Non-linear structure formation in modified gravity models

Add to your list(s) Download to your calendar using vCal

• Kazuya Koyama, ICG, University of Portsmouth
• Monday 05 March 2012, 13:00-14:00
• CMS, Pav.B, CTC Common Room (B1.19).

If you have a question about this talk, please contact Dr Sebastien Renaux-Petel.

The discovery of the accelerated expansion of the Universe has come relatively late in our study of the cosmos, but in showing that gravity can act repulsively, it has opened up many new questions about the nature of gravity and what the Universe might contain. Is the acceleration being driven by dark energy? Or is general relativity (GR) itself in error, requiring a modification at large scales to account for the late acceleration? Structure formation in our Universe can be different even if the geometry of the homogeneous and isotropic universe is the same in these two classes of models, offering a possibility to distinguish between them observationally. Non-linear structure formation is complicated by the fifth force that commonly appears in modified gravity models and new techniques are required to analyse it. We will discuss innovative methods to test GR on non-linear scales, building on the recent developments of N-body simulations for modified gravity.

This talk is part of the Cosmology Lunch series.

This talk is included in these lists:

• All CMS events
• CMS Events
• CMS, Pav.B, CTC Common Room (B1.19)
• Cambridge Astronomy Talks
• Cosmology Lunch
• Cosmology lists
• Cosmology, Astrophysics and General Relativity
• DAMTP info aggregator
• Interested Talks
• Kavli Institute for Cosmology Talk Lists
• Priscilla
• bld31

Note that ex-directory lists are not shown.