Slow nucleation rates in Chain Inflation with QCD Axions or Monodromy
arXiv:0810.0228 · doi:10.1103/PhysRevD.79.067302
Abstract
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. 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.
arXiv comment6 pages, 1 figure
References in corpus (9)
- Axions In String Theory
- Double Field Inflation
- Chain Inflation in the Landscape: "Bubble Bubble Toil and Trouble"
- Field dynamics and tunneling in a flux landscape
- Inflating with the QCD Axion
- Conditions for Successful Extended Inflation
- Chain inflation revisited
- Deforming, revolving and resolving - New paths in the string theory landscape
- Density Perturbations in Chain Inflation
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