Flash Ionization of the Early Universe by Pop III.1 Supermassive Stars

TL;DR

The paper explores how supermassive stars in the early universe ionized the cosmos, influencing cosmic microwave background measurements and potentially resolving key cosmological tensions.

Contribution

It introduces the concept of 'The Flash' ionization era caused by Pop III.1 supermassive stars and discusses its implications for CMB optical depth and cosmic background signals.

Findings

Estimated ionization contribution of τ_popIII.1 ≈ 0.04

Combined reionization contributions yield τ ≈ 0.10

Potential resolution of Hubble tension and 21-cm absorption anomalies

Abstract

The Pop III.1 theory for supermassive black hole (SMBH) formation predicts that a substantial fraction of the early universe was ionized by supermassive stars at redshifts $z\sim20-30$, an era we refer to as ``The Flash''. This is followed by recombination to a mainly neutral state within a few tens of Myr. Here we discuss the implication of this ionization for the scattering optical depth of the cosmic microwave background (CMB), $\tau$. We find a fiducial contribution of $\tau_{\rm PopIII.1}\sim0.04$. Combining this with the contribution to reionization by standard galaxy populations at $z\lesssim 10$ with $\tau_{\rm gal}\simeq0.06$, yields a total of $\tau\simeq0.10$. As noted recently by several authors, such a value may help resolve apparent ``problems'' faced by $\Lambda$CDM of discrepant CMB-based measures of the Hubble constant (``Hubble tension''), as well as negative neutrino masses and dynamical dark energy that have been implied by recent Baryonic Acoustic Oscillation (BAO) results from the Dark Energy Spectroscopic Instrument (DESI). In addition, free-free emission from The Flash boosts the cosmic radio background, which could help explain the large 21-cm absorption depth reported by the Experiment to Detect the Global EoR Signature (EDGES).