arXiv · hep-ph/0210402
A Quintessential Axion
Abstract
The model independent axion of string theory has a decay constant of order of the Planck scale. We explore the properties of this quintessence candidate (quintaxion) in the scheme of hidden sector supergravity breakdown. In models allowing for a reasonable $μ$ term, the hidden sector dynamics may lead to an almost flat potential responsible for the vacuum energy of $(0.003 {\rm eV})^4$. A solution to the strong CP-problem is provided by an additional hidden sector pseudoscalar (QCD axion) with properties that make it an acceptable candidate for cold dark matter of the universe.
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Jihn E. Kim, Hans Peter Nilles. 2002-10-29. A Quintessential Axion. https://doi.org/10.1016/s0370-2693(02)03148-9
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