Exploring the Primordial Power Spectrum with Dark-Age 21 cm fluctuations
astro-ph.CO, gr-qc, hep-ph
Submitted: 2026-09-30
Updated: 2026-09-30
Terminology
Sources
- Planck 2018 results. X. Constraints on inflation
- BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season
- The Atacama Cosmology Telescope: DR6 Constraints on Extended Cosmological Models
- SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field
- Constraints on Primordial Power Spectrum from Galaxy Luminosity Functions
- Impact of the primordial fluctuation power spectrum on the reionization history
- The primordial matter power spectrum on sub-galactic scales
- Constraints on small-scale cosmological fluctuations from SNe lensing dispersion
- Impact of EDGES 21cm Global Signal on Primordial Power Spectrum
- Probing Small Scale Primordial Power Spectrum with 21cm Line Global Signal
- 21 cm Angular Power Spectrum from Minihalos as a Probe of Primordial Spectral Runnings
- How accurately can 21 cm tomography constrain cosmology?
- Precise Measurements of Primordial Power Spectrum with 21 cm Fluctuations
- Probing small-scale cosmological fluctuations with the 21 cm forest: effects of neutrino mass, running spectral index and warm dark matter
- Minimally Parametric Power Spectrum Reconstruction from the Lyman-alpha Forest
- Neutrino masses and cosmology with Lyman-alpha forest power spectrum
- Forecasts for CMB \mu- and i-type spectral distortion constraints on the primordial power spectrum on scales 8 < k < 10^4 Mpc^-1 with the future Pixie-like experiments
- Testing Inflation and Curvaton Scenarios with CMB Distortions
- Running the running
- CMB spectral distortions in generic two-field models
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