(*) singularities at their center, name these astronomical bodies, for which Stephen Hawking developed four laws of mechanics, that are so massive that not even light can escape their pull.
These astronomical objects emit a radiation partially named for Beckenstein, and Penrose theorized a process for extracting energy from rotating ones. These entities are smaller than their Schwarzchild radius, which therefore becomes the event horizon for non-rotating ones. Containing (*) singularities at their center, name these astronomical bodies, for which Stephen Hawking developed four laws of mechanics, that are so massive that not even light can escape their pull.
These astronomical objects emit a radiation partially named for Beckenstein, and Penrose theorized a process for extracting energy from rotating ones.
{Black Hole}s