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arxiv: 1506.01410 · v2 · pith:MWNLK2ECnew · submitted 2015-06-03 · ✦ hep-ph · astro-ph.CO

μ-Term Hybrid Inflation and Split Supersymmetry

classification ✦ hep-ph astro-ph.CO
keywords supersymmetryinflationmasssplittermgravitinogravityhybrid
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We consider $\mu$-term hybrid inflation which, in its minimal format with gravity mediated supersymmetry breaking, leads to split supersymmetry. The MSSM $\mu$-term in this framework is larger than the gravitino mass $m_G$, and successful inflation requires $m_G$ (and hence also $|\mu|$) $\gtrsim 5 \times 10^7$ GeV, such that the gravitino decays before the LSP neutralino freezes out. Assuming universal scalar masses of the same order as $m_G$, this leads to split supersymmetry. The LSP wino with mass $\simeq$ 2 TeV is a plausible dark matter candidate, the gluino may be accessible at the LHC, and the MSSM parameter $\tan \beta \simeq 1.7$ in order to be compatible with the measured Higgs boson mass. The tensor-to-scalar ratio $r$, a canonical measure of gravity waves, can be as high as $0.001$.

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