Tangled tau: Planck CMB Constraints on Flash Reionization
astro-ph.CO
Submitted: 2026-09-21
Updated: 2026-09-21
Comments: 10 pages, 8 figures
Code: https://github.com/CobayaSampler/cobaya
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field
- The BAO-CMB Tension and Implications for Inflation
- On the tension between DESI DR2 BAO and CMB
- Turning a negative neutrino mass into a positive optical depth
- Dispu$\tau$able: the high cost of a low optical depth
- A small and vigorous black hole in the early Universe
- A high black hole to host mass ratio in a lensed AGN in the early Universe
- Flash Ionization of the Early Universe by Pop III.1 Supermassive Stars
- The Impact of Population III.1 Flash Reionization for CMB Polarization and Thomson Scattering Optical Depth
- Fireworks at Cosmic Dawn: relieving BAO-CMB tensions with the Pop III.1 Flash
- The formation of supermassive black holes from Population III.1 seeds. IV. Self-regulated seeding from supermassive star ionizing feedback
- Overmassive black holes and little red dots naturally form in simulations
- The Universe Was Reionized Twice
- Reionization of Hydrogen and Helium by Early Stars and Quasars
- The Reionization History at High Redshifts II: Estimating the Optical Depth to Thomson Scattering from CMB Polarization
- Late reionizations of the Universe and their manifestation in the CMB data
- Cosmic Microwave Background Polarization and reionization: constraining models with a double reionization
- Is Double Reionization Physically Plausible?
- Cosmological parameters from WMAP 5-year temperature maps
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