Joint Workshop, ESO Headquarters, Garching, Germany, 20тАУ24 July 2015
The conference will cover both theory and observations of the large-scale structure of the Universe to discuss recent progress and future directions. Measuring the distribution of matter in the Universe as a function of time and space is a powerful probe of cosmology, both for gravity on scales much greater than the conventional tests of General Relativity and the origin of cosmic acceleration. Statistical properties of the matter distribution can also constrain the nature of initial fluctuations, hence the physics of inflation and the neutrino mass.