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Article overview
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Constraints on dark energy from Chandra observations of the largest relaxed galaxy clusters | S.W. Allen
; R.W. Schmidt
; H. Ebeling
; A.C. Fabian
; L. van Speybroeck
; | Date: |
18 May 2004 | Journal: | Mon.Not.Roy.Astron.Soc. 353 (2004) 457 | Subject: | astro-ph | Affiliation: | IoA Cambridge), R.W. Schmidt (Potsdam University), H. Ebeling (IfA, Hawaii), A.C. Fabian (IoA Cambridge), L. van Speybroeck (CfA | Abstract: | We present constraints on the mean dark energy density, Omega_X and dark energy equation of state parameter, w_X, based on Chandra measurements of the X-ray gas mass fraction in 26 X-ray luminous, dynamically relaxed galaxy clusters spanning the redshift range 0.07-1, the same data require w_X<-0.7 at 95 per cent confidence. Similar results on the mean matter density and dark energy equation of state parameter, Omega_m=0.24pm0.04 and w_X=-1.20^{+0.24}_{-0.28}, are obtained by replacing the CMB data with standard priors on the Hubble constant and mean baryon density and assuming a flat geometry. | Source: | arXiv, astro-ph/0405340 | Services: | Forum | Review | PDF | Favorites |
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