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By insisting on naturalness in both the electroweak and quantum chromodynamics (QCD) sectors of the  minimal supersymmetric standard model (MSSM), the portrait for dark matter production is seriously modified   from the usual weakly interacting massive particle (WIMP) miracle picture. In supersymmetry (SUSY) models with radiatively-driven naturalness   (radiative natural SUSY or radiative natural SUSY (RNS))  which include a Dine–Fischler–Srednicki–Zhitnitsky (DFSZ)-like solution to the strong charge-conjugation-parity (CP) and SUSY \(\mu\) problems,   dark matter is expected to be an admixture of both axions and higgsino-like WIMPs.   The WIMP/axion abundance calculation requires simultaneous solution of a   set of coupled Boltzmann equations which describe quasi-stable axinos and saxions.  In most of parameter space, axions make up the dominant contribution of dark matter  although regions of WIMP dominance also occur.  We show the allowed range of Peccei-Quinn (PQ) scale \(f_a\) and compare to the values expected  to be probed by the axion dark matter search experiment (ADMX) axion detector in the near future.   We also show WIMP detection rates, which are  suppressed from usual expectations, because now WIMPs comprise only a fraction of the   total dark matter.   Nonetheless, ton-scale noble liquid detectors should be able to probe the entirety  of RNS parameter space. Indirect WIMP detection rates are less propitious since they  are reduced by the square of the depleted WIMP abundance

Supersymmetry with Radiatively-Driven Naturalness: Implications for WIMP and Axion Searches