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- W966011712 abstract "In this chapter we derive some important solutions of the gravitational field equations. We note that the gravitational field equations are non-linear equations that include the self-interaction, that is, the interaction of the gravitational field with itself. We begin with the non-relativistic limit of the gravitational field equations and derive the Newton law of gravity from the space-time metric of the general relativity. We then derive the simplest solution of the complete gravitational field equations for the static spherically symmetric field produced by a spherical mass M at rest, known as the Schwarzschild solution. Finally, we study the consequences of the Schwarzschild metric solution whereby we encounter the possibility of the existence of black holes." @default.
- W966011712 created "2016-06-24" @default.
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- W966011712 date "2015-01-01" @default.
- W966011712 modified "2023-10-17" @default.
- W966011712 title "Solutions of Field Equations" @default.
- W966011712 doi "https://doi.org/10.1016/b978-0-12-803397-5.00020-0" @default.
- W966011712 hasPublicationYear "2015" @default.
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