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REMOVING THE COSMOLOGICAL BOUND ON THE AXION SCALE

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

5 Pith papers citing it
abstract

The current cosmological bound on the invisible axion scale may be avoided in the class of theories in which the gauge coupling constant is determined through the expectation value of some scalar field (e.g. moduli in supergravity and string theories). This leads to the cosmological scenario different from that of the standard invisible axion, since the initial values of the fields are usually far away from their true minima, allowing for the color group becoming strong in the very early universe and fixing the axion field to its minimum. The effect disappears as soon as scalar field adjusts to its present value, but the above is enough to ensure that the deviation of the axion expectation value from the minimum is negligible at the moment of the QCD phase transition and thus to eliminate the troublesome coherent oscillations. This may imply that the standard axion window does not necessarily hold in generic supergravity theories. The above observation may open a natural possibility for the existence of the axion resulting from the GUT or R-symmetry breaking.

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2026 4 2020 1

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representative citing papers

An Intermediate Scale R-axion \& the QCD Axion

hep-th · 2026-07-07 · conditional · novelty 7.0

A mixed F- and D-term uplift in supergravity evades the Planckian lower bound on the R-axion decay constant, allowing it to be the QCD axion and dark matter.

The landscape of QCD axion models

hep-ph · 2020-03-02 · unverdicted · novelty 2.0

Review classifies QCD axion models extending the standard mass-coupling window and updates bounds from cosmology, astrophysics, and experiments.

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