Fireworks at Cosmic Dawn: relieving BAO-CMB tensions with the Pop III.1 Flash
Yash Aggarwal, Christopher Cain, Garett Lopez, Hy Trac, Anson D'Aloisio, Philip Tanedo, Jonathan C. Tan
astro-ph.CO, astro-ph.GA
Submitted: 2026-06-17
Comments: 12 pages, 5 figures. Submitted to ApJL, comments welcome
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Positive neutrino masses with DESI DR2 via matter conversion to dark energy
- The CMB optical depth constrains the duration of reionization
- SPT-3G D1: A Measurement of Secondary Cosmic Microwave Background Anisotropy Power
- It's All ${\tt Ok}$: Curvature in Light of BAO from DESI DR2
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- Rapid late-time reionization: constraints and cosmological implications
- Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape
- GLIMPSE: An ultra-faint $\simeq$ 10$^{5}$ $M_{\odot}$ Pop III Galaxy Candidate and First Constraints on the Pop III UV Luminosity Function at $z\simeq6-7$
- Constraints on the Thomson optical depth to the CMB from the Lyman- alpha forest
- A New Constraint on the Optical Depth from the Reionization History Independent of CMB Large-Scale E-Mode Polarization
- Evidence for non-cold dark matter from DESI DR2 measurements
- Probing the ionizing photon output of galaxies near cosmic dawn with the patchy kSZ effect
- The evolution of protostars powered by dark matter annihilation. I. Fiducial model and first results
- The formation of supermassive black holes from Population III.1 seeds. IV. Self-regulated seeding from supermassive star ionizing feedback
- Percent-level timing of reionization: self-consistent, implicit-likelihood inference from XQR-30+ Ly$\alpha$ forest data
- The Evolution of Pop III.1 Protostars Powered by Dark Matter Annihilation. II. Dependence on WIMP Properties
- JWST Measurements of Neutral Hydrogen Fractions and Ionized Bubble Sizes at $z=7-12$ Obtained with Ly$\alpha$ Damping Wing Absorptions in 27 Bright Continuum Galaxies
- Bursty or heavy? The surprise of bright Population III systems in the Reionization era
- The Impact of Population III.1 Flash Reionization for CMB Polarization and Thomson Scattering Optical Depth
- The Origin of Supermassive Black Holes from Pop III.1 Seeds
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