2001•arXiv (Cornell University)Open access

Evolution of flat Universe with a cosmological term in relativistic theory of gravitation

V. V. Kiselev

Abstract

We consider the dynamics of tensor and scalar gravitational fields in the relativistic theory of gravitation with the Minkowskian vacuum metric and generalize the formulation to the lifted degeneration of masses. The potential of scalar field is uniquely determined in the presence of cosmological term. We find cosmological inflationary solutions and analyze conditions providing the transition to the regime of hot expanding Universe.

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Key concepts: Physics, Term (time), Gravitation, Universe, Metric expansion of space, Theoretical physics, Classical mechanics, Cosmology