arXiv · hep-th/9609190
The dilaton as a candidate for dark matter
Abstract
We examine consequences of the stabilization of the dilaton through the axion. An estimate of the resulting dilaton potential yields a relation between the axion parameter $m_a f_{PQ}$ and the average instanton radius, and predicts the ratio between the dilaton mass $m_ϕ$ and the axion mass $m_a$. If we identify the string axion with a Peccei--Quinn axion, then $m_ϕm_{Pl} \sim m_a f_{PQ}$, and the dilaton should be strongly aligned $\sqrt{<ϕ^2>}\leq 10^{-4}m_{Pl}$ at the QCD scale, in order not to overclose the universe.
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Rainer Dick. 1996-10-01. The dilaton as a candidate for dark matter. https://arxiv.org/abs/hep-th/9609190
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