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- W2001938438 abstract "Cold Dark Matter (CDM) theory, a pillar of modern cosmology and astrophysics, predicts the existence of a large number of starless dark matter halos surrounding the Milky Way (MW). However, clear observational evidence of these dark substructures remains elusive. Here, we present a detection method based on the small, but detectable, velocity changes that an orbiting substructure imposes on the stars in the MW disk. Using high-resolution numerical simulations we estimate that the new space telescope Gaia should detect the kinematic signatures of a few starless substructures provided the CDM paradigm holds. Such a measurement will provide unprecedented constraints on the primordial matter power spectrum at low-mass scales and offer a new handle onto the particle physics properties of dark matter." @default.
- W2001938438 created "2016-06-24" @default.
- W2001938438 creator A5063586360 @default.
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- W2001938438 date "2014-11-14" @default.
- W2001938438 modified "2023-09-25" @default.
- W2001938438 title "Detecting dark matter substructures around the Milky Way with Gaia" @default.
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- W2001938438 doi "https://doi.org/10.1093/mnras/stu2147" @default.
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