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Edward Wright (UCLA)29/03/2023, 08:00
Cosmology has advanced from "2.5 facts" in 1963 to a very data-rich field today. This has led to the determination of the baryon density, the dark matter density, and the dark energy density. But more facts lead to a greater reliance on advanced statistical techniques, which are usually useful but occasionally misleading. It is important to consider "look elsewhere effects", and to remember...
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Josh Frieman (Fermilab)29/03/2023, 08:30
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Mike Boylan-Kolchin29/03/2023, 09:00Dark matter and structure in the UniverseTalk
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...
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Dr Anna Nierenberg29/03/2023, 09:30
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Mike Boylan-Kolchin (The University of Texas at Austin)Talk
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