  Supersymmetric models which fulfill the conditions of electroweak naturalness
generally contain light higgsinos with mass not too far from m_h ~125 GeV,
while other sparticles can be much heavier. In R-parity conserving models, the
lightest neutralino is then a higgsino-like WIMP (albeit with non-negligible
gaugino components), with thermal relic density well below measured values.
This leaves room for axions to function as co-dark matter particles. The local
WIMP abundance is then expected to be below standard estimates, and direct and
indirect detection rates must be accordingly rescaled. We calculate rescaled
direct and indirect higgsino-like WIMP detection rates in SUSY models that
fulfil the electroweak naturalness condition. In spite of the rescaling, we
find that ton-scale noble liquid detectors can probe the entire higgsino-like
WIMP parameter space, so that these experiments should either discover WIMPs or
exclude the concept of electroweak naturalness in R-parity conserving natural
SUSY models. Prospects for spin-dependent or indirect detection are more
limited due in part to the rescaling effect.
