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Updated: May 16, 2026

Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
Radiative natural supersymmetry with a 125 GeV Higgs boson
Howard Baer1, Vernon Barger, Peisi Huang
1Department of Physics and Astronomy, University of Oklahoma, Norman,Oklahoma 73019, USA.
Abstract:
It has been argued that requiring low electroweak fine-tuning (EWFT) along with a (partial) decoupling solution to the supersymmetry (SUSY) flavor and CP problems leads to a sparticle mass spectra characterized by light Higgsinos at 100-300 GeV, sub-TeV third generation scalars, gluinos at a few TeV, and multi-TeV first or second generation scalars (natural SUSY). We show that by starting with multi-TeV first or second and third generation scalars and trilinear soft breaking terms, the natural SUSY spectrum can be generated radiatively via renormalization group running effects. Using the complete 1-loop effective potential to calculate EWFT, significantly heavier third generation squarks can be allowed even with low EWFT. The large negative trilinear term and heavier top squarks allow for a light Higgs scalar in the ~125 GeV regime.
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