Dynamics of phase transition in the new inflationary universe scenario and generation of perturbations

Details Dynamics of phase transition in the new inflationary universe scenario and generation of perturbations Dynamics of phase transition in the new inflationary universe scenario and generation of perturbations

Nov 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982phlb..117..175s&link_type=abstract

Physics Letters B, Volume 117, Issue 3-4, p. 175-178.

Physics

1272

Scientific paper

Dynamics of non-equilibrium phase transition in the early universe is investigated. The transition is triggered by vacuum fluctuations of a Higgs scalar field which determine the duration of an intermediate inflationary stage and the amplitude of adiabatic perturbations. This amplitude ranges from g2 to one and more depending on scale that presents a serious problem for the inflationary scenario.

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