Dark matter, fine-tuning and (g-2)_{\mu} in the pMSSM
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 a...
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| 格式: | Article |
| 語言: | English |
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SciPost
2021-09-01
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| 叢編: | SciPost Physics |
| 在線閱讀: | https://scipost.org/SciPostPhys.11.3.049 |