释义 |
Kerr black hole 基本例句 克尔黑洞 The event horizon of the non-stationaryKerr black holeis rotationallysymrnet-ric, but not spherecally symmetric.动态Kerr黑洞的事件视界是旋转对称的;不是球对称的. The location of event horizon and surface gravity near event horizon ofKerr black holeare given directly by Dirac equation htrough generalized Tortoise translation.从 Dirac方程出发 ,经广义 Tortoise坐标变换后 ,在视界曲面附近求解 ,直接导出Kerr黑洞的视界位置及视界表面重力 ,证明了 Kerr黑洞的视界是球对称的 Such spinning black holes are known as Kerr Black Holes.这种旋转的黑洞被称为克尔黑洞。 |