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arxiv: 1011.5877 · v2 · submitted 2010-11-26 · ✦ hep-th · astro-ph.CO· hep-ph

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Axions as Quintessence in String Theory

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classification ✦ hep-th astro-ph.COhep-ph
keywords axionmodelquintessencefieldhighlystringtheorythroats
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We construct a model of quintessence in string theory based on the idea of axion monodromy as discussed by McAllister, Silverstein and Westphal arXiv:0808.0706. In the model, the quintessence field is an axion whose shift symmetry is broken by the presence of 5-branes which are placed in highly warped throats. This gives rise to a potential for the axion field which is slowly varying, even after incorporating the effects of moduli stabilization and supersymmetry breaking. We find that the resulting time dependence in the equation of state of Dark Energy is potentially detectable, depending on the initial conditions. The model has many very light extra particles which live in the highly warped throats, but these are hard to detect. A signal in the rotation of the CMB polarization can also possibly arise.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Constraining F-theory Model Building with QCD Axions

    hep-th 2026-05 unverdicted novelty 5.0

    F-theory models with the Standard Model spectrum are constrained by QCD axion physics, yielding typical detectable axion masses around 10^{-9} eV and decay constants around 10^{15} GeV in allowed regions.

  2. Constraining F-theory Model Building with QCD Axions

    hep-th 2026-05 unverdicted novelty 5.0

    QCD axions constrain F-theory base threefolds to have rigid or flux-rigidified divisors, yielding typical axion masses around 10^{-9} eV and decay constants near 10^{15} GeV in allowed regions.