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There is growing evidence for a larger than expected population of supermassive black holes at high redshifts. These puzzling black holes appear to defy standard formation histories: they are too large at too early a time in the cosmic history. One leading explanation is that these may have formed through the direct collapse of pre-star forming halos. The critical element is a flux of O(10 eV) photons that can suppress molecular hydrogen formation in these systems. We present evidence that decaying dark matter can be a viable source for these photons and may play a role in explaining these high-redshift supermassive black holes.
TG