Black Hole Mergers: from simulation to detection

黑洞合并：从模拟到检测

• 批准号: 0140326
• 负责人: Carlos Lousto
• 金额: $ 30万
• 依托单位: The University of Texas at Brownsville
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2002
• 资助国家: 美国
• 起止时间: 2002-09-01 至 2006-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0140326&HistoricalAwards=false
• 关键词: Black; Hole; Mergers; simulation; detection

Gravitational waves are ripples of gravity thrown off by violent interactions of astrophysical bodies. They were first predicted to exist by Einstein in 1916, but because they are weakened by traveling incredibly large distances before reaching Earth, they have not yet been detected. Presently, a number of countries are completing the construction of detectors which might finally see gravitational waves, including the NSF-funded LIGO detectors. The gravitational waves which should be most easily detected by such instruments will come from colliding black holes. Unfortunately, even these events are likely to be undetectable without powerful techniques to extract the gravitational wave data from the instrumental noise. The research funded by this award will use cutting-edge computer simulations to provide partial, but vital, information about the gravitational waves from colliding black holes. This information will then be used to develop powerful new techniques for detecting the gravitational wave signals.The confirmation of Einstein's prediction of gravitational waves is a laudable scientific objective in itself. However, there is also a much greater promise. Gravitational waves can be produced by objects, like black holes, that cannot be directly observed in any other way. Because so little is known about such objects, it is almost certain that new insights into their origins and workings will result from observing them directly for the first time. Furthermore, it is widely believed that gravitational waves will reveal aspects of the universe that have not yet even been conceived of, thus revolutionizing the current picture of the nature of the cosmos itself. While this revolution will take years to realize, this award enables the importantfirst step of predicting what should be sought and how to seek it.

引力波是天体间剧烈相互作用所产生的引力波。 爱因斯坦在1916年首次预测它们的存在，但由于它们在到达地球之前经过了令人难以置信的长距离旅行而被削弱，因此尚未被发现。 目前，一些国家正在完成最终可能看到引力波的探测器的建造，包括NSF资助的LIGO探测器。 最容易被这种仪器探测到的引力波将来自于碰撞的黑洞。 不幸的是，如果没有强大的技术从仪器噪声中提取引力波数据，即使是这些事件也可能无法检测到。该奖项资助的研究将使用尖端的计算机模拟来提供有关碰撞黑洞引力波的部分但至关重要的信息。 这些信息将被用于开发强大的新技术来探测引力波信号。证实爱因斯坦的引力波预测本身就是一个值得称赞的科学目标。然而，还有一个更大的承诺。 引力波可以由像黑洞这样的物体产生，这些物体不能以任何其他方式直接观察到。 由于对这些天体的了解如此之少，几乎可以肯定的是，通过首次直接观察它们，将对它们的起源和运作产生新的见解。 此外，人们普遍认为，引力波将揭示宇宙中甚至还没有被设想到的方面，从而彻底改变目前对宇宙本身性质的看法。 虽然这场革命需要数年时间才能实现，但这个奖项使我们迈出了重要的第一步，预测应该寻求什么以及如何寻求它。