The Scalar Spectral Index Across Ten Decades of Wavenumber in a Bounce Spectrum
A single spectral index quoted at a pivot scale conceals how much the index itself varies across the full range of scales that different observations probe. This paper tabulates the scalar index of the bounce spectrum from k = 1e-4 to 50 per megaparsec, ten decades short of the full range in logarithmic terms covered by microwave, large-scale-structure, Lyman-alpha, and spectral-distortion probes taken together. The index runs from 0.9819 at the largest tabulated scale through 0.9648 at the pivot to 0.9604 at k = 2 per megaparsec and 0.9628 at k = 50 per megaparsec. The total variation across the table is 0.02149, which is 5.1 times the Planck uncertainty on the pivot index. The spectrum is therefore not describable by a constant index beyond the microwave window: analyses that extrapolate the pivot index to small scales would misestimate the index there by several times the pivot's own error bar. The tabulation provides the scale-by-scale values that joint analyses across probes require. The study is computed from stated assumptions, not measured.
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.24134410
- Primary Topic
- Cosmology and Gravitation Theories
- Type
- article
- Field-Weighted Citation Impact
- 0.00