A Renormalization Group Approach to the Cosmological Constant Problem
arXiv:0708.4374
Abstract
In an earlier paper, it is proposed that, due to resonance tunneling effect, tunneling from a large cosmological constant site in the stringy comic landscape can be fast, while tunneling from a small site may take exponentially long time. Borrowing the renormalization group analysis of the conductance in the Anderson localization transition, we treat the landscape as a multi-dimensional random potential and find that the vastness of the landscape leads to a sharp transition at a small critical value from fast tunneling for to suppressed tunneling for . Mobility in the landscape makes eternal inflation highly unlikely. As an illustration, we find that can easily be exponentially small compared to the string/Planck scale. These properties may help us in finding a qualitative understanding why today's dark energy is so small.
25 pages, 3 figures; new appendices and references added
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Cited by in corpus (12)
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- Rapid Tunneling and Percolation in the Landscape
- The Cosmological Constant Problem and Inflation in the String Landscape
- Resonant Tunneling in Superfluid Helium-3
- Resonant Tunneling in Scalar Quantum Field Theory
- Coleman-de Luccia Tunneling and the Gibbons-Hawking Temperature
- Decay of an inhomogeneous state via resonant tunnelling
- A Smooth Landscape: Ending Saddle Point Inflation Requires Features to be Shallow
- Hawking-Moss Tunneling with a Dirac-Born-Infeld Action
- New Non-Trivial Vacuum Structures in Supersymmetric Field Theories
- Tunneling in Theories with Many Fields
- Topics in vacuum decay (Ph.D Thesis)