Speaker
Martin Kunz
(Unknown)
Description
* Lambda-CDM and its problems
* canonical scalar field models of dark energy
* parametrisation of the DE equation of state, how to measure it (with special emphasis on using SN-Ia to probe the luminosity distance), current constraints
* models that modify gravity
* impact on perturbations in the Universe (e.g. growth of structure)
* outlook (future experiments, e.g. Euclid)
