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We show that the weakly interacting massive particle (WIMP) scenario ofproton-philic spin-dependent inelastic dark matter can still provide a viableexplanation of the observed DAMA effect in compliance with the constraints fromother experiments. We also show that, although the COSINE-100 collaboration hasrecently tested the DAMA effect using the same target material, for the timebeing the comparison between DAMA and COSINE-100 still depends on theparticle-physics model.

Is a WIMP explanation of the DAMA modulation effect still viable?