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Primordial black holes are produced in a minimal UV extension to the Higgs inflation with an included R 2 term. We show that for parameters consistent with Standard Model measurements and Planck observation results lead to M PBH ∊ (10 −16 , 10 −15 ) M ⊙ primordial black holes with significant abundance, which may consist the majority of dark matter.
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Dhong Yeon Cheong (2021) studied this question.
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