Dark matter from hot big bang black holes

Abstract

If the temperature of the hot thermal plasma in the Early Universe was within a few orders of magnitude of the Planck scale \(M_{\rm Pl}\), then the hoop conjecture predicts the formation of microscopic black holes from particle collisions in the plasma. Although these evaporated instantly, they would have left behind a relic abundance of all stable degrees of freedom which couple to gravity. Here we show that, upon minimal assumptions of a high reheat temperature and semiclassical black hole dynamics, this process could have produced the relic abundance of dark matter observed today for a particle mass anywhere in the range of \(100~\mathrm{keV} \lesssim m_{dm} < M_{\rm Pl}\). The production mechanism does not rely on any additional assumptions about non-gravitational dark matter-Standard Model interaction.