An RUI Proposal to Investigate Thermal Noise and Higher-Order Statistical Noise in Initial and Advanced LIGO

RUI 研究初始和高级 LIGO 中的热噪声和高阶统计噪声的提案

• 批准号: 0653590
• 负责人: Steven Penn
• 金额: $ 30万
• 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: 2007
• 资助国家: 美国
• 起止时间: 2007-06-01 至 2010-05-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0653590&HistoricalAwards=false
• 关键词: RUI; Proposal; Investigate; Thermal; Noise

This research project focuses on understanding and reducing thermal noise and upconversion noise in Intermediate and Advanced LIGO. These noise sources are the limiting ones in LIGO's central frequency range of 40 - 400 Hz. Thus their reduction has a direct positive impact on LIGO's sensitivity and expected event rate. The PI will explore the fundamental limits to the loss in fused silica and the practically achievable loss limits required for the Advanced LIGO optics. He will investigate new methods and materials for reducing the loss in the mirror coatings for Advanced LIGO. He will explore improved suspension methods for Intermediate LIGO, to see if a modest change may improve LIGO's sensitivity in time for Science Run 6. He will also begin design studies for test mass mirror configuration for third generation gravity wave observatories. Finally he will continue development of a bicoherence monitor to provide a means for detecting upconversion noise, which has become an increasingly important noise source in Initial LIGO.LIGO's success is dependent upon its ability to increase its sensitivity sufficiently to detect gravity waves and to do so at a rate worthy of a true astronomical observatory. The most direct path toward that goal is to reduce the limiting noise sources in LIGO's most sensitive central frequency region. The PI's research is directed precisely at that goal. In addition, the PI's work is conducted at a small liberal arts college, which has allowed undergraduate and even high school students to get involved in this research. In addition the PI also commits significant efforts to public education and international cooperation. He gives a few public lectures each year; he organized the first joint technical meeting between the LIGO and Virgo collaborations; and he serves on the Executive Committee of the American Physical Society's Topical Group on Gravitation.

该研究项目的重点是了解和降低中级和高级LIGO中的热噪声和上转换噪声。 这些噪声源是LIGO中心频率范围40 - 400 Hz的限制性噪声源。 因此，它们的减少对LIGO的灵敏度和预期事件发生率有直接的积极影响。 PI将探索熔融石英中损耗的基本限制以及Advanced LIGO光学器件所需的实际可实现的损耗限制。 他将研究新的方法和材料，以减少先进LIGO反射镜涂层的损失。 他将为Intermediate LIGO探索改进的悬挂方法，看看适度的改变是否可以及时提高LIGO的灵敏度。 他还将开始为第三代重力波观测站测试质量镜配置的设计研究。 最后，他将继续开发一个双相干监测器，以提供一种检测上转换噪声的方法，上转换噪声已成为Initial LIGO中越来越重要的噪声源。LIGO的成功取决于它是否有能力充分提高其灵敏度，以检测重力波，并以真正的天文观测台的速度这样做。 实现这一目标的最直接途径是减少LIGO最敏感的中心频率区域的限制性噪声源。 PI的研究正是针对这一目标。 此外，PI的工作是在一个小型的文科学院进行的，这使得本科生甚至高中生都可以参与这项研究。 此外，PI还在公共教育和国际合作方面做出了重大努力。 他每年都会做一些公开讲座;他组织了LIGO和Virgo合作的第一次联合技术会议;他是美国物理学会引力专题小组的执行委员会成员。