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Dark Energy and Dark Matter: Observations, Experiments and Theories
E. Pécontal, T. Buchert, Ph. Di Stefano and Y. Copin (eds)
EAS Publications Series, 36 (2009) 113-126
DOI: 10.1051/eas/0936016
Review of Observational Evidence for Dark Matter in the Universe and in upcoming searches for Dark Stars
K. FreeseMichigan Center for Theoretical Physics, University of Michigan, Ann Arbor, MI 48109, USA
Published online: 30 May 2009
Abstract
Over the past decade, a consensus picture has emerged
in which roughly a quarter of the universe consists of
dark matter. The observational evidence for the existence of
dark matter is reviewed: rotation curves of galaxies, weak
lensing measurements, hot gas in clusters,
primordial nucleosynthesis and microwave background experiments.
In addition, a new line of research on Dark Stars is presented,
which suggests that the first stars to exist in the universe
were powered by dark matter heating rather than by fusion:
the observational possibilities of discovering dark matter in this
way are discussed.
© EAS, EDP Sciences 2009
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