Introducing a flat space approximation for their outer regions into their metric yields Rindler geometry. One proposed solutions to their information loss problem is the holographic principle. One theorem states that these objects are describable by just three parameters. One type is named for Kerr and their size can be thought of as the (*) Schwarzschild radius. Surrounded by an event horizon, they contain a singularity. They can be formed by the collapse of massive sta
Introducing a flat space approximation for their outer regions into their metric yields Rindler geometry. One proposed solutions to their information loss problem is the holographic principle. One theorem states that these objects are describable by just three parameters. One type is named for Kerr and their size can be thought of as the (*) Schwarzschild radius. Surrounded by an event horizon, they contain a singularity. They can be formed by the collapse of massive stars. For 10 points, name this objects from which light cannot escape.
Introducing a flat space approximation for their outer regions into their metric yields Rindler geometry.
{black holes} [or {event horizon} before "three parameters"]