Probing the ionizing photon output of galaxies near cosmic dawn with the patchy kSZ effect

TL;DR

This study explores how combining measurements of the patchy kSZ effect and Lyman-alpha forest data can improve constraints on the timing and sources of reionization during cosmic dawn.

Contribution

It demonstrates the potential of pkSZ measurements, combined with Lyman-alpha data, to constrain early reionization and distinguish source clustering effects.

Findings

pkSZ amplitude correlates with reionization start time

Degeneracy between reionization history and source clustering identified

Future measurements can break degeneracies and refine source models

Abstract

A key result from JWST's first cycles is that galaxy formation was well underway by $z=10$. The implications of these early galaxies for reionization are less clear, however. The CMB is one of the few windows into the ionization state of the IGM during reionization's first half, providing an important probe of the ionizing photon sources at those times. Meanwhile, measurements of the Lyman-$\alpha$ forest in the spectra of high-$z$ quasars have improved to the level of tightly constraining the timing of reionization's end. In this paper, we use radiative transfer simulations to explore how measurements of the patchy kinetic Sunyaev Zel'dovich (pkSZ) effect, when combined with Lyman-$\alpha$ forest measurements, can be used to constrain the early stages of reionization and the nature of its sources. For a given source model, we find that the amplitude of the pkSZ power spectra strongly correlates with the start time of reionization, and constrains the number of ionizing photons produced by the high-$z$ source population. Allowing for variations in the source model, this correlation is weakened by a degeneracy between the reionization history and the effects of source clustering. However, we demonstrate two potential ways of breaking this degeneracy using: (1) measurements of large-scale fluctuations in the Ly$\alpha$ forest opacity at $z=5-6$, and/or; (2) the shape of the pkSZ power spectrum measured in future CMB surveys. Models with highly clustered sources yield steeper slopes in the pkSZ power around $\ell = 3,000$, so measurements at additional angular scales can be used to break the history-clustering degeneracy. Our results highlight how future pkSZ measurements will complement JWST observations to improve our understanding of the ionizing sources near cosmic dawn.