Published June 15, 1991 | Version v1
Journal article

Scale-invariant extended inflation

  • 1. Physics Department, Carnegie Mellon University, Pittsburgh, Pennsylvania 15213 (USA)
  • 2. Department of Astronomy and Astrophysics Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637 (USA)
  • 3. NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, Illinois 60510 (USA)
  • 4. Physics Department and the Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637 (USA)

Description

We propose a model of extended inflation which makes use of the nonlinear realization of scale invariance involving the dilaton coupled to an inflaton field whose potential admits a metastable ground state. The resulting theory resembles the Jordan-Brans-Dicke version of extended inflation. However, quantum effects, in the form of the conformal anomaly, generate a mass for the dilaton, thus allowing our model to evade the problems of the original version of extended inflation. We show that extended inflation can occur for a wide range of inflaton potentials with no fine-tuning of dimensionless parameters required. Furthermore, we also find that it is quite natural for the extended-inflation period to be followed by an epoch of slow-rollover inflation as the dilaton settles down to the minimum of its induced potential

Additional details

Publishing Information

Journal Title
Physical Review, D
Journal Volume
43
Journal Issue
12
Series
Phys. Rev., D.
Journal Page Range
3833-3845
ISSN
0556-2821
CODEN
PRVDA

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
22074710
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
COSMOLOGY; INFLATIONARY UNIVERSE; SCALE INVARIANCE; SYMMETRY BREAKING
Descriptors DEC
COSMOLOGICAL MODELS; INVARIANCE PRINCIPLES; MATHEMATICAL MODELS