OVERVIEW. “In this section we’ll look at the observational evidence for cold, non-baryonic dark matter, starting with galaxies, before moving out in scale to galaxy clusters, the cosmic microwave background anisotropies and large scale structure.”
https://lnkd.in/e6ifiQMn
linkedin post 2022-06-29 05:12:48
Nigel Fleming
September 21, 2022