Gravitational Radiation and Relativistic Astrophysics

引力辐射和相对论天体物理学

• 批准号: 0601459
• 负责人: Kip Thorne
• 金额: $ 175万
• 依托单位: California Institute of Technology
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2006
• 资助国家: 美国
• 起止时间: 2006-06-01 至 2011-05-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0601459&HistoricalAwards=false
• 关键词: Gravitational; Radiation; Relativistic; Astrophysics

Theoretical and computational research will be carried out in support of LIGO, the Laser Interferometer Gravitational Wave Observatory: (1) Research close to experiment, e.g. analysis of and methods to reduce thermal noise, light scattering noise, and opto- mechanical instabilities. (2) Development of numerical-relativity tools for simulating gravitational-wave sources, especially acomputer code based on pseudo-spectral methods that is robust, highly accurate, and very efficient. (3) Use of this code and other theoretical methods to develop insights into gravitational wave sources, and especially predict their emitted waveforms. Among the sources to be studied are (a) the slow inspiral of neutron stars and small black holes into intermedicate-mass black holes ("Extreme mass ratio inspirals" or EMRIs), (b) the late inspiral of black-hole binaries including spin-orbit and spin-spin interactions and possible spin flips, (c) the transition from inspiral to plunge in black-hole binaries, (d) the merger of black-hole binaries, and (d) rotating neutron stars. (4) Use of the insights about sources developed in this work to construct better template families for searching for the waves, and improved techniques for extracting information carried by the waves. (5) Participation in the LIGO Scientific Collaboration's gravitational wave searches, using these templates and techniques as well as others.This research is designed to help make LIGO a success by (i) increasing its prospects of detecting gravitational waves from a wide variety of sources, and (ii) improving its ability to extract fromobserved waves the rich information that the waves should carry. It will also contribute to the advance of technology and techniques for high-precision measurement, contribute to our understanding of astrophysical systems, and contribute to the development of numerical methods and computer codes capable of carrying out robust and accurate simulations of highly dynamical spacetimes. This research will be carried out in large measure by about ten graduate students and six postdoctoral students. This program's diversity of types of research and research tools will provide a rich training ground for these students.

为支持激光干涉仪引力波观测站LIGO，将开展理论和计算研究：(1)接近实验的研究，例如减少热噪声、光散射噪声和光机械不稳定性的分析和方法。(2)发展数值相对论模拟引力源的工具，特别是基于伪谱方法的计算机程序，它是健壮的、高精度的、非常有效的。(3)使用该程序和其他理论方法对引力波源进行深入研究，特别是对其发射波形进行预测。要研究的来源包括：(A)中子星和小黑洞进入中间质量黑洞的缓慢激发源(“极端质量比激发源”)，(B)包括自旋-轨道和自旋-自旋相互作用和可能的自旋翻转在内的黑洞双星的晚期激发源，(C)黑洞双星从自旋到俯冲的转变，(D)黑洞双星的合并，以及(D)旋转的中子星。(4)利用这项工作中开发的关于源的见解来构建更好的模板族来搜索波，并改进提取波携带的信息的技术。(5)参与LIGO科学合作组织的引力波搜索，使用这些模板和技术以及其他。这项研究旨在通过以下方式帮助LIGO取得成功：(I)增加其从各种来源探测引力波的前景，以及(Ii)提高其从服务波中提取波应该携带的丰富信息的能力。它还将有助于高精度测量技术和技术的进步，有助于我们对天体物理系统的理解，并有助于开发能够对高动态时空进行稳健和准确模拟的数值方法和计算机代码。这项研究将在很大程度上由大约10名研究生和6名博士后进行。该项目的研究类型和研究工具的多样性将为这些学生提供丰富的培训场地。