Date:
15. August 2014
Occasion:
Workshop "Modern Cosmology: Early Universe, CMB and LSS", Benasque, Spain
Members involved:
Summary:
I give a brief introduction on some numerical methods which are currently being developed in order to simulate cosmic structure formation in the context of general relativity. These techniques will be useful for the study of extensions/alternatives to the ΛCDM concordance model as far as they may modify structure formation at the non-linear level.