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Large-Scale Structure in Modified Gravity – Roman Scoccimarro

Date: Fri. March 27th, 2009, 11:30 am-12:30 pm
Location: Rockefeller 221

Cosmic acceleration may be due to modifications of general relativity (GR) at large scales, rather than dark energy. We use analytic techniques and N-body simulations to find out what observational signatures to expect in brane-induced gravity, with focus on new nonlinear effects not present in GR.

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