Derivation of the divergence in the spherical coordinate

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SUMMARY

The discussion centers on the derivation of the divergence in spherical coordinates, specifically addressing the presence of the term r2 in the partial derivative operator. The volume element in spherical coordinates is defined as r2sin(θ)ΔrΔθΔφ, and the necessity of including r2 arises from the transformation theorem for integrals, which requires adjusting volume elements by the determinant of the transformation matrix. Neglecting this term would incorrectly imply a unit radius, undermining the calculation of infinitesimal volume elements.

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elgen
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Hi,

I am reviewing some vector calculus and have a problem on the derivation of the divergence in the spherical coordinate.

Assume there is a small volume located at r_0, \theta_0, \phi_0 with a volume of r_0^2\sin\theta_0 \Delta r \Delta \theta \Delta \phi.

My question is that why there is an r^2 sitting behind the partial derivative operator? The problem is attached.

My feeling is that as I take the limit of the volume going to 0, I can cannot cancel r_0^2. However, I cannot give a good justification to that.

Would anyone knowledgeable with vector calculus give an explanation? Thank you.


elgen
 

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The procedure is described here: https://en.wikipedia.org/wiki/List_of_common_coordinate_transformations#From_spherical_coordinates

If we change coordinates in an integral we have to adjust the volume elements by the determinant of the transformation matrix, and this determinant is ##r^2 \sin \vartheta##. It is the transformation theorem for integrals. In words: you must not neglect the radius, as it is part of the formulas for volume. Without it you would set ##r=1## which makes no sense if we want to consider an infinitesimal volume element,
 

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