Constraints on Dark Energy from Future Galaxy Cluster Surveys

Details Constraints on Dark Energy from Future Galaxy Cluster Surveys Constraints on Dark Energy from Future Galaxy Cluster Surveys

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aps..apru12008h&link_type=abstract

American Physical Society, April Meeting, 2003, April 5-8, 2003 Philadelphia, Pennsylvania, MEETING ID: APR03, abstract #U12.008

Physics

Scientific paper

I will discuss constraints that can be derived on the energy densitities of dark matter and dark energy from future surveys of hundreds or thousands of galaxy clusters. I will discuss X-ray and microwave (Sunyaev-Zeldovich effect, SZE) surveys, and the statistical constraints available from both the redshift distribution and from the spatial clustering of galaxy clusters. I will also discuss possible systematic errors, and ways of controlling them by using the X-ray and SZE data in combination.

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