English

$\mu$-Term Hybrid Inflation and Split Supersymmetry

High Energy Physics - Phenomenology 2018-02-01 v2 Cosmology and Nongalactic Astrophysics

Abstract

We consider μ\mu-term hybrid inflation which, in its minimal format with gravity mediated supersymmetry breaking, leads to split supersymmetry. The MSSM μ\mu-term in this framework is larger than the gravitino mass mGm_G, and successful inflation requires mGm_G (and hence also μ|\mu|) 5×107\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 mGm_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 tanβ1.7\tan \beta \simeq 1.7 in order to be compatible with the measured Higgs boson mass. The tensor-to-scalar ratio rr, a canonical measure of gravity waves, can be as high as 0.0010.001.

Keywords

Cite

@article{arxiv.1506.01410,
  title  = {$\mu$-Term Hybrid Inflation and Split Supersymmetry},
  author = {Nobuchika Okada and Qaisar Shafi},
  journal= {arXiv preprint arXiv:1506.01410},
  year   = {2018}
}

Comments

10 pages, 5 figures, some minor changes

R2 v1 2026-06-22T09:46:56.087Z