Theoretical Studies in Gravitation and Astrophysics

该奖项支持PI的广义相对论和理论天体物理学研究，一名博士后研究助理，一名夏季研究生和两名REU学生。研究领域包括引力辐射的产生、相对论流体力学、磁流体力学和恒星动力学，其中引力，特别是相对论引力的重要作用是一条共同的主线。紧凑的物体提供了主要的论坛，强引力场中的物质动力学是一个主要的主题。具体的主题包括双中子星，双黑洞和双黑洞-中子星的螺旋和合并，从双星和其他有希望的天体物理引力辐射源产生引力波，引力坍缩，旋转中子星的稳定性和不稳定恒星的演化和最终命运，伽马射线爆发源，以及星系和类星体核心中超大质量黑洞的形成和成长。这些问题大多需要大规模的计算来解决。 因此，该方法涉及到一个显着程度的大规模计算并行机，以及分析建模。许多数值计算采用了UIUC的国家超级计算应用中心（NCSA）的最先进的计算资源。它们包括初始值和演化计算，并处理包含黑洞的真空时空以及包含现实物质源和磁场的时空。 这些结果对天文观测具有重要意义，包括那些计划用于引力波干涉仪的观测，如LIGO和丽莎。计划中的研究将连接广义相对论和天体物理学领域。相当一部分资金用于本科生、研究生和博士后学生的教育、培训和支持。该补助金支持PI的本科生研究经验（REU）团队在UIUC计算天体物理学和广义相对论的活动。每个PI的本科生，研究生和博士后学生在大规模计算和科学可视化以及理论物理和天体物理学的几个不同领域接受的培训，使他们能够在广泛的科学和技术领域从事职业生涯。所开发的计算机算法和数值代码对其他从事计算物理学和天体物理学工作的小组很有用。通过PI及其团队的研究和外展活动，该补助金有助于在各级教育中推广计算机和可视化工具的使用，以及公众对引力物理学和天体物理学最新和最令人兴奋的发展的认识。

This award supports the research in general relativity and theoretical astrophysics of the PI, one postdoctoral research associate, one graduate student during the summer, and two REU students. The research areas include the generation of gravitational radiation, relativistic hydrodynamics, magnetohydrodynamics, and stellar dynamics, having as a common thread the crucial role of gravitation, especially relativistic gravitation. Compact objects provide the principal forum, and the dynamics of matter in a strong gravitational field is a major theme. Specific topics include the inspiral and coalescence of binary neutron stars, binary black holes, and binary black hole--neutron stars, the generation of gravitational waves from binaries and other promising astrophysical sources of gravitational radiation, gravitational collapse, the stability of rotating neutron stars and the evolution and final fate of unstable stars, gamma-ray burst sources, and the formation and growth of supermassive black holes in the cores of galaxies and quasars. Most of these topics require large-scale computation for solution. Hence the approach involves to a significant degree large-scale computations on parallel machines, as well as analytical modeling. Many of the numerical calculations employ the state-of-the-art computational resources of the UIUC's National Center for Supercomputing Applications (NCSA). They comprise both initial value and evolution computations and treat vacuum spacetimes containing black holes as well as spacetimes containing realistic matter sources and magnetic fields. The results have important implications for astronomical observations, including those planned for gravitational wave interferometers, such as LIGO and LISA.The planned research bridges the fields of general relativity and astrophysics. An appreciable portion of the funding is devoted to the education, training and support of undergraduate, graduate, and postdoctoral students. The grant supports the activities of the PI's Research Experiences for Undergraduates (REU) team at UIUC in computational astrophysics and general relativity theory. The training that each of the PI's undergraduate, graduate, and postdoctoral students receives in large-scale computations and scientific visualization, as well as in several different areas of theoretical physics and astrophysics, prepares them to pursue professional careers in a broad range of scientific and technical fields. The computer algorithms and numerical codes that are developed are useful to other groups working in computational physics and astrophysics. Through the research and outreach activities of the PI and his group, the grant helps promote the use of computers and visualization tools at all levels of education, as well as the public awareness of some the latest and most exciting developments in gravitation physics and astrophysics.