The consequences for cosmology of the phase transition in which SU(2)×U(1) symmetry is broken in the Weinberg-Salam model are discussed. The qualitative arguments concerning the effect of the phase transition on the baryon-to-entropy ratio that were recently posed by Witten for the case of a Coleman-Weinberg light Higgs boson are confirmed through exact numerical computations, but some quantitative disagreement is found. The computations are extended to the case in which the light Higgs boson is not of the Coleman-Weinberg type and the nature of the phase transition is discussed. Other cosmological effects are considered.
|Original language||English (US)|
|Number of pages||17|
|Journal||Nuclear Physics, Section B|
|State||Published - Mar 16 1981|
All Science Journal Classification (ASJC) codes
- Nuclear and High Energy Physics