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In the post-LHC8 era, it is perceived that what is left of SUSY modelparameter space is highly finetuned in the EW sector (EWFT). We discuss howconventional measures overestimate EWFT in SUSY theory. Radiatively-drivennatural SUSY (RNS) models maintain the SUSY GUT paradigm with low EWFT at 10%level, but are characterized by light higgsinos ~100-300 GeV and a thermalunderabundance of WIMP dark matter. Implementing the SUSY DFSZ solution to thestrong CP problem explains the small \mu parameter but indicates dark mattershould be comprised mainly of axions with a small admixture of higgsino-likeWIMPs. While RNS might escape LHC14 searches, we would expect ultimately directdetection of both WIMPs and axions. An e^+e^- collider with \sqrt{s} ~ 500-600GeV should provide a thorough search for the predicted light higgsinos.

Supersymmetry and Dark Matter post LHC8: why we may expect both axion and WIMP detection