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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| Materiálatiipa: | Artihkal |
| Giella: | English |
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SciPost
2021-09-01
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| Ráidu: | SciPost Physics |
| Liŋkkat: | https://scipost.org/SciPostPhys.11.3.049 |
| _version_ | 1831559931883421696 |
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| author | Melissa van Beekveld, Wim Beenakker, Marrit Schutten, Jeremy De Wit |
| author_facet | Melissa van Beekveld, Wim Beenakker, Marrit Schutten, Jeremy De Wit |
| author_sort | Melissa van Beekveld, Wim Beenakker, Marrit Schutten, Jeremy De Wit |
| collection | DOAJ |
| description | 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. |
| first_indexed | 2024-12-17T05:37:31Z |
| format | Article |
| id | doaj.art-863f020cb15e4335bf3c8415f93a43c8 |
| institution | Directory Open Access Journal |
| issn | 2542-4653 |
| language | English |
| last_indexed | 2024-12-17T05:37:31Z |
| publishDate | 2021-09-01 |
| publisher | SciPost |
| record_format | Article |
| series | SciPost Physics |
| spelling | doaj.art-863f020cb15e4335bf3c8415f93a43c82022-12-21T22:01:34ZengSciPostSciPost Physics2542-46532021-09-0111304910.21468/SciPostPhys.11.3.049Dark matter, fine-tuning and (g-2)_{\mu} in the pMSSMMelissa van Beekveld, Wim Beenakker, Marrit Schutten, Jeremy De WitIn 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.https://scipost.org/SciPostPhys.11.3.049 |
| spellingShingle | Melissa van Beekveld, Wim Beenakker, Marrit Schutten, Jeremy De Wit Dark matter, fine-tuning and (g-2)_{\mu} in the pMSSM SciPost Physics |
| title | Dark matter, fine-tuning and (g-2)_{\mu} in the pMSSM |
| title_full | Dark matter, fine-tuning and (g-2)_{\mu} in the pMSSM |
| title_fullStr | Dark matter, fine-tuning and (g-2)_{\mu} in the pMSSM |
| title_full_unstemmed | Dark matter, fine-tuning and (g-2)_{\mu} in the pMSSM |
| title_short | Dark matter, fine-tuning and (g-2)_{\mu} in the pMSSM |
| title_sort | dark matter fine tuning and g 2 mu in the pmssm |
| url | https://scipost.org/SciPostPhys.11.3.049 |
| work_keys_str_mv | AT melissavanbeekveldwimbeenakkermarritschuttenjeremydewit darkmatterfinetuningandg2muinthepmssm |