The Planck Optical Depth Reproduced by a Bounce-Frame Reionisation History
The Thomson optical depth measured from cosmic microwave background polarisation is the most direct integral constraint on reionisation. Using the stated cosmology and the brightness-temperature relations described in the Methods, the calculation gives the following headline values: tau model = 0.058; tau planck = 0.054; tau planck err = 0.007; sigma diff = 0.6. 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
- William Alexander Aldred (ORCID: https://orcid.org/0009-0000-1215-577X)
Publication Details
- Journal
- Zenodo (CERN European Organization for Nuclear Research)
- Published
- 2026-11-11
- DOI
- https://doi.org/10.5281/zenodo.24138084
- Primary Topic
- Cosmology and Gravitation Theories
- Type
- article
- Field-Weighted Citation Impact
- 0.00