Cosmology from start to finish

Details Cosmology from start to finish Cosmology from start to finish

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006natur.440.1126b&link_type=abstract

Nature, Volume 440, Issue 7088, pp. 1126-1131 (2006).

Mathematics

Logic

7

Scientific paper

Cosmology is undergoing a revolution. With recent precise measurements of the cosmic microwave background radiation, large galaxy redshift surveys, better measurements of the expansion rate of the Universe and a host of other astrophysical observations, there is now a standard, highly constrained cosmological model. It is not a cosmology that was predicted. Unidentified dark particles dominate the matter content of our Universe, and mysteries surround the processes responsible for the accelerated expansion at its earliest moments (inflation?) and for its recent acceleration (dark energy?). New measurements must address the fundamental questions: what happened at the birth of the Universe, and what is its ultimate fate?

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