| | WMAP Cosmology 101: Cosmological Constant |
 | | The main attraction of the cosmological constant term is that it significantly improves the agreement between theory and observation. |
 | | A cosmological constant term added to the inflationary model, an extension of the Big Bang theory, leads to a model that appears to be consistent with the observed large-scale distribution of galaxies and clusters, with COBE's measurements of cosmic microwave background fluctuations, and with the observed properties of X-ray clusters. |
 | | By characterizing the detailed structure of the cosmic microwave background fluctuations, WMAP should be able to accurately determine the basic cosmological parameters, including the cosmological constant, to better than 5%. |
| map.gsfc.nasa.gov /m_uni/uni_101accel.html (474 words) |