Towards Understanding the Impact of the Baryon-Dark Matter Relative Velocity on the 2 and 3-Point Correlation Functions

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• Zack Slepian (Harvard)
• Wednesday 17 June 2015, 13:15-13:45
• Sackler Lecture Theatre, IoA.

If you have a question about this talk, please contact ma557.

I will describe recent work to quantify the shift in 2 and 3-point correlation functions induced by the relative velocity, present an analytic approach to deriving the matter transfer function showing why the relative velocity has its spatial structure, and conclude with a new 3-point algorithm offering a significant speed advantage over previous works. 

This talk is part of the Institute of Astronomy Seminars series.

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• Combined External Astrophysics Talks DAMTP
• Cosmology lists
• Cosmology, Astrophysics and General Relativity
• Institute of Astronomy Seminars
• Institute of Astronomy Talk Lists
• Kavli Institute for Cosmology Talk Lists
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• Sackler Lecture Theatre, IoA

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