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Inflation in Generalized Einstein Theories

  • K. Maeda
  • A. L. Berkin
  • J. Yokoyama
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 169)

Abstract

We classify inflationary models into three types: (1) the Einstein gravity theory with inflaton scalar field, (2) modified gravity theories with ordinary matter fluid and (3) the hybrid of these two models. Extended inflation and soft inflation belong to the third class. We then analyze the details of soft inflationary models, which have two scalar fields: one the standard inflaton, whose potential is exponentially coupled to the other field. We consider satisfaction of the inflationary constraints. New inflation works well, with the coupling constant near the values allowed by grand unified theories. For chaotic inflation with a massive inflaton, we find successful inflation without fine-tuning of the coupling constant or initial data.

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References

  1. [1]
    D. La and P.J. Steinhardt, Phys. Rev. Lett. 62, 376 (1989).ADSCrossRefGoogle Scholar
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    A.L. Berkin, K. Maeda, and J. Yokoyama, Phys. Rev. Lett. 65, 141 (1990).ADSCrossRefGoogle Scholar
  3. [3]
    A.L. Berkin and K. Maeda, preprint WU-AP/10/91 (1991).Google Scholar
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    K. Maeda, Phys. Rev. D39, 3159 (1989), and citations within.ADSGoogle Scholar

Copyright information

© Springer Science+Business Media Dordrecht 1991

Authors and Affiliations

  • K. Maeda
    • 1
  • A. L. Berkin
    • 1
  • J. Yokoyama
    • 2
  1. 1.Dept. of PhysicsWaseda UniversityTokyoJapan
  2. 2.Dept. of PhysicsUniversity of TokyoTokyoJapan

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