Stochastic String Topography and Multivacua
J. W. Moffat

TL;DR
This paper models the string landscape using stochastic equations to explore how vacuum fluctuations might explain the small positive cosmological constant observed in our universe.
Contribution
It introduces a stochastic Langevin framework for string topography and derives a Focker-Planck equation to analyze multivacua in string/M-theory.
Findings
Stochastic fluctuations can produce a small positive cosmological constant.
The model describes non-supersymmetric multivacua in string theory.
Probabilistic landscape of vacua is characterized mathematically.
Abstract
The suggestion that there exist causally disconnected universes or sub-universes to explain the values of physical parameters such as the cosmological constant is discussed. A statistical model of the string landscape/topography is formulated using a stochastic Langevin equation for string and supergravity potentials. A Focker-Planck equation for the probability density of superpotentials is derived and the possible non-supersymmetric multivacua describing string/M-theory topography are investigated. The stochastic fluctuations of the superpotentials and their associated vacuum states can possibly lead to a small positive cosmological constant.
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Taxonomy
TopicsAlgorithms and Data Compression
