30+ Schwarzschild Solution Pics. The kretschmann scalar invariant is calculated for the original schwarzschild solution and for hilbert's version of the schwarzschild solution. 2 einstein equations and schwarzschild solution.
(PDF) Cosmological milestones and gravastars : topics in ... from www.researchgate.net Karl schwarzschild, in 1916, gives us the very first description of a black hole in general relativity. 83c05, 83c57, 83c75 key words and phrases: Schwarzschild published this result just months after einstein published his theory of general relativity.
It describes spacetime in the vicinity of a non rotating massive spherically symmetric object.
Since we know that the solution will be unique, we are free to make guesses about the coecients γ ab and check them a posteriori. The kerr solution is only unique if the multipole moments of its mass and its angular momentum take on prescribed values. Karl schwarzschild, in 1916, gives us the very first description of a black hole in general relativity. The coeecient matrix, denoted gµ⌫ is as follows
