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

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
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
NOV
article

The Scalar Spectral Index Across Ten Decades of Wavenumber in a Bounce Spectrum

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

The Scalar Spectral Index Across Ten Decades of Wavenumber in a Bounce Spectrum

William Alexander Aldred
article en

Abstract

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.

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

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.

Laika access coming soon