The Laplacian from Rectangular to Spherical Coordinates
Swapnil Sunil Jain
Date: June 4, 2006
We begin by recognizing the familiar conversion from rectangular to spherical coordinates1
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(1) |
and conversely from spherical to rectangular coordinates
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(2) |
Now, we know that the Laplacian in rectangular coordinates is defined in the following way2
We also know that the partial derivatives in rectangular coordinates can be expanded in the following way by using the chain rule
The next step is to manipulate the right-hand side of each of the above three equations so that it is only a function of , and . We can do this by substituting the following expressions in their respective places in the above three equations3
After the substitution, equation (4) looks like the following
Assuming that is a sufficiently differentiable function, we can replace by
and arrive at the following
Now the trick is to substitute equation (8)
equation (9) in order to eliminate any partial derivatives with respect to . The result is the following equation
In the hopes of simplifying the above equation, we operate the derivatives on the operands and get
After further simplifying the above equation, we arrive at the following form
Notice that we have derived the first term of the right-hand side of equation (3) (i.e.
) in terms of spherical coordinates. We now have to do a similar arduous derivation for the rest of the two terms (i.e.
and
). Lets do it!
After we substitute the values of (7) into equation (5) we get
We then differentiate both sides with respect to and arrive at the following
Now we substitute equation (10) into equation (11) in order to eliminate any partial derivatives with respect to . The result is the following
Now we operate the operators and get
and after some simplifications
Now its time to derive
. After our substitution of value in (7) into equation (6) we get
We then differentiate both sides of the above equation with respect to resulting in the following
Now we substitute equation (12) into equation (13) in order to eliminate any partial derivatives with respect to and we arrive at
After operating the operators we get
and then simplifying
Now that we have all three terms of the right hand side of equation (3)(i.e.
,
and
), we add them all together (because of equation (3)) to get the laplacian in terms of , and 
It may be hard to believe but the truth is that the above expression, after some miraculous simplifications of course, reduces to the following succinct expression and we finally arrive at the Laplacian in spherical coordinates!
By further manipulating the above expression, we can write the Laplacian in a more compact form as
Footnotes
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1
- Note that convention in use here:
is the azimuthal angle, whereas is the polar angle.
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2
- Readers should note that we do not have to define the Laplacian this way. A more rigorous approach would be define the Laplacian using a coordinate-free expression.
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3
- These expression can be derived simply by taking the proper derivative of the expressions in (2) and then substituting the expressions from (1) in order to eliminate any dependence on
, , and .
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