Evolution of flat universe with a cosmological term in modified Relativistic Theory of Gravitation as a scalar-tensor extension of General Relativity

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dc.creatorKiselev, V. V.
dc.date2001-06-01
dc.date2002-04-04
dc.date.accessioned2026-07-25T18:24:25Z
dc.descriptionWe 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 massless graviton. The potential of scalar field is determined in the presence of cosmological term under clear physical motivations. We find cosmological inflationary solutions and analyze conditions providing the transition to the regime of hot expanding universe.
dc.description23 pages, 3 eps-figures, title extended, arguements added, evolution eqs. unchanged, derivation and treatment of dimensional parameter improved
dc.identifierhttps://arxiv.org/abs/hep-ph/0106003
dc.identifierhttp://arxiv.org/abs/hep-ph/0106003
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/55198
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleEvolution of flat universe with a cosmological term in modified Relativistic Theory of Gravitation as a scalar-tensor extension of General Relativity
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