation gives the following headline values: max heat frac = 0.59; depth at bound mK = -150; unheated depth mK = -260. The comparison values taken from the published record — including the EDGES and SARAS reports, HERA limits and the Planck optical depth where relevant — are used exactly as published, and the bounce contribution enters only through the named timing, heating or shear inputs. The result is a computed prediction for the delayed-onset history, with its sensitivity to each input stated in the Discussion. This study is simulated and computed from stated assumptions; it is not a measurement.

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-11-11
DOI
https://doi.org/10.5281/zenodo.24138144
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
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article

The SARAS 3 Non-Detection as a Bound on Early X-ray Heating in the Bounce Frame

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

The SARAS 3 Non-Detection as a Bound on Early X-ray Heating in the Bounce Frame

William Alexander Aldred
article en

Abstract

Where EDGES reported a deep feature, the SARAS 3 experiment reported no such feature and rejected the EDGES best-fitting profile at stated confidence. Using the stated cosmology and the brightness-temperature relations described in the Methods, the calculation gives the following headline values: max heat frac = 0.59; depth at bound mK = -150; unheated depth mK = -260. The comparison values taken from the published record — including the EDGES and SARAS reports, HERA limits and the Planck optical depth where relevant — are used exactly as published, and the bounce contribution enters only through the named timing, heating or shear inputs. The result is a computed prediction for the delayed-onset history, with its sensitivity to each input stated in the Discussion. This study is simulated and computed from stated assumptions; it is not a measurement.

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