Gravitational couplings of the inflaton in extended inflation

Richard Holman, Edward W. Kolb, and Yun Wang
Phys. Rev. Lett. 65, 17 – Published 2 July 1990
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Abstract

We discuss a new extended-inflationary scenario evading the difficulties of the original model. Our model can thermalize the energy in the bubble walls by the necessary epoch, and establish a Robertson-Walker frame in the bubble clusters. The essential new ingredient in our model is the observation that the coupling of inflaton to the Jordan-Brans-Dicke field is expected to be different from that of visible matter.

  • Received 12 March 1990

DOI:https://doi.org/10.1103/PhysRevLett.65.17

©1990 American Physical Society

Authors & Affiliations

Richard Holman, Edward W. Kolb, and Yun Wang

  • Department of Physics, Carnegie Mellon University, Pittsburgh, Pennsylvania 15213
  • NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, Illinois 60510
  • Department of Astronomy Astrophysics and Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637

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Vol. 65, Iss. 1 — 2 July 1990

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