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One Bubble Inflation

Published online by Cambridge University Press:  25 May 2016

Takahiro Tanaka
Takahiro Tanaka*
Affiliation:
Department of Earth and Space Science, Graduate School of Science, Osaka University, Toyonaka 560, Japan

Abstract

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Evaluating the temperature fluctuation in the cosmic microwave background radiation, the viability of the one bubble inflation scenario is studied. It is shown that it is possible to construct a model which explains the creation of an open universe.

Information

Type
V. Cosmological Models
Information
Symposium - International Astronomical Union , Volume 183: Cosmological Parameters and the Evolution of the Universe , 1999 , pp. 303 - 308
Copyright
Copyright © Kluwer 1999 

References

Garriga, J., Montes, X., Sasaki, M. and Tanaka, T. (1997) Canonical Quantization of Cosmological perturbation in the One Bubble Open Universe, astro-ph/9706229 Google Scholar
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Sasaki, M., Tanaka, T. and Yakushige, T. (1997) Wall fluctuation modes and tensor CMB anisotropy in open inflation models, Phys. Rev., D 56, 616–624 Google Scholar
Tanaka, T. and Sasaki, M. (1997) The Spectrum of Gravitational Wave Perturbations in the One-Bubble Open Inflationary Universe, Prog. Theor. Phys., 97, 243–262 CrossRefGoogle Scholar
Yamamoto, K., Sasaki, M. and Tanaka, T. (1996) Quantum fluctuations and CMB anisotropies in one-bubble open inflation models, Phys. Rev., D 54, 5031–5048 Google Scholar