Constraints on Early Star Formation from the 21-cm Global Signal

TL;DR

The paper discusses how the EDGES 21-cm signal constrains early star formation, suggesting that standard, metal-poor stellar populations can explain the observations without invoking exotic sources, and provides implications for reionization history.

Contribution

It demonstrates that the EDGES signal is consistent with extrapolated galaxy UV luminosity densities and constrains star formation rates and escape fractions at high redshift.

Findings

EDGES results align with existing galaxy UV luminosity data at 4<z<9.

No need for exotic UV sources to explain the 21-cm absorption.

Escape fractions below 20% are sufficient to delay reionization.

Abstract

The tentative detection by the EDGES experiment of a global 21-cm absorption trough centered at redshift 17 opens up the opportunity to study the birth of the first luminous sources, the intensity of radiation backgrounds at cosmic dawn, the thermal and ionization history of the young intergalactic medium. Here, we focus on the astrophysical implications of the Lyman-alpha photon field needed to couple the spin temperature to the kinetic temperature of the gas at these early epochs. Under the basic assumption that the 21-cm signal is activated by extremely metal-poor stellar systems, we show that the EDGES results are consistent with an extrapolation of the declining galaxy UV luminosity density measured at 4<z<9 by deep HST observations. A substantially enhanced star formation rate density or new exotic sources of UV photons are not required at the redshifts of the EDGES signal. The amount of ionizing radiation produced by the same stellar systems that induce Lyman-alpha coupling is significant, of order 0.5 Lyman-continuum photons per H-atom per 100 Myr. To keep hydrogen largely neutral and delay the reionization process consistently with recent Planck CMB results, mean escape fractions of f_esc < 20% are required at z>15.