How to see the invisible: Using the dark matter distribution to test our cosmological model

Astrophysicists have measured a value for the ‘clumpiness’ of the universe’s dark matter (known to cosmologists as ‘S8’) of 0.776, which does not align with the value derived from the Cosmic Microwave Background, which dates back to the universe’s origins. This has intriguing implications for the standard cosmological model.

Source: ScienceDaily.com