Schwarzschild Solution

The Schwarzschild solution is a key result in Einstein's theory of General Relativity. It describes the gravitational field outside a spherical, non-rotating mass, like a planet or a black hole. This solution shows how gravity affects the shape of space and the passage of time. For example, it predicts that time runs slower near a massive object compared to far away. The solution helps us understand phenomena such as the orbits of planets and the behavior of light near black holes, providing a mathematical framework to explain how mass influences the fabric of spacetime.