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- W1985395655 abstract "Abstract 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." @default.
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- W1985395655 date "1979-02-01" @default.
- W1985395655 modified "2023-09-24" @default.
- W1985395655 title "Baryon asymmetry in the very early universe" @default.
- W1985395655 cites W2096742001 @default.
- W1985395655 doi "https://doi.org/10.1016/0370-2693(79)90366-6" @default.
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