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Astrophysics Colloquium: Matthew Walker, Center for Astrophysics, Harvard University: "Galactic Dynamics and the Nature of Dark Matter"

Event Type
Seminar/Symposium
Sponsor
Astronomy Department
Location
134 Astronomy
Date
Feb 14, 2013   4:00 pm  
Speaker
Matthew Walker
Contact
Brian Fields
E-Mail
bdfields@illinois.edu
Views
2033
Originating Calendar
Astronomy Colloquium Speaker Calendar

I will explain how to use the motions of stars to learn about the nature of particles.  More specifically, I will translate the stellar kinematics that I observe in the nearest, smallest and `darkest' galaxies into a test of the standard hypothesis that dark matter consists of `cold' and `collisionless' (i.e., weakly interacting) particles.  This model escapes falsification only if baryon-driven processes (e.g., energetic feedback from supernova explosions) alter the internal structure of galactic dark matter halos systematically with respect to predictions derived from cosmological N-body simulations.  I will identify future work -- both observational and theoretical -- that I expect will tell definitively whether such reconciliation is energetically feasible or whether the dark matter model requires additional complexity.

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