The Sunergism of Analytic and Numerical Technologies in General Relativity

广义相对论中的非线性相互作用将使用一个模拟真空内爆和再爆炸的代码来研究。轴对称引力波。随着波幅的增加，波开始通过自身的质量能量(暂时)将自己保持在一起。如果振幅足够大，黑洞就会形成并辐射出它的非球面。另一种代码目前正在针对微扰理论进行测试，正在专门开发用于研究黑洞时空的代码。它将被用来研究高度扭曲的单个黑洞的辐射特性，并最终模拟两个黑洞的迎头碰撞，并计算发出的引力波。

Nonlinear interactions in general relativity will be studied using a code that simulates the implosion and re-explosion of a vacuum. axisymmetric gravitational wave. As the wave amplitude is increased, the wave begins to hold itself together (temporarily) by its own mass energy. If the amplitude is large enough a black hole will form and radiate off its asphercity. Another code, currently being tested against perturbation theory, is being developed specifically to study black hole spacetimes. It will be used to investigate the radiative properties of very highly distorted single black holes and eventually to simulate the head-on collision of two black holes and calculate the gravitational waves emitted.