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High-precision cosmology and the nature of dark matter

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If you have a question about this talk, please contact Tommaso Giannantonio .

The latest data of the Planck satellite, combined with other observations of the large-scale structure of the Universe, is only compatible with very small deviations from the minimal standard cosmological model (LambdaCDM). Still, in these small deviations, there would be room for interesting effects related to particle physics models. I will focus on several Dark Matter properties that can be constrained by current data, and may be tested with the next generation of cosmological surveys.

This talk is part of the Cosmology Lunch series.

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Department of Computer Science (Room TBA, meet at reception for now) Latimer Room , Clare College Room 138, Alison Richard Building, 7 West Road, University of Cambridge, Cambridge CB3 9DT

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