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  1. 5 days ago · The Einstein field equations are the 16 coupled hyperbolic-elliptic nonlinear partial differential equations that describe the gravitational effects produced by a given mass in general relativity. As result of the symmetry of G_(munu) and T_(munu), the actual number of equations reduces to 10, although there are an additional four differential identities (the Bianchi identities) satisfied by G ...

  2. Relativity, wide-ranging physical theories formed by the German-born physicist Albert Einstein. Special relativity is limited to objects that are moving with respect to inertial frames of reference. General relativity is concerned with gravity, one of the fundamental forces in the universe.

  3. Malcolm A.H. MacCallum (2013), Scholarpedia, 8 (12):8584. Exact Solutions of Einstein's Equations. Einstein's General Relativity is the leading theory of space-time and gravity: it is highly nonlinear. Exact solutions of Einstein's equations thus model gravitating systems and enable exploration of the mathematics and physics of the theory.

  4. General Relativity is the classical theory that describes the evolution of systems under the e ect of gravity. Its history goes back to 1915 when Einstein postulated that the laws of gravity can be expressed as a system of equations, the so-called Einstein equations. In order to formulate his theory, Einstein had to reinterpret fundamental ...

  5. The motion of a body in this gravitational field is explained almost perfectly by the geodesic equations. Einstein used three principles to develop his general theory of relativity. 1. Mach's Principle: Ernest Mach gave some ideas without any proof and arguments that are known as Mach's principle. There are several forms of Mach's principle.

  6. Credit: NSF/LIGO/Sonoma State University/A. Simonnet. Our modern understanding of gravity comes from Albert Einstein’s theory of general relativity, which stands as one of the best-tested theories in science. General relativity predicted many phenomena years before they were observed, including black holes, gravitational waves, gravitational ...

  7. e. In physics, Maxwell's equations in curved spacetime govern the dynamics of the electromagnetic field in curved spacetime (where the metric may not be the Minkowski metric) or where one uses an arbitrary (not necessarily Cartesian) coordinate system. These equations can be viewed as a generalization of the vacuum Maxwell's equations which are ...

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