Light dark matter in NMSSM and implication on Higgs phenomenology

作者： Cao,J ¹ Hikasa,K ¹ Wang,W ¹ Yang,JM ¹ Hikasa,K ² Wang,W ³ Yang,JM ⁴
作者单位：

1. Henan Normal U.

2. Tohoku U.

3. Beijing U. of Tech.

4. Beijing, Inst. Theor. Phys.
提交时间：2016-12-28 10:57:05

摘要: For the experimental search of neutralino dark matter, it is important to know its allowed mass and scattering cross section with the nucleon. In order to figure out how light a neutralino dark matter can be predicted in low energy supersymmetry, we scan

dark matter: relic density scale: TeV Higgs particle: mass DAMA CERN LHC Coll supersymmetry neutralino: mass minimal supersymmetric standard model: parameter space neutralino: relic density Higgs particle: decay superfield: chiral dark matter: mass dark m

分类： 物理学物理学 >> 基本粒子与场物理学
引用： ChinaXiv:201612.00449 (或此版本 ChinaXiv:201612.00449V1)
DOI:10.12074/201612.00449V1
CSTR:32003.36.ChinaXiv.201612.00449.V1
推荐引用方式： Cao,J,Hikasa,K,Wang,W,Yang,JM,Hikasa,K,Wang,W,Yang,JM.(2016).Light dark matter in NMSSM and implication on Higgs phenomenology.中国科学院科技论文预发布平台.[ChinaXiv:201612.00449] (点此复制)

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2016-12-28 10:57:05

ChinaXiv:201612.00449V1

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