Amplification of hypercharge electromagnetic fields by a cosmological pseudoscalar


The origin of the cosmological baryon asymmetry remains one of the most fundamental open questions in high energy physics, in spite of the effort and attention it has attracted in the last three decades. In 1967 Sakharov noticed [1] that three conditions are essential for the creation of a net baryon number in a previously symmetric universe: 1) baryon non… (More)

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