Black holes require the general relativistic concept of a curved spacetime: their most striking properties rely on a distortion of the geometry of the space surrounding them.
Black holes require the general relativistic concept of a curved spacetime: their most striking properties rely on a distortion of the geometry of the space surrounding them.
黑洞需要弯曲时空广义相对论概念:他们最显著的特性依赖它们周围空间的几何学变形。