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Quantifying Limits on CP Violating Phases from EDMs in Supersymmetry

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arxiv 2303.02822 v1 pith:6IT7FVRB submitted 2023-03-06 hep-ph hep-ex

classification hep-phhep-ex
keywords thetaedmslimitssupersymmetriccmssmelectronexperimentalimprovements
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We revisit the calculation of the electron, neutron, and proton electric dipole moments (EDMs) in the constrained minimal supersymmetric standard model (CMSSM). The relatively large mass of the Higgs boson, $m_H \simeq 125$ GeV coupled with the (as yet) lack of discovery of any supersymmetric particle at the LHC, has pushed the supersymmetry breaking scale to several TeV or higher. Though one might expect this decoupling to have relaxed completely any bounds on the two CP violating phases in the CMSSM ($\theta_\mu$ and $\theta_A$), the impressive experimental improvements in the limits on the EDMs (particularly the electron EDM) still allow us to set constraints of order $(0.01 - 0.1)\pi$ on $\theta_A$ and $(0.001 - 0.1)\pi$ on $\theta_\mu$. We also discuss the impact of future improvements in the experimental limits on supersymmetric models.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. The EDM inverse problem: Identifying the sources of CP violation and PQ breaking with electric dipole moments

    hep-ph 2026-04 unverdicted novelty 5.0 of 10

    Six classes of CP-violating operators near the QCD scale produce distinct EDM patterns that enable discrimination of their origins and distinguish high-scale versus low-energy sources of the axion vacuum expectation value.

  2. The EDM inverse problem: Identifying the sources of CP violation and PQ breaking with electric dipole moments

    hep-ph 2026-04 unverdicted novelty 4.0 of 10

    Six classes of CP-violating operators near the QCD scale produce distinct EDM patterns that enable discrimination of their origins and can distinguish high-scale versus low-scale sources of axion VEV.

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