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

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

1998-07-30

arxiv.org/abs/hep-ph/9807553v1

Phys.Lett. B442 (1998) 63-67

Physics

High Energy Physics

High Energy Physics - Phenomenology

LaTeX, uses axodraw style, 7 pages, 1 ps-figure

Scientific paper

10.1016/S0370-2693(98)01269-6

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.

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