Speaker
Aurel Schneider
(University of Zurich)
Summary
Observations from both the local and the high-redshift universe can be used to test the nature of dark matter. I will discuss several astrophysical probes (dwarf galaxy counts, Lyman-alpha forest, ..) and their constraining power on different dark matter scenarios (such as warm, mixed, and interacting dark matter).
Based on (arXiv number) | 1601.07553, 1412.2133 |
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Author
Aurel Schneider
(University of Zurich)