Open universe from inflation

Journal Article · Fri Sep 15 04:00:00 EDT 1995 · Physical Review, D

DOI:https://doi.org/10.1103/PhysRevD.52.3314· OSTI ID:124184

Bucher, M ^[1]; Goldhaber, A S ^[2]; Turok, N ^[1]

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1. Physics Department, Princeton University, Princeton, New Jersey 08544 (United States)
2. Institute for Theoretical Physics, State University of New York, Stony Brook, New York 11794-3840 (United States)

We present a natural scenario for obtaining an open universe ({Omega}{sub 0}{lt}1) through inflation. In this scenario, there are two epochs of inflationary expansion---an epoch of ``old inflation,`` during which the inflaton field is stuck in a false vacuum, followed by an epoch of ``new inflation,`` during which the inflation field slowly rolls toward its true minimum. During the first epoch, inflation solves the smoothness and horizon problems. Then an open universe (with negative spatial curvature) is created by the nucleation of a single bubble. In effect {Omega} is instantaneously ``reset`` to zero. During the subsequent ``new`` inflation {Omega} rises toward unity. The value of {Omega} today is calculable in terms of the parameters of the potential, and we show that obtaining values significantly different from zero or unity (though within the range 0{lt}{Omega}{lt}1) does not require significant fine-tuning. We compute the spectrum of density perturbations by evolving the Bunch-Davies vacuum modes across the bubble wall into its interior.

• Research Organization: Institute for Advanced Study
• DOE Contract Number: FG02-90ER40542
• OSTI ID: 124184
• Journal Information: Physical Review, D, Journal Name: Physical Review, D Journal Issue: 6 Vol. 52; ISSN PRVDAQ; ISSN 0556-2821
• Country of Publication: United States
• Language: English

Related Subjects

66 PHYSICS
DENSITY
EXPANSION
INFLATION
INFLATIONARY UNIVERSE
PERTURBATION THEORY
POTENTIALS
SPECTRA
VACUUM STATES