arXiv (All)
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Breaking the axion abundance-isocurvature relation: Scale invariance and high-scale inflation
cosmology-and-nongalactic-astrophysicsgeneral-relativity-and-quantum-cosmologyhigh-energy-physics-phenomenology
A QCD axion accounting for dark matter through pre-inflationary misalignment is strongly constrained by CMB isocurvature bounds, which place the classic axion window in tension with high-scale inflation. The tension arises because the same decay constant controls both the relic abundance and the pri
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