Running of the Scalar Spectral Index From a Scale-Dependent Shear Fraction at the Bounce

If the conditions at a bounce vary with the scale crossing it, the spectral index runs. This paper computes the running produced when the shear fraction at crossing scales with wavenumber as a power law, f(k) = f* (k/k*)^gamma, and compares it with the Planck measurement. At the fiducial scaling exponent gamma = 0.12, the running at the pivot is alpha = -0.002109 and the running of the running is beta = -0.00012656. The Planck 2018 value is alpha = -0.0045 plus or minus 0.0067, so the prediction deviates by 0.36 standard deviations, comfortably inside the measurement. The same comparison bounds the scaling exponent: gamma above 1 would push the running outside the two-standard-deviation band. The observed near-absence of running therefore translates into a real constraint on how strongly the bounce conditions may vary across the decade of scales the microwave background probes. The study is 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.24134377
Primary Topic
Cosmology and Gravitation Theories
Type
article
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article

Running of the Scalar Spectral Index From a Scale-Dependent Shear Fraction at the Bounce

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

Running of the Scalar Spectral Index From a Scale-Dependent Shear Fraction at the Bounce

William Alexander Aldred
article en

Abstract

If the conditions at a bounce vary with the scale crossing it, the spectral index runs. This paper computes the running produced when the shear fraction at crossing scales with wavenumber as a power law, f(k) = f* (k/k*)^gamma, and compares it with the Planck measurement. At the fiducial scaling exponent gamma = 0.12, the running at the pivot is alpha = -0.002109 and the running of the running is beta = -0.00012656. The Planck 2018 value is alpha = -0.0045 plus or minus 0.0067, so the prediction deviates by 0.36 standard deviations, comfortably inside the measurement. The same comparison bounds the scaling exponent: gamma above 1 would push the running outside the two-standard-deviation band. The observed near-absence of running therefore translates into a real constraint on how strongly the bounce conditions may vary across the decade of scales the microwave background probes. The study is computed from stated assumptions, not measured.

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