Prospects for axion detection in natural SUSY with mixed axion-higgsino dark matter: back to invisible?

被引：24

作者：

Bae, Kyu Jung ^{[1
]}

Baer, Howard ^{[2
]}

Serce, Hasan ^{[2
]}

机构：

[1] Inst for Basic Sci Korea, Ctr Theoret Phys Universe, Daejeon 34051, South Korea

[2] Univ Oklahoma, Dept Phys & Astron, Norman, OK 73019 USA

来源：

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2017年 / 06期

关键词：

axions; dark matter experiments; dark matter theory; supersymmetry and cosmology; STRONG CP PROBLEM; BREAKING; SUPERSYMMETRY; CONSERVATION; CONSTRAINTS; INVARIANCE; SYMMETRY; MASS;

D O I：

10.1088/1475-7516/2017/06/024

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Under the expectation that nature is natural, we extend the Standard Model to include SUSY to stabilize the electroweak sector and PQ symmetry to stabilize the QCD sector. Then natural SUSY arises from a Kim-Nilles solution to the SUSY mu problem which allows for a little hierarchy where mu similar to f(a)(2) /M-P similar to 100-300 GeV while the SUSY particle mass scale m(SUSY) similar to 1 - 10TeV >> mu. Dark matter then consists of two particles: a higgsino-like WIMP and a SUSY DFSZ axion. The range of allowed axion mass values m(a) depends on the mixed axion-higgsino relic density. The range of m(a) is actually restricted in this case by limits on WIMPs from direct and indirect detection experiments. We plot the expected axion detection rate at microwave cavity experiments. The axion-photon-photon coupling is severely diminished by charged higgsino contributions to the anomalous coupling. In this case, the axion may retreat, at least temporarily, back into the regime of near invisibility. From our results, we urge new ideas for techniques which probe both deeper and more broadly into axion coupling versus axion mass parameter space.

引用

页数：17

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