# GUT-inspired MSSM in light of muon $g-2$ and LHC results at   $\sqrt{s}=13$ TeV

**Authors:** Hieu Minh Tran, Huong Thu Nguyen

arXiv: 1812.11757 · 2019-02-28

## TL;DR

This paper explores a GUT-inspired MSSM model that addresses the muon g-2 anomaly and complies with recent LHC constraints, identifying viable parameter regions for future experimental tests at the LHC and E989.

## Contribution

It provides a detailed analysis of the minimal SUSY model with universal gaugino masses, integrating muon g-2 and LHC data to narrow down the parameter space for light SUSY particles.

## Key findings

- Allowed windows for neutralino and smuon masses identified.
- Model remains viable for small mass regions testable at LHC Run 3.
- Future E989 measurements will further constrain the parameter space.

## Abstract

The recent results of the LHC search for electroweak production of supersymmetric (SUSY) particles at $\sqrt{s}=13$ TeV have shown improved lower limits for their masses. In addition, the projected experiment E989 will be able to measure the muon anomalous magnetic moment precisely so that the experimental uncertainty can be reduced by a factor of four. It was pointed out that if the center value of the muon $g-2$ remains unchanged the deviation between the standard model (SM) prediction and the experimental value will be as large as 7.0$\sigma$. Such a large deviation will be solid evidence for new physics beyond the SM. Motivated by these results, we investigate the minimal SUSY extension of the SM with universal gaugino masses at the grand unified scale in the light of the muon $g-2$ and the updated LHC constraints. The squarks are assumed to be heavy and decoupled from physics at low energy scales to resemble the SM-like Higgs boson mass of 125 GeV and other bounds for squark masses at the LHC. We have pinned down allowed windows for the lightest neutralino and the smuon masses as well as other input parameters relevant to the light SUSY sector. The expected results of the E989 experiment play a crucial role in narrowing these windows. The viability of the model for small mass regions can be tested at the LHC Run 3 and the High Luminosity LHC in the near future.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1812.11757/full.md

## Figures

8 figures with captions in the complete paper: https://tomesphere.com/paper/1812.11757/full.md

## References

43 references — full list in the complete paper: https://tomesphere.com/paper/1812.11757/full.md

---
Source: https://tomesphere.com/paper/1812.11757