Chandrasekhar Centennial Symposium; Chicago, IL; October 16-17, 2010

该奖项支持前往科学研讨会将于2010年10月16日至17日在芝加哥大学举行的荣誉100周年的苏布拉马尼扬·拉塞卡出生。诺贝尔奖赢家，卡拉塞卡最出名的是他最早的工作表明，白色矮星不能有一个质量大于“卡拉塞卡极限”，这一结果在目前的恒星演化，超新星和引力坍缩的理解中发挥了核心作用。 在完成这项工作后，Eschrasekhar继续，先后分析恒星结构，恒星动力学，辐射传输，等离子体物理学，流体力学和磁流体力学，以及平衡解决方案的旋转机构在牛顿引力。 然后，他把生命中最后35年的大部分时间都投入到广义相对论的研究中，在那里他对后牛顿分析、黑洞理论和许多其他领域做出了重大贡献。研讨会将汇集国际领先的物理学家和天体物理学家，把他的工作的角度和阐明他的工作在当前的研究的许多后果。 研讨会应该为参加的学生和博士后提供一个关于广义相对论和天体物理学研究的一些关键领域的很好的介绍。这可能是一个足够“高调”的事件，以吸引当地、国家和国际媒体的注意，从而使更广泛的公众对卡拉塞卡尔的工作产生更大的兴趣。

This award supports travel to a scientific symposium to be held October 16 - 17, 2010 at the University of Chicago in honor of the 100th anniversary of the birth of Subrahmanyan Chandrasekhar. A Nobel Prize winner, Chandrasekhar is best known for his earliest work showing that white dwarf stars cannot have a mass greater than the "Chandrasekhar limit," a result that plays a central role in current understanding of stellar evolution, supernovae, and gravitational collapse. After completing this work, Chandrasekhar went on, successively, to the analysis of stellar structure, stellar dynamics, radiative transfer, plasma physics, hydrodynamics and magnetohydrodynamics, and equilibrium solutions for rotating bodies in Newtonian gravity. He then devoted most of the last thirty-five years of his life to research in general relativity, where he made major contributions to post-Newtonian analysis, the theory of black holes, and many other areas. The symposium will bring together internationally leading physicists and astrophysicists to put his work in perspective and elucidate many of the ramifications of his work in current research. The symposium should provide an excellent introduction to some key areas of research in general relativity and astrophysics for students and postdocs who participate. It may be a sufficiently "high profile" event to attract attention in the local, national, and international media, leading to greater interest by the broader public in the work of Chandrasekhar.