Dark matter, fine-tuning and $(g-2)_{\mu}$ in the pMSSM

van Beekveld, Melissa; Beenakker, Wim; Schutten, Marrit; De Wit, Jeremy

doi:10.21468/SciPostPhys.11.3.049

SciPost Physics

Dark matter, fine-tuning and $(g-2)_{\mu}$ in the pMSSM

Melissa van Beekveld, Wim Beenakker, Marrit Schutten, Jeremy De Wit

SciPost Phys. 11, 049 (2021) · published 7 September 2021

doi: 10.21468/SciPostPhys.11.3.049
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Abstract

In this paper we perform for the first time an in-depth analysis of the spectra in the phenomenological supersymmetric Standard Model that simultaneously offer an explanation for the $(g-2)_{\mu}$ discrepancy $\Delta a_{\mu}$, result in the right dark-matter relic density $\Omega_{\rm DM} h^2$ and are minimally fine-tuned. The resulting spectra may be obtained from [1]. To discuss the experimental exclusion potential for our models, we analyse the resulting LHC phenomenology as well as the sensitivity of dark-matter direct detection experiments to these spectra. We find that the latter type of experiments with sensitivity to the spin-dependent dark-matter\,--\,nucleon scattering cross section $\sigma_{\rm SD,p}$ will probe all of our found solutions.

TY  - JOUR
PB  - SciPost Foundation
DO  - 10.21468/SciPostPhys.11.3.049
TI  - Dark matter, fine-tuning and $(g-2)_{\mu}$ in the pMSSM
PY  - 2021/09/07
UR  - https://www.scipost.org/SciPostPhys.11.3.049
JF  - SciPost Physics
JA  - SciPost Phys.
VL  - 11
IS  - 3
SP  - 049
A1  - van Beekveld, Melissa
AU  - Beenakker, Wim
AU  - Schutten, Marrit
AU  - De Wit, Jeremy
AB  - In this paper we perform for the first time an in-depth analysis of the spectra in the phenomenological supersymmetric Standard Model that simultaneously offer an explanation for the $(g-2)_{\mu}$ discrepancy $\Delta a_{\mu}$, result in the right dark-matter relic density $\Omega_{\rm DM} h^2$ and are minimally fine-tuned. The resulting spectra may be obtained from [1]. To discuss the experimental exclusion potential for our models, we analyse the resulting LHC phenomenology as well as the sensitivity of dark-matter direct detection experiments to these spectra. We find that the latter type of experiments with sensitivity to the spin-dependent dark-matter\,--\,nucleon scattering cross section $\sigma_{\rm SD,p}$ will probe all of our found solutions.
ER  -

@Article{10.21468/SciPostPhys.11.3.049,
	title={{Dark matter, fine-tuning and $(g-2)_{\mu}$ in the pMSSM}},
	author={Melissa van Beekveld and Wim Beenakker and Marrit Schutten and  Jeremy De Wit},
	journal={SciPost Phys.},
	volume={11},
	pages={049},
	year={2021},
	publisher={SciPost},
	doi={10.21468/SciPostPhys.11.3.049},
	url={https://scipost.org/10.21468/SciPostPhys.11.3.049},
}

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Authors / Affiliations: mappings to Contributors and Organizations

See all Organizations.

¹ Melissa van Beekveld,
¹ Wim Beenakker,
¹ Marrit Schutten,
¹ Jeremy De Wit

Funder for the research work leading to this publication

Science and Technology Facilities Council [STFC]