Was the Universe Reionized by Massive Population-iii Stars?

The WMAP satellite has measured a large optical depth to electron scattering after cosmological recombination of τes = 0.17 ± 0.04, implying significant reionization of the primordial gas only ∼ 200 million years after the big bang. However, the most recent overlap of intergalactic HII regions must have occurred at z . 9 based on the Lyα forest constraint on the thermal history of the intergalactic medium. Here we argue that a first generation of metal–free stars with a heavy (rather than Salpeter) mass function is therefore required to account for much of the inferred optical depth. This conclusion holds if feedback regulates star formation in early dwarf galaxies as observed in present-day dwarfs. Subject headings: Cosmology: theory – Early universe – Intergalactic medium – Stars: population-III