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Full text | |
Author(s): |
Lima, J. A. S.
;
Holanda, R. F. L.
;
Cunha, J. V.
;
Alimi, JM
;
Fuzfa, A
Total Authors: 5
|
Document type: | Journal article |
Source: | INVISIBLE UNIVERSE INTERNATIONAL CONFERENCE; v. 1241, p. 6-pg., 2010-01-01. |
Abstract | |
The present cosmic accelerating stage is discussed through a new kinematic method based on the Sunyaev-Zel'dovich effect (SZE) and X-ray surface brightness data from galaxy clusters. By using the SZE/X-ray data from 38 galaxy clusters in the redshift range 0.14 <= z <= 0.89 [Bonament et al., Astrop. J. 647, 25 (2006)] it is found that the present Universe is accelerating and that the transition from an earlier decelerating to a late time accelerating regime is relatively recent. The ability of the ongoing Planck satellite mission to obtain tighter constraints on the expansion history through SZE/X-ray angular diameters is also discussed. Our results are fully independent on the validity of any metric gravity theory, the possible matter-energy contents filling the Universe, as well as on the SNe Ia Hubble diagram from which the presenting accelerating stage was inferred. (AU) | |
FAPESP's process: | 04/13668-0 - Cosmology in the era of precision: dark energy, dark matter and background cosmic radiation |
Grantee: | Jose Ademir Sales de Lima |
Support Opportunities: | Research Projects - Thematic Grants |