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Dark energy from the string axiverse

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
abstract

String theories suggest the existence of a plethora of axion-like fields with masses spread over a huge number of decades. Here we show that these ideas lend themselves to a model of quintessence with no super-Planckian field excursions and in which all dimensionless numbers are order unity. The scenario addresses the "why now" problem, i.e., why has accelerated expansion begun only recently, by suggesting that the onset of dark-energy domination occurs randomly with a slowly decreasing probability per unit logarithmic interval in cosmic time. The standard axion potential requires us to postulate a rapid decay of most of the axion fields that do no become dark energy. The need for these decays is averted, though, with the introduction of a slightly modified axion potential. In either case, a Universe like ours arises in roughly 1 in 100 universes. The scenario may have a host of observable consequences.

years

2026 2

verdicts

UNVERDICTED 2

representative citing papers

Bounding axion dark energy

astro-ph.CO · 2026-04-10 · unverdicted · novelty 6.0

An analytic bound on axion parameters in thawing quintessence is derived independently of initial conditions and used with cosmological observations plus quantum gravity constraints to exclude large regions of axion dark energy parameter space.

Constraining F-theory Model Building with QCD Axions

hep-th · 2026-05-05 · unverdicted · novelty 5.0 · 2 refs

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.

citing papers explorer

Showing 2 of 2 citing papers.

  • Bounding axion dark energy astro-ph.CO · 2026-04-10 · unverdicted · none · ref 38

    An analytic bound on axion parameters in thawing quintessence is derived independently of initial conditions and used with cosmological observations plus quantum gravity constraints to exclude large regions of axion dark energy parameter space.

  • Constraining F-theory Model Building with QCD Axions hep-th · 2026-05-05 · unverdicted · none · ref 41 · 2 links · internal anchor

    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.