arXiv · 1207.3343
Radiative natural SUSY with a 125 GeV Higgs boson
Abstract
It has been argued that requiring low electroweak fine-tuning (EWFT) along with a (partial) decoupling solution to the 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/second generation scalars (natural SUSY). We show that by starting with multi-TeV first/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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Howard Baer, Vernon Barger, Peisi Huang, Azar Mustafayev, Xerxes Tata. 2012-09-18. Radiative natural SUSY with a 125 GeV Higgs boson. https://doi.org/10.1103/physrevlett.109.161802
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