One can use Kruskal coordinates to describe these objects when they fit the Reissner-Nordstrom solution, and they can be formed when an object surpasses the Oppenheimer-Volkoff limit. Carter's theorem states that only the Kerr-Newman metric is correct for describing a spinning charged one. Its temperature is inversely proportional to its mass and its entropy is proportional to its surface area. Laplace was one of the first people to conceive of the idea, but it was Schwarzschild who understood them in terms of relativit
One can use Kruskal coordinates to describe these objects when they fit the Reissner-Nordstrom solution, and they can be formed when an object surpasses the Oppenheimer-Volkoff limit. Carter's theorem states that only the Kerr-Newman metric is correct for describing a spinning charged one. Its temperature is inversely proportional to its mass and its entropy is proportional to its surface area. Laplace was one of the first people to conceive of the idea, but it was Schwarzschild who understood them in terms of relativity and John Wheeler who named them. For 10 points, what are these objects formed when stars collapse, from which light cannot escape?
One can use Kruskal coordinates to describe these objects when they fit the Reissner-Nordstrom solution, and they can be formed when an object surpasses the Oppenheimer-Volkoff limit.
{black hole}