Understanding the Theory of Black Holes
Black holes are regions of space where gravity is so strong that nothing, not even light, can escape. They are formed when massive stars collapse under their own gravity at the end of their life cycles.
According to Einstein's Theory of Relativity, if an object is sufficiently compact, gravity can lead to the creation of a black hole. These astrophysical phenomena are among the most intriguing and studied in all of cosmology and physics.
The Event Horizon
The event horizon of a black hole is the boundary beyond which nothing can escape. It is the point of no return and marks the limits of our observable universe.
The Singularity
At the core of a black hole lies the singularity, a point where the curvature of space-time becomes infinite. The laws of physics as we know them cease to apply, and this remains one of the greatest enigmas for scientists today.
Time Dilation
Close to a black hole, time operates differently due to intense gravitational forces. This phenomenon, known as time dilation, was famously illustrated in the movie "Interstellar".