Constraining Dark Energy 3 different ways

Details Constraining Dark Energy 3 different ways Constraining Dark Energy 3 different ways

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...202.2309v&link_type=abstract

American Astronomical Society Meeting 202, #23.09; Bulletin of the American Astronomical Society, Vol. 35, p.728

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I will present three different ways to constrain the properties of dark energy. One is based on combining the WMAP observations of the Cosmic microwave background (CMB) with Large Scale Structure surveys, another method exploits stellar ages. The third method cross correlates the primordial CMB signal with the lensing signal and the Rees-Sciama effect. While for the first two methods there are already some results, a new high-resolution CMB experiment will be needed to apply the third method.

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