High-redshift physics from the acoustic scale
astro-ph.CO, hep-ph
Submitted: 2026-03-18
Updated: 2026-08-29
Comments: 37+11 pages, 11 figures; matches published version
Journal ref: JCAP 08 (2026) 072
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Planck 2018 results. VI. Cosmological parameters
- The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $\Lambda$CDM Parameters
- SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field
- The Cosmic Microwave Background Spectrum from the Full COBE/FIRAS Data Set
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- Massive neutrinos and cosmic composition
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- Theoretical uncertainty in baryon oscillations
- On Precision Measurement of the Mean Curvature
- Neutrino mass from Cosmology
- Dark Matter from an ultra-light pseudo-Goldsone-boson
- Ultra-light Axions: Degeneracies with Massive Neutrinos and Forecasts for Future Cosmological Observations
- A search for ultra-light axions using precision cosmological data
- Future CMB tests of dark matter: ultra-light axions and massive neutrinos
- Cosmology with varying fundamental constants from hyperlight, coupled scalars
- Cosmological implications of baryon acoustic oscillation (BAO) measurements
- A fresh look at linear cosmological constraints on a decaying dark matter component
- Converting non-relativistic dark matter to radiation
- Converting dark matter to dark radiation does not solve cosmological tensions
- What's the matter with $\Sigma m_{\nu}$?
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