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Black Holes

Black Holes.
Black holes are one of the many universes many wonders. Something with so much pull and so much gravitational force that nothing can escape it, not even light. With light not being to escape there is no feasible way to see the interior. General Relativity describes blackholes as nothing more than empty space, for that whatever goes into it, can’t come back out and will just put a void in the universe. The concept of black holes have been discussed by many great thinkers such as the likes of Karl Schwarzschild, Stephen Hawking and Pierre-Simon Laplace. These thinkers have came to the conclusion that there are at least four different types of black holes; Supermassive Blackholes, Intermediate-mass blackholes, Stellar-mass black holes, and Primordial Black holes. All these separate types have a distinction between size and mass.
Black holes have three properties. Mass, charge and angular momentum. If there are two black holes that share these properties than they are considered indistinguishable. This counteracts the fact that stars have many parameters. But when a star collapses it loses unfortunately a great deal of information and leaving only mass, charge, and the angular momentum. The black hole information paradox is a question astronomers have because usually in almost all cases information is preserved, so losing information about the star and transforming into in some sense a gravitational junk yard is puzzling.
The simplest black hole we have discovered is named the Schwarzschild Black hole. Karl Schwarzschild discovered that there are in fact black holes that consist of mass but neither charge nor angular momentum. This is the first solution to any one of Einstein’s equations and theory’s on black holes. Also later on in the twentieth century the Reissner-Nordstrom solution and Kerr solutions were discovered. The Reissner-Nordstrom solution proved that black holes have electic charges while Kerr solution describes a rotating...