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This document discusses the potential of primordial micro black holes (µBHs) as candidates for dark matter, particularly in scenarios where gravity is modified by extra dimensions or a large number of species. It highlights the unique properties of these black holes, including their mass-radius relation, temperature, and evaporation characteristics, which differ from conventional black holes, allowing for cosmological stability. The authors analyze observational consequences, emphasizing neutron star surviv

Author

break.the.rules26

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EN