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What is Einsteins equation?

What is Einsteins equation?

Einstein’s theory of special relativity (1905) shows that matter (as mass) and energy can be converted into each other according to the famous equation E = mc2, where E is energy, m is mass, and c is the speed of light.

Which relationship does Einstein’s equation E mc2 describe?

The second offered experimental proof of the existence of atoms. And the third introduced the theory of special relativity. Then, in this fourth paper, Einstein explained the relationship between energy and mass, described by E=mc2. In other words, energy equals mass times the speed of light squared.

What are field equations in physics?

In theoretical physics and applied mathematics, a field equation is a partial differential equation which determines the dynamics of a physical field, specifically the time evolution and spatial distribution of the field.

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What is the unit of the Einstein constant 8πG/c4?

In standard units, each term on the left has units of 1/length 2. With this choice of Einstein constant as 8πG/c 4, then the stress-energy tensor on the right side of the equation must be written with each component in units of energy-density (i.e., energy per volume = pressure).

What are Einstein’s field equations in physics?

Einstein field equations. The Einstein field equations ( EFE; also known as Einstein’s equations) comprise the set of 10 equations in Albert Einstein ‘s general theory of relativity that describe the fundamental interaction of gravitation as a result of spacetime being curved by mass and energy.

What is Einstein’s equation of general relativity?

The basic equation of general relativity is called Einstein’s equation. In units where c = 8πG = 1, it says Gαβ = Tαβ. The beautiful geometrical meaning of this equation is a bit hard to find in most treatments of relativity. It’s all about geometry. There is an easy way to express the whole content of Einstein’s equation in plain English.

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How do the EFE relate the geometry of spacetime to its distribution?

Analogously to the way that electromagnetic fields are related to the distribution of charges and currents via Maxwell’s equations, the EFE relate the spacetime geometry to the distribution of mass–energy, momentum and stress, that is, they determine the metric tensor of spacetime for a given arrangement of stress–energy–momentum in the spacetime.

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