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In this paper we analyze spectra in the phenomenological supersymmetric Standard Model that simultaneously result in the right dark-matter relic density $\Omega_{\rm DM} h^2$, offer an explanation for the $(g-2)_{\mu}$ discrepancy $\Delta a_{\mu}$ and are minimally fine-tuned.
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K. Melnikov and A. Vainshtein, Hadronic light-by-light scattering contribution to the muon anomalous magnetic moment revisited
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F. Mahmoudi, SuperIso v2.3: A Program for calculating flavor physics observables in Supersymmetry
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T. Mibe, Measurement of muon g-2 and edm with an ultra-cold muon beam at j-parc
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2011
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2011
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2016
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M. Drees and J. S. Kim, Minimal natural supersymmetry after the LHC8
2016
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H. Baer, V. Barger, and M. Savoy, Upper bounds on sparticle masses from naturalness or how to disprove weak scale supersymmetry
2016
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The GAMBIT Dark Matter Workgroup
2017
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E. Bagnaschi et al., Likelihood Analysis of the pMSSM11 in Light of LHC 13-TeV Data
2018
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2018
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H. Baer, V. Barger, D. Sengupta, and X. Tata, Is natural higgsino-only dark matter excluded?
2018
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2018
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2018
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G. Colangelo, M. Hoferichter, and P. Stoffer, Two-pion contribution to hadronic vacuum polarization
2019
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2019
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2019
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2020
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Muon 𝐠 − 𝟐 \mathbf{g-2}
2021
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Muon 𝐠 − 𝟐 \mathbf{g-2}
2021
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Muon 𝐠 − 𝟐 \mathbf{g-2}
2021
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CMS Collaboration
2021
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Accessed: 2021-03-24
“Toward a next-generation dark matter search with the PICO-40L bubble chamber.” https://indico.cern.ch/event/606690/contributions/2623446/attachments/1497228/2330240/Fallows_2017_07_24__TAUP__PICO-40L_v1.2.pdf · 2021
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