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Count your halos

One of the strongest predictions of the standard cold dark matter paradigm is the hierarchy of structure down to Earth-mass scales. However, individual self-bound clumps of dark matter--"halos"--are difficult to detect directly. Instead, we use galaxies as lampposts for halos. By counting galaxies, we can measure the underlying population of dark matter halos. In this talk, I describe results that seem completely at odds with each other in measuring the population of small halos. I argue that the resolution to the problem is a better mapping between galaxies and halos. I will show what my group is doing so far to address the problem, and what opportunities lie ahead in the wide-field surveys of the 2020's.

See weblink for Zoom information, or attend in person

Friday, 05/20/22

Contact:

Website: Click to Visit

Cost:

Free

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Varian Physics Building

382 Via Pueblo Mall
Room 355
Stanford, CA 94305