Relativistic Gravitation and Astrophysics

相对论引力和天体物理学

• 批准号: 0353180
• 负责人: Clifford Will
• 金额: $ 39万
• 依托单位: Washington University
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2004
• 资助国家: 美国
• 起止时间: 2004-04-01 至 2007-03-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0353180&HistoricalAwards=false
• 关键词: Relativistic; Gravitation; Astrophysics

The likely detection of gravitational waves from astrophysical sources will open a new window for astronomy and provide new tests of Einstein's theory of general relativity. Interpreting the observations and advancing this new field will require accurate theoretical gravitational waveforms calculated from the theory. This project will endeavor to provide the needed waveforms, by solving Einstein's equations systematically in an approximation known as the post-Newtonian method. Development of a novel diagnostic tool, based on higher-order post-Newtonian methods, to elucidate the physical content of numerical simulations of black-hole and neutron-star binary inspiral will be continued. Ways to use gravitational-wave data to test alternative theories of gravity will also be studied. This includes testing the scalar-tensor alternative theories and theories in which the graviton has a mass, by observing gravitational waves from inspiralling compact binaries. Such tests could provide verification of Einstein's theory in entirely new regimes.Education and training of graduate and undergraduate students and of a post-doctoral researcher will be integrated into the research program. The PI will continue to give public lectures on topics related to this research, bringing understanding of the validity and implications of Einstein's ideas to the broader community. He will prepare an update of his comprehensive review article on experimental gravitation for the web-based journal Living Reviews in Relativity, update his popular book ``Was Einstein Right?'' and enhance his current website with web pages providing information on testing fundamental physics with gravitational waves. The work on equations of motion and gravitational wave forms will impact the field of astronomy, as gravitation-wave observations, which rely upon these calculations, become a reality. The research on post-Newtonian diagnostics will foster closer ties between the post-Newtonian experts and numerical relativity experts, leading to more realistic simulations of the important final phase of binary inspiral.

从天体物理学来源可能探测到引力波将为天文学打开一扇新的窗口，并为爱因斯坦的广义相对论提供新的检验。解释观测结果和推进这一新领域将需要从理论计算出的精确的理论引力波形。 该项目将奋进提供所需的波形，通过系统地解决爱因斯坦方程的近似称为后牛顿方法。 将继续开发一种新的诊断工具，以高阶后牛顿方法为基础，阐明黑洞和中子星双星内旋数值模拟的物理内容。 还将研究如何利用引力波数据来检验其他引力理论。 这包括测试标量张量替代理论和引力子具有质量的理论，通过观察来自螺旋形紧凑双星的引力波。这些测试可以在全新的领域验证爱因斯坦的理论。研究生和本科生以及博士后研究人员的教育和培训将纳入研究计划。PI将继续就与这项研究相关的主题进行公开讲座，将对爱因斯坦思想的有效性和影响的理解带到更广泛的社区。 他将为网络杂志《相对论的生活评论》准备一篇关于实验引力的综合评论文章的更新，更新他的畅销书《爱因斯坦是对的吗？并在他的网站上增加了一些网页，这些网页提供了用引力波测试基础物理学的信息。 运动方程和引力波形式的工作将影响天文学领域，因为依赖于这些计算的引力波观测将成为现实。 对后牛顿诊断的研究将促进后牛顿专家和数值相对论专家之间更密切的联系，从而对双星螺旋的重要最后阶段进行更逼真的模拟。