Collaborative Research: Enabling Megawatt Optical Power in Cosmic Explorer

合作研究：在宇宙探测器中实现兆瓦级光功率

• 批准号: 2309007
• 负责人: Stefan Ballmer
• 金额: $ 20.23万
• 依托单位: Syracuse University
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2023
• 资助国家: 美国
• 起止时间: 2023-08-01 至 2026-07-31
• 项目状态: 未结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2309007&HistoricalAwards=false
• 关键词: Collaborative; Research; Enabling; Megawatt; Optical

Gravitational-wave astronomy has opened a new window on the universe. A century after Einstein predicted gravitational waves, the Laser Interferometer Gravitational-wave Observatory (LIGO) has rewarded decades of investment with the first direct observations of gravitational waves from merging black holes and neutron stars. Cosmic Explorer, a concept for a next-generation gravitational-wave observatory in the United States, aims to push the reach of gravitational-wave astronomy to the edge of the observable universe, using proven LIGO technology in a ten times larger facility. Cosmic Explorer will enable transformative discoveries across physics, astronomy, and cosmology, by observing black holes and neutron stars across cosmic time, probing the nature of the most extreme matter in the universe, and exploring questions in gravity and fundamental physics. This award supports research to design an adaptive optical sensing and controls system critical to enabling Cosmic Explorer. The success of Cosmic Explorer will reshape the field of gravitational-wave astrophysics and the futures of current early-career researchers. By clearing a key technological hurdle towards its realization, this award will ensure that gravitational-wave science continues inspiring young scientists across the country to fulfill their potential as the world-leading researchers of the future.To achieve its unprecedented sensitivity, Cosmic Explorer will require much higher circulating laser power (1.5 MW) than has ever been demonstrated in a large interferometer. The objective of this work is to enable laser interferometry at the megawatt scale, by developing the initial design of a Mode Sensing and Control system for Cosmic Explorer capable of overcoming the thermally-induced optical aberrations that limit current detectors. Specifically, Cosmic Explorer’s thermal compensation requirements will be modeled, documenting the degree to which known sources of wavefront error must be sensed and corrected to achieve the detector design sensitivity. Then, current and emerging technological options will be comprehensively assessed, making down-selections where possible, to deliver a detector subsystem conceptual design for optical mode sensing and control. This work supported by this award will feed into the overall detector design, ahead of a conceptual design review anticipated to take place roughly five years from the award start date.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

爱因斯坦预言引力波一个世纪后，引力波天文学打开了一扇新的窗户，激光干涉仪引力波天文台（LIGO）首次对黑洞和中子合并产生的引力波进行了直接观测，这对数十年的投资带来了回报。宇宙探索者是美国下一代引力波天文台的概念，旨在扩大引力波的影响范围。在十倍大的设施中使用经过验证的 LIGO 技术，宇宙探索者将通过在整个宇宙时间内观察黑洞和中子星，探索宇宙的本质，实现物理学、天文学和宇宙学领域的变革性发现。该奖项支持设计自适应光学传感和控制系统的研究，该系统对于宇宙探索者的成功将重塑宇宙。通过扫清实现这一目标的关键技术障碍，该奖项将确保引力波科学继续激励全国各地的年轻科学家发挥其作为世界领先者的潜力。为了实现前所未有的灵敏度，宇宙探索者将需要比大型干涉仪更高的循环激光功率（1.5 MW）。这项工作的目标是实现激光干涉测量。在兆瓦级，通过为宇宙探索者开发模式传感和控制系统的初始设计，该系统能够克服限制电流探测器的热致光学像差，具体而言，将对宇宙探索者的热补偿要求进行建模，记录其程度。必须感测和纠正已知的波前误差源，以达到探测器设计的灵敏度，然后，将全面评估当前和新兴的技术选项，在可能的情况下进行向下选择，以提供探测器子系统概念设计。该奖项支持的这项工作将在概念设计审查之前纳入整体探测器设计，预计从该奖项开始之日起大约五年内进行。该奖项的法定使命是值得支持。通过使用基金会的智力优点和更广泛的影响审查标准进行评估。