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