# Revisiting the SUSY mu problem and its solutions in the LHC era

**Authors:** Kyu Jung Bae, Howard Baer, Vernon Barger, Dibyashree Sengupta

arXiv: 1902.10748 · 2019-06-26

## TL;DR

This paper reviews twenty solutions to the SUSY mu problem, analyzing their compatibility with the Little Hierarchy in light of LHC constraints, and discusses the theoretical and experimental implications of these solutions.

## Contribution

It provides a comprehensive re-evaluation of existing mu problem solutions considering current LHC data and the naturalness of the Little Hierarchy, highlighting the role of symmetries and mechanisms involved.

## Key findings

- Most solutions can accommodate the Little Hierarchy
- Discrete R-symmetries are favored for mu solutions
- Global symmetries face gravity-safety issues

## Abstract

The supersymmetry preserving mu 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 mu problem. Its solution involves two steps: 1. first forbid mu, perhaps via some symmetry, and then 2. re-generate it of order the scale of soft SUSY breaking terms. However, present LHC limits suggest the soft breaking scale m_{soft} lies in the multi-TeV regime whilst naturalness requires mu~ m_{W,Z,h}~ 100 GeV so that a Little Hierarchy (LH) appears with mu << m_{soft}. We review twenty previously devised solutions to the SUSY mu problem and re-evaluate them in light of whether they are apt to support the LH. We organize the twenty solutions according to: 1. solutions from supergravity/superstring constructions, 2. extended MSSM solutions, 3. solutions from an extra local U(1)' and 4. solutions involving Peccei-Quinn (PQ) symmetry and axions. Early solutions would invoke a global Peccei-Quinn symmetry to forbid the mu term while relating the mu 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 (Z_M^R) which emerge as remnants of 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 experimental verification or falsifiability of various solutions to the mu problem. Almost all solutions seem able to accommodate the LH.

## Full text

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## Figures

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## References

114 references — full list in the complete paper: https://tomesphere.com/paper/1902.10748/full.md

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