Published March 15, 2009 | Version v1
Journal article

Slow nucleation rates in chain inflation with QCD axions or monodromy

  • 1. Michigan Center for Theoretical Physics, University of Michigan, Ann Arbor, Michigan 48109-1040 (United States)

Description

The previous proposal (by two of us) of chain inflation with the QCD axion is shown to fail. The proposal involved a series of fast tunneling events, yet here it is shown that tunneling is too slow. We calculate the bubble nucleation rates for phase transitions in the thick wall limit, approximating the barrier by a triangle. A similar problem arises in realization of chain inflation in the string landscape that uses series of minima along the monodromy staircase around the conifold point. The basic problem is that the minima of the potential are too far apart to allow rapid enough tunneling in these two models. We entertain the possibility of overcoming this problem by modifying the gravity sector to a Brans-Dicke theory. However, one would need extremely small values for the Brans-Dicke parameter in the early universe. Many successful alternatives exist, including other axions (with mass scales not set by QCD) or potentials with comparable heights and widths that do not suffer from the problem of slow tunneling and provide successful candidates for chain inflation.

Additional details

Publishing Information

Journal Title
Physical Review. D, Particles Fields
Journal Volume
79
Journal Issue
6
Journal Page Range
p. 067302-067302.4
ISSN
0556-2821
CODEN
PRVDAQ

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
41011048
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Descriptors DEI
AXIONS; COMPUTERIZED SIMULATION; GRAVITATION; INFLATION; MASS; NUCLEATION; PHASE TRANSFORMATIONS; POTENTIALS; QUANTUM CHROMODYNAMICS; TUNNEL EFFECT
Descriptors DEC
BOSONS; ELEMENTARY PARTICLES; FIELD THEORIES; GOLDSTONE BOSONS; POSTULATED PARTICLES; QUANTUM FIELD THEORY; SIMULATION

Optional Information

Notes
(c) 2009 The American Physical Society