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Phys. Rev. Lett. 77, 4704–4707 (1996)

Observational Constraints on Open Inflation Models

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Martin White1 and Joseph Silk2
1Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637
2Center for Particle Astrophysics and Departments of Astronomy and Physics, University of California, Berkeley, California 94720

See Also: Erratum

Received 23 August 1996; published in the issue dated 2 December 1996

We discuss observational constraints on models of open inflation. Current data from large-scale structure and the cosmic microwave background prefer models with blue spectra and/or Ω0≥0.3–0.5. Models with minimal anisotropy at large angles are strongly preferred.

© 1996 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.77.4704
DOI:
10.1103/PhysRevLett.77.4704
PACS:
98.80.Cq, 98.65.Dx, 98.70.Vc, 98.80.Es

See Also

Erratum: Martin White and Joseph Silk, Observational Constraints on Open Inflation Models [Phys. Rev. Lett. 77, 4704 (1996)], Phys. Rev. Lett. 78, 3799 (1997).