On the cosmological constant problem and inflation in the framework of nonminimal coupling between a scalar field and the gravitation.

Mathematics – Logic

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Cosmology: Inflationary Universe, Cosmological Constant

Scientific paper

In the framework of the classical field theory, homogeneous and isotropic cosmological models are considered the 3-spaces of which are flat. The source of the gravitational field is a Higgs-type scalar field with nonminimal coupling to the gravitational field. The effective cosmological constant of the degenerated ground state compensates an a priori cosmological constant. The investigation concentrates mainly on negative values for the constant b of the nonminimal coupling. Models with a superinflationary and an inflationary stage exist for large -b. For sufficiently small -b only an inflationary stage during a time interval long enough is possible.

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