Abstract
By eschewing fine-tuning from the electroweak and QCD sectors of supersymmetry (natural supersymmetry or SUSY), and by invoking the Kim-Nilles solution to the SUSY μ problem, one is lead to models wherein the dark matter is comprised of a mixture of axions and Higgsino-like WIMPs. Over a large range of Peccei-Quinn breaking scale fa∼109-1012 GeV, one then expects about 90%-95% axion dark matter. In such a scenario, both axion and WIMP direct detection may be expected.
| Original language | English |
|---|---|
| Article number | 031701 |
| Journal | Physical Review D - Particles, Fields, Gravitation and Cosmology |
| Volume | 89 |
| Issue number | 3 |
| DOIs | |
| State | Published - 10 Feb 2014 |
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