Baryogenesis in the Inflationary Universe

Details Baryogenesis in the Inflationary Universe Baryogenesis in the Inflationary Universe

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pthph..74..405s&link_type=abstract

Progress of Theoretical Physics, Vol. 74, No. 2, pp. 405-408

Physics

4

Scientific paper

Baryogenesis in the inflationary universe is investigated in the standard SU(5) GUT. It is shown that Ti >~ 1011GeV (Ti is the reheating temperature) is required to explain the observed baryon to entropy ratio (nB/s), and that the sign of nB/s depends on Ti.

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