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gr-qcMar 1, 2007
10
citations (OpenAlex)
authors
  • Vladimir Folomeev
institutions
  • National Academy of Sciences of the Republic of Kyrgyzstan
arXiv abstractPDF
paper

Bianchi type I model with two interacting scalar fields

arXiv:gr-qc/0703004 · doi:10.1142/S0218271807011139

Abstract

The flat anisotropic model of the early Universe is considered. Two interacting scalar fields with special form of potential energy are a source of matter fields. Analytic solutions for inflationary and scalaron stages are found. It is shown that the solutions tend asymptotically to isotropic Friedmann model.

6 pages, 1 figure

References in corpus (8)

  • Towards the Theory of Reheating After Inflation
  • Particle Physics Models of Inflation and the Cosmological Density Perturbation
  • Hybrid Inflation
  • Color defects in a gauge condensate
  • Boson stars from a gauge condensate
  • Quantum Evolution of the Bianchi Type I Model
  • Cosmic string with two interacting scalar fields
  • Thick brane solution in the presence of two interacting scalar fields

Cited by in corpus (6)

  • Star-plus-wormhole systems with two interacting scalar fields
  • Anisotropic chiral cosmology: exact solutions
  • Compact and extended objects from self-interacting phantom fields
  • Dirac procedure and the Hamiltonian formalism for cosmological perturbations in a Bianchi I universe
  • Stochastic Eternal Inflation in a Bianchi Type I Universe
  • Classical and quantum exact solutions for the anisotropic Bianchi type I in multi-scalar field cosmology with an exponential potential driven inflation
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