NMSSM neutralino dark matter for CDF II W-boson mass and muon g-2 and the promising prospect of direct detection

被引：17

作者：

Tang, Tian-Peng ^{[1
,2
]}

Abdughani, Murat ^{[1
,3
]}

Feng, Lei ^{[1
,2
,4
]}

Tsai, Yue-Lin Sming ^{[1
]}

Wu, Jian ^{[1
,2
]}

Fan, Yi-Zhong ^{[1
,2
]}

机构：

[1] Chinese Acad Sci, Key Lab Dark Matter & Space Astron, Purple Mt Observ, Nanjing 210033, Peoples R China

[2] Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Peoples R China

[3] Xinjiang Univ, Sch Phys Sci & Technol, Urumqi 830046, Peoples R China

[4] Nanjing Univ, Joint Ctr Particle Nucl Phys & Cosmol, Purple Mt Observ, Nanjing 210093, Peoples R China

来源：

SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY | 2023年 / 66卷 / 03期

基金：

中国博士后科学基金; 中国国家自然科学基金;

关键词：

supersymmetry; dark matter; W-boson; muon g; 2; MAGNETIC-MOMENT; MILKY-WAY; SEARCH; SUPERSYMMETRY;

D O I：

10.1007/s11433-022-2046-y

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Two experiments from the Fermilab, E989 and CDF II, have reported two anomalies for muon g - 2 and W-boson mass that may indicate the new physics at the low energy scale. Here we examine the possibility of a common origin of these two anomalies in the Next-to-Minimal Supersymmetric Standard Model. Considering various experimental and astrophysical constraints such as the Higgs mass, collider data, flavor physics, dark matter relic density, and direct detection experiments, we find that lighter electroweakinos and sleptons can generate sufficient contributions to muon g - 2 and m(W). Moreover, the corresponding bino-like neutralino dark matter mass is in the similar to 180-280 GeV range. Interestingly, the favored dark matter (DM) mass region can soon be entirely probed by ongoing direct detection experiments like PandaX-4T, XENONnT, LUX-ZEPLIN, and DARWIN.

引用

页数：9

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