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Cosmological Parameters from Cosmic Background Imager Observations and Comparisons with BOOMERANG, DASI, and MAXIMA | | J. L. Sievers
; J. R. Bond
; J. K. Cartwright
; C. R. Contaldi
; B. S. Mason S. T. Myers
; S. Padin
; T. J. Pearson
; U.-L. Pen
; D. Pogosyan
; S. Prunet
; A. C. S. Readhead
; M. C. Shepherd
; P. S. Udomprasert
; L. Bronfman
; W. L. Holzapfel
; J. May
; | | Date: |
23 May 2002 | | Journal: | Astrophys.J. 591 (2003) 599-622 | | Subject: | astro-ph | | Affiliation: | Caltech), J. R. Bond (CITA), J. K. Cartwright (Caltech), C. R. Contaldi (CITA), B. S. Mason (Caltech) S. T. Myers (NRAO), S. Padin (Caltech), T. J. Pearson (Caltech), U.-L. Pen (CITA), D. Pogosyan (CITA), S. Prunet (CITA), A. C. S. Readhead (Caltech), | | Abstract: | We report on the cosmological parameters derived from observations with the Cosmic Background Imager (CBI), covering 40 square degrees and the multipole range 300 < l < 3500. The angular scales probed by the CBI correspond to structures which cover the mass range from 10^14 to 10^17 M_sun, and the observations reveal, for the first time, the seeds that gave rise to clusters of galaxies. These unique, high-resolution observations also show damping in the power spectrum to l ~ 2000, which we interpret as due to the finite width of the photon-baryon decoupling region and the viscosity operating at decoupling. Because the observations extend to much higher l the CBI results provide information complementary to that probed by the Boomerang, DASI, Maxima, and VSA experiments. As the observations are pushed to higher multipoles no anomalies relative to standard models appear, and extremely good consistency is found between the cosmological parameters derived for the CBI observations over the range 610 < l < 2000 and observations at lower l [abridged]. | | Source: | arXiv, astro-ph/0205387 | | Services: | Forum | Review | PDF | Favorites | |
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