Can the simplest two-field model of open inflation survive?
- 15 October 1996
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 54 (8) , R4705-R4708
- https://doi.org/10.1103/physrevd.54.r4705
Abstract
We investigate the quantum fluctuations of an inflaton field in a two-field model of one-bubble open inflation. One of the inflatons is assumed to be responsible for the first false vacuum stage of inflation and the other is assumed to be responsible for the second slow-roll stage of inflation. The mass of the second inflaton is assumed to be negligible throughout the whole era of inflation. We find the supercurvature fluctuations are enhanced by the factor given by the ratio of the Hubble constants at false vacuum and true vacuum. This gives a strong constraint on a class of open inflation models. In particular, this implies the simplest two-field model proposed by Linde and Mezhlumian is in trouble.Keywords
All Related Versions
This publication has 10 references indexed in Scilit:
- Quantum fluctuations and CMB anisotropies in one-bubble open inflation modelsPhysical Review D, 1996
- Observational Tests of One-Bubble Open Inflationary Cosmological ModelsThe Astrophysical Journal, 1996
- Inflation with Ω≠1Physical Review D, 1995
- Large-Angle Cosmic Microwave Background Anisotropy in an Open Universe in the One-Bubble Inflationary ScenarioThe Astrophysical Journal, 1995
- Open inflation with an arbitrary false vacuum massPhysical Review D, 1995
- Inflation with variable ΩPhysics Letters B, 1995
- Euclidean vacuum mode functions for a scalar field on open de Sitter spacePhysical Review D, 1995
- Cold dark matter cosmogony in an open universeThe Astrophysical Journal, 1994
- Gravitational effects on and of vacuum decayPhysical Review D, 1980
- Fate of the false vacuum: Semiclassical theoryPhysical Review D, 1977