arXiv · hep-th/0512184
A Planck-scale axion and SU(2) Yang-Mills dynamics: Present acceleration and the fate of the photon
Abstract
From the time of CMB decoupling onwards we investigate cosmological evolution subject to a strongly interacting SU(2) gauge theory of Yang-Mills scale $Λ\sim 10^{-4}$ eV (masquerading as the $U(1)_{Y}$ factor of the SM at present). The viability of this postulate is discussed in view of cosmological and (astro)particle physics bounds. The gauge theory is coupled to a spatially homogeneous and ultra-light (Planck-scale) axion field. As first pointed out by Frieman et al., such an axion is a viable candidate for quintessence, i.e. dynamical dark energy, being associated with today's cosmological acceleration. A prediction of an upper limit $Δt_{m_γ=0}$ for the duration of the epoch stretching from the present to the point where the photon starts to be Meissner massive is obtained: $Δt_{m_γ=0}\sim 2.2$ billion years.
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Francesco Giacosa, Ralf Hofmann. 2006-11-27. A Planck-scale axion and SU(2) Yang-Mills dynamics: Present acceleration and the fate of the photon. https://doi.org/10.1140/epjc%2Fs10052-007-0214-x
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