Physics
Scientific paper
Apr 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005naap.conf...90u&link_type=abstract
NON-ACCELERATOR ASTROPARTICLE PHYSICS. Proceedings of the 7th School. Held 26 July-6 August 2004 in ICTP, Trieste, Italy. Edited
Physics
Scientific paper
With the recent remarkable progresses in our understanding of the dynamics of the Universe and of structure formation, the evidence for non-baryonic dark matter and dark energy has become stronger and stronger. We summarize here the steps that have led to the current picture and the expectations for the future. On the other hand, we are still far from a comprehensive understanding of the dark side of the Universe from a particle physics point of view. We present here some of the most popular frameworks to embed dark energy in a high energy setup, putting emphasis on the fundamental problems which still have to be addressed. For what concerns dark matter, several interesting ideas have been proposed and are being tested, possibly already with some hints that we might be on the right track in the quest for dark matter.
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