CMB Anisotropies, Large-Scale Structure and the Future

Details CMB Anisotropies, Large-Scale Structure and the Future CMB Anisotropies, Large-Scale Structure and the Future

1995-09-07

arxiv.org/abs/astro-ph/9509035v1

Astronomy and Astrophysics

Astrophysics

9 pages, including 4 figures in a uuencoded self-unpacking shell script. To appear in Proceedings of the ASP Symposium: Cluste

Scientific paper

We are now beginning to learn detailed information about cosmological parameters from the shapes of the matter and radiation power spectra, together with their relative normalization. As more high quality data are gathered from galaxy surveys and from microwave anisotropies, the range of allowed models is expected to get incrementally smaller. The amount of information potentially available from a high-resolution satellite experiment should allow a determination of essentially {\it all} currently discussed cosmological parameters to less than ~10%.

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