Dynamical evolution of a Higgs field in the inflationary stage of universe

Details Dynamical evolution of a Higgs field in the inflationary stage of universe Dynamical evolution of a Higgs field in the inflationary stage of universe

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984phlb..142...18s&link_type=abstract

Physics Letters B, Volume 142, Issue 1-2, p. 18-22.

Physics

8

Scientific paper

Numerical simulation of the evolution of the adjoint Higgs field in the new inflationary universe scenario based on the SU(5) GUT model with the Coleman-Weinberg potential is carried out by introducing a suitable viscosity term in the equation of motion. It is found that in order for a consistent scenario of the universe without too large density inhomogeneity to be constructed, the value of viscosity should lie in an appropriate range.

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