An RUI Proposal to Study Thermal Noise and Bilinear Noise in LIGO and Advanced LIGO

RUI 研究 LIGO 和高级 LIGO 中热噪声和双线性噪声的提案

• 批准号: 1002585
• 负责人: Steven Penn
• 金额: $ 35.5万
• 依托单位: Hobart and William Smith Colleges
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2010
• 资助国家: 美国
• 起止时间: 2010-07-01 至 2014-06-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1002585&HistoricalAwards=false
• 关键词: RUI; Proposal; Study; Thermal; Noise

This award supports research to overcome noise sources that are expected to limit the sensitivity of Advanced LIGO. The high-index of refraction coating material to be used initially in Advanced LIGO is the main source of thermal noise. Past research to determined the source of excess loss in a low-index coating material allowed demonstration of how it may be reduced or eliminated. These studies of low-index material provided important indicators to guide the search for the necessary high-index coating but with low mechanical loss. LIGO scientists have studied and reduced the multitude of sources of noise that directly couple into the interferometer, thereby exposing indirect, bilinear noise processes, such as up-conversion of noise produced outside LIGO's band of sensitive frequencies into that band. Bicoherence provides a measure of such bilinear coupling while being insensitive to Gaussian noise. Development of a data monitor for bicoherence will continue under this award. Once identified, this noise can be monitored and if possible, eliminated. The bicoherence calculation engine could be adapted eventually to search for gravitational waves, since inspiral and burst signals both have nonzero bicoherence.Advanced LIGO, which is scheduled to be fully operational by 2015, has been designed with a sensitivity to allow it to make regular observations of gravitational waves. Improvement in Advanced LIGO sensitivity through improved optical coatings and amelioration of up-conversion noise will allow achievement of the greatest discovery potential. The PI plans to involve several undergraduates in his research. This matches well with Hobart and William Smith 9HWS0 Colleges' ongoing effort to expand their science program. The opportunity to work in research programs like LIGO at HWS is helping to increase the number of physics majors and to change their attitude about a career in physics.

该奖项支持研究克服预计会限制高级 LIGO 灵敏度的噪声源。 Advanced LIGO 最初使用的高折射率折射涂层材料是热噪声的主要来源。过去的研究确定了低折射率涂层材料中过量损耗的来源，从而证明了如何减少或消除这种损耗。这些低折射率材料的研究为指导寻找必要的高折射率涂层但机械损失低提供了重要指标。 LIGO 科学家研究并减少了直接耦合到干涉仪中的众多噪声源，从而暴露了间接双线性噪声过程，例如将 LIGO 敏感频段之外产生的噪声上转换到该频段。双相干性提供了这种双线性耦合的度量，同时对高斯噪声不敏感。该奖项将继续开发双相干数据监视器。一旦识别出来，就可以监控这种噪音，如果可能的话，可以消除噪音。双相干计算引擎最终可以用于搜索引力波，因为吸气信号和突发信号都具有非零双相干性。高级 LIGO 计划于 2015 年全面投入运行，其设计的灵敏度使其能够进行定期观测引力波。通过改进光学涂层和改善上转换噪声来提高先进 LIGO 的灵敏度，将实现最大的发现潜力。 PI 计划让几名本科生参与他的研究。 这与霍巴特和威廉史密斯 9HWS0 学院不断努力扩大其科学项目非常吻合。在 HWS 参与 LIGO 等研究项目的机会有助于增加物理专业学生的数量，并改变他们对物理学职业的态度。