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Breakdown of Chiral Perturbation Theory for the Axion Hot Dark Matter Bound
Luca Di Luzio1,2,3, Guido Martinelli4, Gioacchino Piazza5
1DESY, Notkestraße 85, D-22607 Hamburg, Germany.
Abstract:
We show that the commonly adopted hot dark matter bound on the axion mass m_{a}≲1 eV is not reliable, since it is obtained by extrapolating the chiral expansion in a region where the effective field theory breaks down. This is explicitly shown via the calculation of the axion-pion thermalization rate at the next-to-leading order in chiral perturbation theory. We finally advocate a strategy for a sound extraction of the axion hot dark matter bound via lattice QCD techniques.
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