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Asymmetric Origin for Gravitino Relic Density in the Hybrid Gravity-Gauge Mediated Supersymmetry Breaking

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arxiv 1111.7313 v3 pith:S2356HGA submitted 2011-11-30 hep-ph

classification hep-ph
keywords gravitinoasymmetricmasssupersymmetricdensitymediatedparticlesrelic
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We propose the hybrid gravity-gauge mediated supersymmetry breaking where the gravitino mass is about several GeV. The strong constraints on supersymmetry viable parameter space from the CMS and ATLAS experiments at the LHC can be relaxed due to the heavy colored supersymmetric particles, and it is consistent with null results in the dark matter (DM) direct search experiments such as XENON100. In particular, the possible maximal flavor and CP violations from the relatively small gravity mediation may naturally account for the recent LHCb anomaly. In addition, because the gravitino mass is around the asymmetric DM mass, we propose the asymmetric origin of the gravitino relic density and solve the cosmological coincident problem on the DM and baryon densities \Omega_{\rm DM}:\Omega_{B}\approx 5:1. The gravitino relic density arises from asymmetric metastable particle (AMP) late decay. However, we show that there is no AMP candidate in the minimal supersymmetric Standard Model (SM) due to the robust gaugino/Higgsino mediated wash-out effects. Interestingly, AMP can be realized in the well motivated supersymmetric SMs with vector-like particles or continuous U(1)_R symmetry. Especially, the lightest CP-even Higgs boson mass can be lifted in the supersymmetric SMs with vector-like particles.

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  1. Asymmetric Dark Matter in SUSY with approximate $R-$symmetry

    hep-ph 2025-02 conditional novelty 6.0 of 10

    A supersymmetric model with approximate R-symmetry links the baryon asymmetry to a gravitino dark matter relic, predicting a 5 to 10 GeV gravitino and a multi-TeV sparticle spectrum.

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