PlanetPhysics/Gradient

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The gradient is the [[../Vectors/|vector]] sum of the resultant rate of increase of a [[../Vectors/|scalar]] funcion V and is denoted V. It represents a directed rate of change of V. A directed derivative or vector derivative of V, so to speak. In cartesian coordinates

V=Vx𝐒^+Vy𝐣^+Vz𝐀^

It is common to regard as the gradient operator which obtains a vector V from a scalar [[../Bijective/|function]] V of [[../Position/|position]] in space.

V=(x𝐒^+y𝐣^+z𝐒𝐀^)V

Thus it is easy to [[../Work/|work]] with just the gradient operator

=x𝐒^+y𝐣^+z𝐀^

This symbolic [[../QuantumSpinNetworkFunctor2/|operator]] was introduced by Sir W. R. Hamilton. It has been found by experience that the monosyllable del is so short and easy to pronounce that even in complicated [[../Formula/|formulas]] in which occurs a number of times no inconvenience to the speaker or hearer arises from the repetition. V is read simply as "del V."

Coordinate System Independence

Although this operator has been defined as

V=x𝐒^+y𝐣^+z𝐀^

so that it appears to depend upon the choice of the axes, it is in reality independent of them. This would be surmised from the interpretation of as the [[../AbsoluteMagnitude/|magnitude]] and direction of the most rapid increase of V. To demonstrate the independence take another set of axes, 𝐒^, 𝐣^, 𝐀^ and a new set of variables x, y, z referred to them. Then referred to this [[../SimilarityAndAnalogousSystemsDynamicAdjointnessAndTopologicalEquivalence/|system]] is

=x𝐒^+y𝐣^+z𝐀^

(Please Insert PROOF here...)

Leaving behind the proof of coordinate system independence, here is the gradient opertor in the most common coordinate systems.

Cartesian Coordinates

V=Vx𝐒^+Vy𝐣^+Vz𝐀^

Cylindrical Coordinates

V=Vr𝐫^+1rVθθ^+Vz𝐳^

Spherical Coordinates

V=Vr𝐫^+1rVϕϕ^+1rsinϕVθθ^

References

[1] Wilson, E. "Vector Analysis." Yale University Press, New Haven, 1913.

This entry is a derivative of the Public [[../Bijective/|domain]] work [1].

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