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Cosmology with non-minimal scalar field: graceful entrance into inflation

We propose a scenario of the beginning of inflation in which the non-vacuum value of the scalar field that drives inflation develops dynamically due to the non-minimal coupling to gravity. In this scenario, inflation emerges as an intermediate stage of the evolution of the Universe, well after the Planck epoch, from a fairly general initial state.

preprint1998arXivOpen access
M. V. LibanovV. A. RubakovP. G. Tinyakov
astro-phhep-ph
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M. V. LibanovV. A. RubakovP. G. Tinyakov

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