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Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
对于WIMP暗物质来说,这是真理的时刻
1Institut d'Astrophysique de Paris, UMR 7095-CNRS, Université Pierre et Marie Curie, 98 bis Boulevard Arago, 75014 Paris, France. bertone@iap.fr
Nature
|November 19, 2010
概括
弱相互作用的大质粒子 (WIMPs) 是主要的暗物质候选者. 大强子对撞机及其他地方的实验将很快证实或驳斥它们的存在.
科学领域:
- 宇宙学和粒子物理学的研究.
- 天体粒子物理学的物理学
背景情况:
- 暗物质占宇宙物质含量的85%.
- 暗物质的组成仍然是未知的.
- 弱相互作用的大质粒子 (WIMPs) 是暗物质的突出理论候选者.
研究的目的:
- 突出WIMP作为暗物质候选者的重要性.
- 讨论由于即将到来的实验结果,WIMP理论的关键时刻.
主要方法:
- 粒子物理学的标准模型的理论扩展自然预测WIMP.
- 正在使用大型强子对撞机 (LHC) 进行WIMP的搜索.
- 新一代的天体粒子实验也在探测WIMP的存在.
主要成果:
- 这项研究并没有提出新的实验结果,而是框架了WIMP研究的当前状态.
- 即将进行的实验准备提供支持或反对WIMP的明确证据.
结论:
- 接下来的五到十年对WIMP研究来说是一个关键时期.
- 实验结果将要么证实WIMP是暗物质难题的解决方案,要么导致它们的突出地位下降.
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