CDMS II: A Search for Cold Dark Matter with Cryogenic Detectors at the Soudan Mine

CDMS II：在苏丹矿用低温探测器寻找冷暗物质

• 批准号: 9978911
• 负责人: Bernard Sadoulet
• 金额: $ 880.27万
• 依托单位: University of California-Berkeley
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2000
• 资助国家: 美国
• 起止时间: 2000-01-01 至 2006-12-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=9978911&HistoricalAwards=false
• 关键词: CDMS; II; Search; Cold; Dark

AbstractAST 9978911In the last decade considerable additional evidence has been gathered supporting the hypothesis that at least 90% of the mass in the universe is dark: it does not emit or absorb any form of electromagnetic radiation. Understanding this dark matter has become one of the more central problems in astronomy and cosmology. A number of observations indicate that the predominant form of the dark matter is nonbaryonic, presumably in the form of elementary particles produced in the early universe. Weakly Interactive Massive Particles form a particularly interesting generic class of candidates as there appears to be a convergence between cosmology and particle physics. The direct observation of the interaction of WIMPs in a terrestrial detector would be of tremendous importance to particle physics and cosmology. The observed WIMPs would be particles that reflect physics beyond the Standard Model of strong and electroweak interactions, and the identification of these WIMPs would solve the central problem of dark matter and help us understand the evolution of the early universe and the formation of structure.Because of a long development effort funded both by the National Science Foundation (through the Center for Particle Astrophysics) and the Department Of Energy, the sensor technology exists to provide a great step forward in this type of search, giving the best change for a positive result. The simultaneous measurement of the phonons and the ionization produced by the WIMP interactions provides a powerful discrimination against radioactive background, and this technique is now being utilized at Stanford, in the Cryogenic Dark Matter Search Experiment (CDMS I).This award, which is being supportred jointly by the Division of Astronomical Sciences, the Division of Physics, and the Office of Multidisciplinary Activities, will support construction and operation of a second generation experiment (CDMS II) at a deep site in the Soudan mine in northern Minnesota.

在过去的十年中，已经收集了大量的额外证据来支持宇宙中至少90%的质量是黑暗的假设：它不发射或吸收任何形式的电磁辐射。 了解这种暗物质已经成为天文学和宇宙学中更核心的问题之一。 大量的观测表明，暗物质的主要形式是非重子的，可能是早期宇宙中产生的基本粒子的形式。 弱相互作用大质量粒子形成了一个特别有趣的候选类别，因为宇宙学和粒子物理学之间似乎存在收敛。 在地面探测器中直接观测WIMP的相互作用对粒子物理学和宇宙学将具有巨大的重要性。 观测到的WIMP是反映强相互作用和电弱相互作用标准模型之外的物理学的粒子，这些WIMP的识别将解决暗物质的核心问题，并帮助我们了解早期宇宙的演化和结构的形成。（通过粒子天体物理中心）和能源部，传感器技术的存在为这种类型的搜索提供了一个很大的进步，为积极的结果提供了最好的改变。 同时测量声子和由WIMP相互作用产生的电离提供了对放射性背景的强有力的区分，这种技术目前正在斯坦福大学的低温暗物质搜索实验（CDMS I）中使用。该奖项由天文科学司、物理司和多学科活动办公室联合支持，将支持在明尼苏达州北方的Soudan矿的深部建造和运行第二代实验（CDMS II）。