Harmonic Coordinates

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Harmonic coordinates satisfy the condition

Gamma^lambda=g^(munu)Gamma_(munu)^lambda=0,

(1)

or equivalently,

partial/(partialx^kappa)(sqrt(g)g^(lambdakappa))=0.

(2)

It is always possible to choose such a system. Using the d'Alembertian,

square ^2phi=(g^(lambdakappa)phi_(;lambda))_(;kappa)=g^(lambdakappa)(partial^2phi)/(partialx^lambdapartialx^kappa)-Gamma^lambda(partialphi)/(partialx^lambda).

(3)

But since Gamma^lambda=0 for harmonic coordinates, the result is a generalization of the harmonic equation

del ^2x=0

(4)

to

square ^2x^mu=0.

(5)


See also

d'Alembertian

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References

Weinberg, S. Gravitation and Cosmology: Principles and Applications of the General Theory of Relativity. New York: Wiley, 1972.

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Harmonic Coordinates

Cite this as:

Weisstein, Eric W. "Harmonic Coordinates." From MathWorld--A Wolfram Resource. https://mathworld.wolfram.com/HarmonicCoordinates.html

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