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- W4307700922 abstract "We study the minimum mass of dark compact objects formed in dissipative dark-matter halos and show that the simple atomic-dark-matter model consistent with all current observations can create low-mass fragments that can evolve into compact objects forbidden by stellar astrophysics. We model the collapse of the dark halo's dense core by tracing the thermo-chemical evolution of a uniform-density volume element under two extreme assumptions for density evolution: hydrostatic equilibrium and pressure-free collapse. We then compute the opacity-limited minimum fragment mass from the minimum temperature achieved in these calculations." @default.
- W4307700922 created "2022-11-05" @default.
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- W4307700922 date "2022-10-28" @default.
- W4307700922 modified "2023-10-04" @default.
- W4307700922 title "A Lower Bound on the Mass of Compact Objects from Dissipative Dark Matter" @default.
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- W4307700922 doi "https://doi.org/10.3847/2041-8213/ac997c" @default.
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