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- W2141153227 abstract "An exact solution of Einstein equation is easier th an actual solution. The Schwarzschild metric is est ablished on the basis of Einstein's exact solution and it is also a static a nd stationary solution. The Schwarzschild solution expresses the geometry of a spherically symmetric massive body's (star) exterio r solution. It predicts small observable departures from the Newtonian gravity. It also represents theory of black holes when suffi ciently massive stars unable to support themselves against the pull of self gravity and must undergo a complete gravitational c ollapse when they have exhausted their internal nuc lear fuel. Various sides of Schwarzschild geometry, such as, Kruskal-Szekeres extension, space-time singularities and black hole f ormation, are discussed with simple but detail calculations. The black hole is a region from which no causal signals can reach to the external observers and it contains a space-time singularity hidden wit hin the event horizon. Schwarzschild established his metric by conside ring asymptotically flat solutions to Einstein's equatio n. Hence in our study we will consider all the known solutio ns of null geodesics of the space-time. This provides a c omplete illustration of the light cone from an arbitrary ap ex in the space-time (3)." @default.
- W2141153227 created "2016-06-24" @default.
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- W2141153227 date "2013-08-11" @default.
- W2141153227 modified "2023-09-27" @default.
- W2141153227 title "Schwarzschild Geometry from Exact Solution of Einstein Equation" @default.
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