Mike Boylan-Kolchin
3/29/23, 9:00 AM
Dark matter and structure in the Universe
Talk
In its most basic form, the highly successful $\Lambda$CDM cosmology can be encapsulated in six parameters. Once these parameters are specified, so too is a wide variety of phenomena, from fluctuations in the microwave background to the growth of structure to the evolution of the expansion rate of the Universe. I will review the predictions related to cosmological structure formation, focusing...