Probing dark sectors with exploding black holes: gamma rays

A bstract The Hawking radiation from the explosion of a black hole would provide definitive information on the particle spectrum of nature. Here we quantify the potential of current and future gamma ray telescopes to probe new dark sectors. We improve on the analysis used in previous work by making careful use of the experimental response functions, deriving a more realistic estimate of the backgrounds and optimizing the statistical analysis. We compute the sensitivity of the current experiments (HAWC and LHAASO) and estimate the reach of the future experiments (SWGO and CTA North and South), for various sky positions of the explosion. We find that for a black hole exploding at 0 . 01 pc the gamma ray signal observed by HAWC could probe dark sectors with 10–20 (or more) new Dirac fermions up to masses around 10 5 GeV, while CTA will be able to probe 2–15 new Dirac fermions with masses up to 10 6 GeV. CTA North and South will have sensitivity to 10 dark fermions up to a distance of 0.1 pc and 50 up to a distance of 0.6 pc.