Exemplos de uso de Field equations em Inglês e suas traduções para o Português
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Begin entering your warp field equations.
The Einstein field equations describe how this curvature is produced.
For example, an important approach is to linearise the field equations.
The Einstein field equations(EFE) are the core of general relativity theory.
Systematic references are made, of course, to Einstein's field equations, but there is nothing more.
The Einstein field equations are nonlinear and very difficult to solve.
It is merely the image of a function totally described by the field equations.
The publication featuring the field equations is Einstein 1915, cf. Pais 1982, ch.
The field equations may be derived by using the Einstein-Hilbert action.
Therefore, solutions of the Einstein field equations describe the evolution of the Universe.
Georges Lemaître discusses the creation event of an expanding universe governed by the Einstein field equations.
The form of the Einstein field equations with cosmological constant Λ becomes Rμν+ Λgμν 1/2Rgμν+ Tμν.
Ricci curvature plays an important role in general relativity,where it is the key term in the Einstein field equations.
We present here the linear regime of the einstein¿s field equations in the characteristic formulation.
Solutions==Einstein's field equations are not used in deriving the general form for the metric: it follows from the geometric properties of homogeneity and isotropy.
It was the first exact solution of the Einstein field equations other than the trivial flat space solution.
The Einstein field equations do not determine the metric uniquely, even if one knows what the metric tensor equals everywhere at an initial time.
It is therefore reasonable to suppose that the field equations can be used to derive the geodesic equations. .
But as early as 1916,the astrophysicist Karl Schwarzschild found the first non-trivial exact solution to the Einstein field equations, the Schwarzschild metric.
Now we can attempt to construct various field equations, analogous to what Maxwell wrote on electromagnetism.
The Einstein-Hilbert action(also referred to as Hilbert action) in general relativity is the action that yields the Einstein field equations through the principle of least action.
The nonlinearity of the Einstein field equations often leads one to consider approximation methods in solving them.
Alexandru Proca was the first to develop and report the massive vector boson field equations and a theory of the mesonic field of nuclear forces.
Derivation of Einstein's field equations==Suppose that the full action of the theory is given by the Einstein-Hilbert term plus a term formula_8 describing any matter fields appearing in the theory.
General Theory of Relativity,despite its impressiveness and its field equations, never received the Nobel prize, after so many“empirical contrasts”.
The Einstein field equations(EFE) or Einstein's equations are a set of 10 equations in Albert Einstein's general theory of relativity which describe the fundamental interaction of gravitation as a result of spacetime being curved by matter and energy.
The relation is specified by the Einstein field equations, a system of partial differential equations. .
This model is directly associated to the field equations, with magnetic vector potential formulation, by means of a differential reluctivity tensor.
Solitons are classical solutions of non-linear field equations, that have finite energy and localised energy density.
This would eliminate 8πG from the Einstein field equations, Einstein-Hilbert action, Friedmann equations, and the Poisson equation for gravitation.