Examples of using In general relativity in English and their translations into Turkish
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In general relativity, the effects of gravitation are ascribed to spacetime curvature instead of a force.
In general relativity the metric tensor symbolizes the gravitational potential,
In General Relativity, every separate local quantity which is used to describe the geometry is itself a local dynamical field, with its own equation of motion.
increasing with distance from this axis, the solution is rather artificial, but as one of the simplest known solutions in general relativity.
When discussing the evolution of a system in general relativity, or more specifically Minkowski space, physicists often refer to a"light cone.
But in general relativity, which is theory of curved space-time, if you take a shortcut,
Although the calculations are considerably more complicated, one can show that a static field in general relativity does not suffer from aberration problems as seen by an unaccelerated observer
Einstein also said that in general relativity the"aether" is not absolute anymore, as the gravitational field and therefore the structure of spacetime depends on the presence of matter.
In general relativity, objects in free-fall follow geodesics of spacetime,
The two null cones overlap in general relativity, which makes tracking the speed-of-gravity effects difficult and requires a special mathematical technique of gravitational retarded potentials, which was worked out by Kopeikin
involving time(the Hamiltonian constraint) is more subtle because it is related to dynamics and the so-called"problem of time" in general relativity.
In general relativity, these fields are symmetric(in the matrix sense),
They only refer to the basic structure of the laws of physics:"c" and"G" are part of the structure of spacetime in general relativity, and ℏ captures the relationship between energy and frequency which is at the foundation of quantum mechanics.
This by itself is not significant, since any spacetime geometry is a solution of the field equations for some configuration of the stress-energy tensor field see exact solutions in general relativity.
Related units==One solar mass,, can be converted to related units:* 27,068,510 Lunar mass("M"L)* 332,946 Earth mass()* 1,047.56 Jupiter mass()It is also frequently useful in general relativity to express mass in units of length or time.
Schwarzschild metric===Besides the flat space metric the most important metric in general relativity is the Schwarzschild metric which can be given in one set of local coordinates by:
correspond to inertial motion within a curved geometry of spacetime in general relativity; there is no gravitational force deflecting objects from their natural, straight paths.
Historically, these ideas were first stated in the context of classical electromagnetism and later in general relativity.
The Kerr-Newman metric is a generalization of other exact solutions in general relativity: Kerr metric if the charge Q is zero.
Gravity wells are frequently confused with embedding diagrams used in general relativity theory, but the two concepts are distinctly separate