Published July 1985 | Version v1
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Inflationary stages in cosmological models with a scalar field

Creators

  • 1. International Centre for Theoretical Physics, Trieste (Italy)
  • 2. Sternberg Astronomical Inst., Moscow (USSR)
  • 3. AN SSSR, Moscow. Inst. Fizicheskikh Problem

Description

Homogeneous cosmological models of Friedmann type in the presence of the massive scalar field are studied. Using qualitative theory of dynamical systems we show that the majority of trajectories in phase space undergoes the inflationary stage. (author)

Availability note (English)

MF available from INIS under the Report Number.

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Additional details

Publishing Information

Imprint Pagination
27 p.
Report number
IC--85/93

INIS

Country of Publication
International Atomic Energy Agency (IAEA)
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
17030018
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
DYNAMICS; EQUATIONS OF MOTION; INFLATIONARY UNIVERSE; PHASE SPACE; SCALAR FIELDS; TRAJECTORIES
Descriptors DEC
COSMOLOGICAL MODELS; DIFFERENTIAL EQUATIONS; EQUATIONS; MATHEMATICAL MODELS; MATHEMATICAL SPACE; MECHANICS; PARTIAL DIFFERENTIAL EQUATIONS; SPACE

Optional Information

Notes
9 refs, 4 figs.