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  Inflation in curved model universes with noncritical density

Hübner, P., & Ehlers, J. (1991). Inflation in curved model universes with noncritical density. Classical and Quantum Gravity, 8(2), 333-346. doi:10.1088/0264-9381/8/2/013.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-5CD0-7 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-5CD1-5
Genre: Journal Article

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333060.pdf (Publisher version), 515KB
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 Creators:
Hübner, Peter1, Author
Ehlers, Jürgen1, Author
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1Geometric Analysis and Gravitation, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, escidoc:24012              

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 Abstract: Non-flat Friedmann-Lemaitre models solving the horizon problem in which, prior to and during inflation, curvature, cosmological constant and radiation are taken into account, are constructed for present density parameter values in the range 0.3<or= Omega 0<or=1.5. The presentation is based on an exact solution to the Lemaitre equation containing the three above-mentioned contributions. Then the influence of matter different from radiation is discussed. The authors also give an example for what happens when the expansion is anisotropic.

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 Dates: 1991-02
 Publication Status: Published in print
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 Identifiers: eDoc: 333060
DOI: 10.1088/0264-9381/8/2/013
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Title: Classical and Quantum Gravity
  Alternative Title : Class. Quant. Grav.
Source Genre: Journal
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Pages: - Volume / Issue: 8 (2) Sequence Number: - Start / End Page: 333 - 346 Identifier: ISSN: 0264-9381