Gravitational field of the early universe. I: A nonlinear scalar field as a source

zbMath0958.83065arXivgr-qc/9706028MaRDI QIDQ1576159

Sergey Chervon

Publication date: 17 April 2001

Published in: Gravitation \& Cosmology (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/9706028

zbMATH Keywords

self-interacting scalar fieldgravitational field of the early universestandard inflationary model

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Related Items (6)

Comparative analysis of approximate and exact models in inflationary cosmology ⋮ New method of exponential potentials reconstruction based on given scale factor in phantonical two-field models ⋮ The Bianchi IX cosmological models ⋮ An inflationary cosmological model ⋮ Exact solutions in gravity with a sigma model source ⋮ New exact solutions in a chiral model for a planar-symmetry gravitational field

This page was built for publication: Gravitational field of the early universe. I: A nonlinear scalar field as a source