作者: N. V. Bulatov , R. V. Gorbachev , I. Ya. Aref'eva , S. Yu. Vernov
DOI: 10.1088/0264-9381/31/6/065007
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摘要: We study dynamics of non-minimally coupled scalar field cosmological models with Higgs-like potentials and a negative constant. In these the inflationary stage Universe evolution changes into quasi-cyclic oscillation behaviour Hubble parameter from positive to values. Depending on initial conditions can perform either one or several cycles before become forever.