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D. Loomba (University of New Mexico)
The current best-fit cosmological model will be summarized together with observations that support it. Prospects for advancing our knowledge in this field look great, in part due to significant experimental improvements in a number of areas. This is particularly true of dark matter search experiments and probes of the Cosmic Microwave Background Radiation, which will be discussed.
The author(s) of this abstract have provided an email address for comments about the abstract: dloomba@unm.edu
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Bulletin of the American Astronomical Society, 34
© 2002. The American Astronomical Soceity.