PSILOGO

Laboratory for Particle Physics (LTP)


LTP Colloquium

Simulating the Universe

Friday, October 24, 2003, 16:00
OFLA/209

Prof. B. Moore, Univ. Zürich

Abstract:
The initial conditions that give rise to structure formation are now well constrained and we know that the Universe is dominated by dark energy and dark matter. However several problems remain: Astronomers have only identified and understood one percent of the Universe and we are also unsure how the matter in the Universe arranges itself into stars, planets and galaxies. Recent supercomputer calculations have allowed us to make substantial progress in these areas.