The Sunergism of Analytic and Numerical Technologies in General Relativity

将研究广义相对论中的非线性相互作用 使用一个代码，模拟内爆和再爆炸的一个 真空。轴对称引力波 当波的振幅 增加，波浪开始将自己聚集在一起， （暂时）靠自己的质量能量。 如果振幅很大 足以形成一个黑洞，并从它的球体中辐射出来。 另一个代码，目前正在测试对微扰理论， 是专门用来研究黑洞时空的 它将被用来研究辐射特性的非常 高度扭曲的单个黑洞，并最终模拟 两个黑洞的正面碰撞， 引力波发射。

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.