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arxiv: 1505.07388 · v1 · pith:ZYMFG567new · submitted 2015-05-27 · ✦ hep-ph · hep-th

Peccei-Quinn Symmetry from Dynamical Supersymmetry Breaking

classification ✦ hep-ph hep-th
keywords breakingpeccei-quinnsupersymmetrydynamicalsymmetryaxiongravitymatter
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The proximity of the Peccei-Quinn scale to the scale of supersymmetry breaking in models of pure gravity mediation hints at a common dynamical origin of these two scales. To demonstrate how to make such a connection manifest, we embed the Peccei-Quinn mechanism into the vector-like model of dynamical supersymmetry breaking a la IYIT. Here, we rely on the anomaly-free discrete Z4R symmetry required in models of pure gravity mediation to solve the mu problem to protect the Peccei-Quinn symmetry from the dangerous effect of higher-dimensional operators. This results in a rich phenomenology featuring a QCD axion with a decay constant of O(10^10) GeV and mixed WIMP/axion dark matter. In addition, exactly five pairs of extra 5 and 5* matter multiplets, directly coupled to the supersymmetry breaking sector and with masses close to the gravitino mass, m3/2 ~ 100 TeV, are needed to cancel the Z4R anomalies.

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