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Queen's University Infrastructure support for the development of SNOLAB experiments

Queen's University Infrastructure support for the development of SNOLAB experiments
女王大学为 SNOLAB 实验发展提供基础设施支持
批准号:
SAPMR-2014-00004
负责人:
Noble, Anthony
金额:
$10.56万
依托单位:
依托单位国家:
加拿大
项目类别:
Subatomic Physics Envelope - Major Resources Support Program
财政年份:
2014
资助国家:
加拿大
项目状态:
已结题
起止时间:
2014-01-01 至 2015-12-31

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中文摘要
翻译
这项赠款是在女王大学的基础天体粒子物理学研究的支持,与我们的合作者在阿尔伯塔,卡尔顿,劳伦蒂安,蒙特利尔和多伦多的大学,以及在国家实验室TRIUMF和SNOLAB的同事进行。这项研究的目标是设计,建造和操作新的国家的最先进的探测器,将在SNOLAB,新的国际地下科学设施在萨德伯里,安大略选址。这些探测器将提供有关暗物质的性质、难以捉摸的中微子的性质、地球的热容量以及超新星爆炸机制的宝贵信息。 SNO和其他人的重大发现使人们认识到中微子具有质量和不寻常的量子特性。通过在更深层次上理解中微子,我们将了解这种基本粒子的基本性质,它是宇宙中最多产的粒子。这将有助于更好地理解它们在宇宙结构形成和演化中的作用。如果中微子具有正确的性质,就可以解释为什么我们生活在一个由物质而不是反物质主导的宇宙中。中微子也是研究超新星星星坍缩内部运作的探针,并可能被用来研究地核中热量的产生。 我们知道宇宙由大约25%的暗物质组成。它的存在是通过它对星系和宇宙中其他结构的引力效应来推断的,但它还没有被直接探测到。我们不知道它是什么形式的物质。 这笔资金将为位于皇后大学的工程和技术人员提供支持。他们将帮助开发安装在斯诺实验室的复杂探测器。所有这些探测器的一个主要设计要素是需要超低水平的放射性,该合同还将支持一个能够测量各种材料中低水平放射性的设施的运作。这些资源可供所有从事SNOLAB应用的合作机构使用,并将根据优先事项委员会的建议进行分配,该委员会的成员来自加拿大各地的机构。
英文摘要
This grant is in support of fundamental astroparticle physics research at Queen’s University, undertaken with our collaborators at the Universities of Alberta, Carleton, Laurentian, Montreal and Toronto, as well as with colleagues at the national labs TRIUMF and SNOLAB. The goals of this research are to design, build and operate new state-of-the-art detectors which will be sited in SNOLAB, the new International Facility for Underground Science in Sudbury, Ontario. The detectors will provide valuable information on the nature of dark matter, the properties of the elusive neutrino, the thermal heat content of the earth, and the mechanisms of supernovae explosions. The major discoveries by the SNO and others led to the realization that neutrinos have mass and unusual quantum properties. By understanding neutrinos at a deeper level we will learn about basic properties of this fundamental particle, the most prolific in the Universe. This will lead to a better understanding of their role in the formation and evolution of structures within the Universe. With the right properties, neutrinos could explain why we live in a universe dominated by matter, rather than anti-matter. Neutrinos are also a probe into the inner workings of supernovae star collapse, and may be used to study the production of heat in the core of the earth. The Universe is known to be comprised of about 25% dark matter. Its existence is inferred through the gravitational effects it has on galaxies and other structures in the Universe, yet it has not been detected directly. We have little idea what form of matter it is. This funding will provide support for engineering and technical staff located at Queen’s University. They will help develop complex detectors for installation in SNOLAB. A major design element for all these detectors is the need for ultra-low levels of radioactivity and this award will also support the operation of a facility capable of measuring low levels of radioactivity in a wide variety of materials. These resources are available to all collaborations working on SNOLAB applications, and will be allocated in accordance with the recommendations of a Prioritization Board with membership from institutions across Canada.
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PICO Search for Dark Matter with Bubble Chambers
  • 批准号:
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  • 项目类别:
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  • 资助金额:
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  • 财政年份:
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  • 项目类别:
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  • 资助金额:
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  • 财政年份:
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  • 依托单位:
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海外基金