Kavli Affiliate: George Efstathiou | Summary:High-mass X-ray binaries are one of the primary drivers of the 21-cm signal from Cosmic Dawn and Reionization, playing a leading role in the thermal history of the intergalactic medium. In traditional semi-numerical simulations, a deterministic scaling relation between the total X-ray luminosity of high-mass X-ray binaries, $L_rm X$, and […]
Continue.. Impact of Stochastic Pop~III X-ray Binaries on the Cosmological 21-cm Signal