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C. R. Contaldi (CITA), CBI/BOOMERanG Collaboration
We present the latest results from the BOOMERanG and CBI experiments which chart the angular power spectrum of the Cosmological Microwave Background anisotropies upto multipoles \ell = 3500 .
We investigate the cosmological parameters obtained by including the new data in our parameter fits to a host of CMB datasets. We show how the CMB strongly constrains the curvature of the Universe, the baryon density and the tilt of the primordial power spectrum. We also show how including external constraints from various experiments can help to significantly constrain the density of cold dark matter and cosmological constant.
If you would like more information about this abstract, please follow the link to http://www.astro.caltech.edu/~tjp/CBI/. This link was provided by the author. When you follow it, you will leave the Web site for this meeting; to return, you should use the Back comand on your browser.
The author(s) of this abstract have provided an email address for comments about the abstract: contaldi@cita.utoronto.ca
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Bulletin of the American Astronomical Society, 34
© 2002. The American Astronomical Soceity.