• Open Access

Revisiting the SUSY μ problem and its solutions in the LHC era

Kyu Jung Bae, Howard Baer, Vernon Barger, and Dibyashree Sengupta
Phys. Rev. D 99, 115027 – Published 21 June 2019

Abstract

The supersymmetry (SUSY)-preserving μ parameter in SUSY theories is naively expected to be of order the Planck scale while phenomenology requires it to be of order the weak scale. This is the famous SUSY μ problem. Its solution involves two steps: first forbid μ, perhaps via some symmetry, and then regenerate it of order the scale of soft SUSY-breaking terms. However, present LHC limits suggest the soft breaking scale msoft lies in the multi-TeV regime while naturalness requires μmW,Z,h100GeV so that a little hierarchy (LH) appears with μmsoft. We review 20 previously devised solutions to the SUSY μ problem and reevaluate them in light of whether they are apt to support the LH. We organize the 20 solutions as follows: (1) solutions from supergravity/superstring constructions, (2) extended minimal supersymmetric Standard Model solutions, (3) solutions from an extra local U(1) and (4) solutions involving Peccei-Quinn symmetry and axions. Early solutions invoked a global Peccei-Quinn symmetry to forbid the μ term while relating the μ solution to solving the strong CP problem via the axion. We discuss the gravity-safety issue pertaining to global symmetries and the movement instead toward local gauge symmetries or R symmetries, either continuous or discrete. At present, discrete R symmetries of order M (ZMR) which emerge as remnants of the Lorentz symmetry of compact dimensions seem favored. Even so, a wide variety of regenerative mechanisms are possible, some of which relate to other issues such as the strong CP problem or the generation of neutrino masses. We also discuss the issue of the experimental verification or falsifiability of various solutions to the μ problem. Almost all solutions seem able to accommodate the LH.

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  • Received 5 March 2019

DOI:https://doi.org/10.1103/PhysRevD.99.115027

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

Kyu Jung Bae1,*, Howard Baer2,†, Vernon Barger3,‡, and Dibyashree Sengupta2,§

  • 1Center for Theoretical Physics of the Universe, Institute for Basic Science (IBS), Daejeon 34126, Korea
  • 2Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman, Oklahoma 73019, USA
  • 3Department of Physics, University of Wisconsin, Madison, Wisconsin 53706, USA

  • *kyujungbae@ibs.re.kr
  • baer@nhn.ou.edu
  • barger@pheno.wisc.edu
  • §Dibyashree.Sengupta-1@ou.edu

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Issue

Vol. 99, Iss. 11 — 1 June 2019

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