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• W3204189511 abstract "Very recently, a Fermilab report of muon $g-2$ showed a $4.2sigma$ discrepancy between it and the standard model (SM) prediction. Motivated by this inspiring result and the increasing tension in supersymmetric interpretation of the anomalous magnetic moment, it is argued that in the general next-to-minimal supersymmetric standard model (GNMSSM), a singlino-dominated neutralino can act as a feasible dark matter (DM) candidate in explaining the discrepancy naturally. In this case, the singlino-dominated DM and singlet-dominated Higgs bosons can form a secluded DM sector with $tilde{chi}_1^0tilde{chi}_1^0 to h_s A_s$ responsible for the measured DM relic abundance. when $m_{tilde{chi}_1^0} gtrsim 150~{rm GeV}$ and the Yukawa coupling $kappa$ is around $0.2$. This sector communicates with the SM sector by weak singlet-doublet Higgs mixing, so the scatterings of the singlino-dominated DM with nucleons are suppressed. Furthermore, due to the singlet nature of the DM and the complex mass hierarchy, sparticle decay chains in the GNMSSM are lengthened in comparison with the prediction of the minimal supersymmetric standard model. These characteristics lead to sparticle detection at the Large Hadron Collider (LHC) being rather tricky. This study surveys a specific scenario of the GNMSSM, which extends the $mathbb{Z}_3$-NMSSM by adding an explicit $mu$-term, to reveal the features. It indicates that the theory can readily explain the discrepancy of the muon anomalous magnetic moment without conflicting with the experimental results in DM and Higgs physics, and the LHC searches for sparticles." @default.
• W3204189511 created "2021-10-11" @default.
• W3204189511 creator A5028129237 @default.
• W3204189511 creator A5030611214 @default.
• W3204189511 creator A5046155820 @default.
• W3204189511 creator A5071920735 @default.
• W3204189511 creator A5073905105 @default.
• W3204189511 date "2021-09-28" @default.
• W3204189511 modified "2023-10-17" @default.
• W3204189511 title "Improved $(g-2)_mu$ measurement and singlino dark matter in $mu$-term extended $mathbb{Z}_3$-NMSSM." @default.
• W3204189511 cites W1528104978 @default.
• W3204189511 cites W1545763467 @default.
• W3204189511 cites W1582929838 @default.
• W3204189511 cites W1596934525 @default.
• W3204189511 cites W1964474300 @default.
• W3204189511 cites W1965311100 @default.
• W3204189511 cites W1970296662 @default.
• W3204189511 cites W1987435915 @default.
• W3204189511 cites W1991852818 @default.
• W3204189511 cites W1996218638 @default.
• W3204189511 cites W1997649357 @default.
• W3204189511 cites W2009409441 @default.
• W3204189511 cites W2030066520 @default.
• W3204189511 cites W2031026718 @default.
• W3204189511 cites W2042204882 @default.
• W3204189511 cites W2049023320 @default.
• W3204189511 cites W2050031497 @default.
• W3204189511 cites W2056501192 @default.
• W3204189511 cites W2057404189 @default.
• W3204189511 cites W2061391240 @default.
• W3204189511 cites W2078766197 @default.
• W3204189511 cites W2080912762 @default.
• W3204189511 cites W2081587539 @default.
• W3204189511 cites W2095998354 @default.
• W3204189511 cites W2104244123 @default.
• W3204189511 cites W2106031600 @default.
• W3204189511 cites W2116109970 @default.
• W3204189511 cites W2118179359 @default.
• W3204189511 cites W2129535822 @default.
• W3204189511 cites W2137941090 @default.
• W3204189511 cites W2145413943 @default.
• W3204189511 cites W2145896602 @default.
• W3204189511 cites W2148292621 @default.
• W3204189511 cites W2148311865 @default.
• W3204189511 cites W2170199401 @default.
• W3204189511 cites W2191179926 @default.
• W3204189511 cites W2202858735 @default.
• W3204189511 cites W2419388984 @default.
• W3204189511 cites W2441413825 @default.
• W3204189511 cites W2548110653 @default.
• W3204189511 cites W2559250318 @default.
• W3204189511 cites W2580611012 @default.
• W3204189511 cites W2724561677 @default.
• W3204189511 cites W2729634584 @default.
• W3204189511 cites W2752877928 @default.
• W3204189511 cites W2759987187 @default.
• W3204189511 cites W2790208792 @default.
• W3204189511 cites W2799405389 @default.
• W3204189511 cites W2802950673 @default.
• W3204189511 cites W2805537661 @default.
• W3204189511 cites W2807156318 @default.
• W3204189511 cites W2808176613 @default.
• W3204189511 cites W2886452646 @default.
• W3204189511 cites W2887517691 @default.
• W3204189511 cites W2896054351 @default.
• W3204189511 cites W2900681269 @default.
• W3204189511 cites W2908132890 @default.
• W3204189511 cites W2908326761 @default.
• W3204189511 cites W2908366406 @default.
• W3204189511 cites W2911446281 @default.
• W3204189511 cites W2917282362 @default.
• W3204189511 cites W2923293525 @default.
• W3204189511 cites W2963162504 @default.
• W3204189511 cites W2963206689 @default.
• W3204189511 cites W2963854811 @default.
• W3204189511 cites W2972599699 @default.
• W3204189511 cites W2974453305 @default.
• W3204189511 cites W2978291699 @default.
• W3204189511 cites W2979932679 @default.
• W3204189511 cites W2982621696 @default.
• W3204189511 cites W2993196017 @default.
• W3204189511 cites W2995724601 @default.
• W3204189511 cites W2996362743 @default.
• W3204189511 cites W3022539788 @default.
• W3204189511 cites W3024479057 @default.
• W3204189511 cites W3048175090 @default.
• W3204189511 cites W3082735346 @default.
• W3204189511 cites W3099155575 @default.
• W3204189511 cites W3099275011 @default.
• W3204189511 cites W3099558046 @default.
• W3204189511 cites W3099829108 @default.
• W3204189511 cites W3104738021 @default.
• W3204189511 cites W3105352509 @default.
• W3204189511 cites W3105808240 @default.
• W3204189511 cites W3105997434 @default.
• W3204189511 cites W3111256350 @default.
• W3204189511 cites W3112664937 @default.
• W3204189511 cites W3123237830 @default.
• W3204189511 cites W3124205123 @default.
• W3204189511 cites W3127454881 @default.

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