English

Super-Natural MSSM

High Energy Physics - Phenomenology 2015-08-05 v1

Abstract

We point out that the electroweak fine-tuning problem in the supersymmetric Standard Models (SSMs) is mainly due to the high energy definition of the fine-tuning measure. We propose super-natural supersymmetry which has an order one high energy fine-tuning measure automatically. The key point is that all the mass parameters in the SSMs arise from a single supersymmetry breaking parameter. In this paper, we show that there is no supersymmetry electroweak fine-tuning problem explicitly in the Minimal SSM (MSSM) with no-scale supergravity and Giudice-Masiero (GM) mechanism. We demonstrate that the ZZ-boson mass, the supersymmteric Higgs mixing parameter μ\mu at the unification scale, and the sparticle spectrum can be given as functions of the universal gaugino mass M1/2M_{1/2}. Because the light stau is the lightest supersymmetric particle (LSP) in the no-scale MSSM, to preserve RR parity, we introduce a non-thermally generated axino as the LSP dark matter candidate. We estimate the lifetime of the light stau by calculating its 2-body and 3-body decays to the LSP axino for several values of axion decay constant faf_a, and find that the light stau has a lifetime ττ~1\tau_{\tilde \tau_1} in [104,100][10^{-4},100] s for an faf_a range [109,1012][10^{9},10^{12}] GeV. We show that our next to the LSP stau solutions are consistent with all the current experimental constraints, including the sparticle mass bounds, B-physics bounds, Higgs mass, cosmological bounds, and the bounds on long-lived charge particles at the LHC.

Keywords

Cite

@article{arxiv.1502.06893,
  title  = {Super-Natural MSSM},
  author = {Guangle Du and Tianjun Li and D. V. Nanopoulos and Shabbar Raza},
  journal= {arXiv preprint arXiv:1502.06893},
  year   = {2015}
}

Comments

32 pages,10 figures and 1 table

R2 v1 2026-06-22T08:36:49.913Z