A black hole is a localized gravitational collapse. It consists of a horizon and a Singularity.
It is impossible to escape from a black hole. Except at the quantum level:
The black hole horizon is the point of no return. Once you have passed it, you can no longer escape its gravitational grip.
Our time accelerates when we cross the horizon. Thus, an outside observer will see our image frozen (slowed down), billions of years have passed, whereas for us it is only a few seconds.
We can't move across the horizon, we don't have enough energy.
The more matter a black hole swallows, the more it starts to evaporate. Its radiation is called the Hawking Radiation.
A black hole emits particle depending on its temperature, depending on the mass. The higher the mass, the lower the temperature.
A black hole is characterized by:
With this, we can calculate something called the Surface Gravity.
Status:: #wiki/notes/germinating
Plantations:: Astrophysics - 20230221093947
References:: L'Univers à portée de main, Brief Answers to the Big Questions, Parallel Worlds, A Brief History of Time