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(Mainly) axion dark matter

机译:(主要)轴暗物质

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摘要

The strong CP problem of QCD is at heart a problem of naturalness: why is the FF term highly suppressed in the QCD Lagrangian when it seems necessary to explain why there are three and not four light pions? The most elegant solution posits a spontaneously broken Peccei-Quinn (PQ) symmetry which requires the existence of the axion field a. The axion field settles to the minimum of its potential thus removing the offensive term but giving rise to the physical axion whose coherent oscillations can make up the cold dark matter. Only now are experiments such as ADMX beginning to explore QCD axion parameter space. Since a bonafide scalar particle- the Higgs boson- has been discovered, one might expect its mass to reside at the axion scale f_a ~ 10~(11) GeV. The Higgs mass is elegantly stabilized by supersymmetry: in this case the axion is accompanied by its axino and saxion superpartners. Requiring naturalness also in the electroweak sector implies higgsino-like WIMPs so then we expect mixed axion-WIMP dark matter. Ultimately we would expect detection of both an axion and a WIMP while signals for light higgsinos may show up at LHC and must show up at ILC.
机译:QCD的强烈CP问题是心脏存在自然的问题:为什么在QCD拉格朗尼亚似乎有必要解释为什么有三个而不是四个轻薄的π最优雅的解决方案为需要存在轴场a的自发性破碎的Peccei-Quinn(PQ)对称性。轴场将其稳定在其潜力的最小值,从而消除了令人反感的术语,而是产生相干振荡可以构成冷暗物质的物理轴。只有现在是诸如ADMX开始的实验,开始探索QCD轴参数空间。由于已经发现了Bonafide标量粒子 - 已经发现了Higgs Boson-,因此可以预期其质量驻留在轴级F_A〜10〜(11)GEV。 HIGGS质量通过超对称稳定稳定:在这种情况下,轴伴随其轴突和撒撒撒撒超级分支。在Electroweak Sector中也需要自然暗示Higgsino样的WiMP,因此我们预计我们预计混合轴 - 黑猩猩暗物质。最终我们希望在LHC的LHC中出现的轴和旋轴和一只轴和WIMP的检测,并且必须在ILC上出现。

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