Unified Maximally Natural Supersymmetry

preprint2016arXivOpen access

Abstract

Maximally Natural Supersymmetry, an unusual weak-scale supersymmetric extension of the Standard Model based upon the inherently higher-dimensional mechanism of Scherk-Schwarz supersymmetry breaking (SSSB), possesses remarkably good fine tuning given present LHC limits. Here we construct a version with precision SU(2)L×U(1)YSU(2)_{\rm L} \times U(1)_{\rm Y} unification: sin⁡2θW(MZ)≃0.231\sin^2 θ_W(M_Z) \simeq 0.231 is predicted to ±2%\pm 2\% by unifying SU(2)L×U(1)YSU(2)_{\rm L} \times U(1)_{\rm Y} into a 5D SU(3)EWSU(3)_{\rm EW} theory at a Kaluza-Klein scale of 1/R5∼4.4 TeV1/R_5 \sim 4.4\,{\rm TeV}, where SSSB is simultaneously realised. Full unification with SU(3)CSU(3)_{\rm C} is accommodated by extending the 5D theory to a N=4N=4 supersymmetric SU(6)SU(6) gauge theory on a 6D rectangular orbifold at 1/R6∼40 TeV1/R_6 \sim 40 \,{\rm TeV}. TeV-scale states beyond the SM include exotic charged fermions implied by SU(3)EWSU(3)_{\rm EW} with masses lighter than ∼1.2 TeV\sim 1.2\,{\rm TeV}, and squarks in the mass range 1.4 TeV−2.3 TeV1.4\,{\rm TeV} - 2.3\,{\rm TeV}, providing distinct signatures and discovery opportunities for LHC run II.

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