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We revise primordial black holes (PBHs) production in the axion-curvaton model, in light of recent developments in the computation of their abundance accounting for non-gaussianities (NGs) in the curvature perturbation up to all orders.
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S. Vagnozzi, Implications of the NANOGrav results for inflation , Mon. Not. Roy. Astron. Soc. 502
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