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- W3036193497 abstract "We discuss formation of dark matter (DM) mini-halos around primordial black holes (PBHs) and its implication on DM direct detection experiments, including axion searches. Motivated by LIGO observations, we consider $f_{textrm{DM}} simeq 0.01$ as the fraction of DM in PBHs with masses $10 M_{odot} - 70 M_{odot}$. In this case, we expect the presence of dressed PBHs after Milky Way halo formation with mini-halo masses peaked around $M_{textrm{halo}} sim (50-55) M_{textrm{PBH}}$. We analyze the effect of tidal forces acting on dressed PBHs within the Milky Way galaxy. In the solar neighborhood, the mini-halos are resistant against tidal disruption from the mean-field potential of the galaxy and encounters with stars, but they undergo a small level of disruption caused by disk shocking. The presence of mini-halos around LIGO-motivated PBHs today could reduce by half the local dark matter background. High-resolution simulations are encouraged. If the proposed scenario is realized, chances of direct detection of DM would decrease." @default.
- W3036193497 created "2020-06-25" @default.
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- W3036193497 date "2020-08-01" @default.
- W3036193497 modified "2023-10-14" @default.
- W3036193497 title "Implications for dark matter direct detection in the presence of LIGO-motivated primordial black holes" @default.
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- W3036193497 doi "https://doi.org/10.1016/j.physletb.2020.135566" @default.
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