Baryon asymmetry in the very early universe

Details Baryon asymmetry in the very early universe Baryon asymmetry in the very early universe

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979phlb...81..416d&link_type=abstract

Physics Letters B, Volume 81, Issue 3-4, p. 416-418.

Physics

25

Scientific paper

We suggest a three stage mechanism for the development of a net baryon excess in the universe. The first phase is an initial heating due to strong gravitational fluctuations during the first 10-43 s. This is followed by a stage in which baryon and CP violating processes produce a large excess via a mechanism suggested by Weinberg. Finally thermalization dissipates most of the initially produced baryon number leaving a small excess.

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