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Tests of cosmological models constrained by inflation
Abstract
The inflationary scenario requires that the universe have negligible curvature along constant-density surfaces. In the Friedmann-Lemaitre cosmology that leaves us with two free parameters, Hubble's constant H0 and the density parameter Ω0 (or, equivalently, the cosmological constant Λ). The author discusses here tests of this set of models from local and high-redshift observations. The data agree reasonably well with Ω0 ≡ 0.2.
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Metadata
- Authors
- Peebles, P. J. E.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 1984-09
- Volume
- 284
- Pages
- 439
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2016548438
- Cited by
- 500
- References
- 0
- FWCI
- 21.50
- Type
- journal article
- Language
- en
- Open access
- closed
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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