Angular momentum of the EM field of rotating sphere

Shinobii
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The angular momentum of the electromagnetic field is defined as,

$$
\vec{L_{em}} = \int \vec{l_{em}} d^3r.
$$

To solve this for a rotating sphere I must consider the cases where r < R and r > R.

When I did this problem I thought that there would be two solutions, one for both cases; however, it turns out that there is one solution,

$$
\vec{L_{em}} = \int \vec{l_{em}}_{(r<R)} \, d^3r + \int \vec{l_{em}}_{(r>R)} \, d^3r.
$$

Can anyone tell me why that is? Conceptually I do not understand what is going here.
 
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Also for the integration, would I integrate the r < R case from \int_0^R = \int_0^r + \int_r^R and the case of r > R, \int_R^{\infty}?

Or would I simply just integrate \int_0^R for both cases, without splitting the integral.
 
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I suppose when calculating the field angular momentum, we do not need to split the r < R integral \int_0^R. I also understand now that we are integrating over all space or over the entire field.
 
To solve this, I first used the units to work out that a= m* a/m, i.e. t=z/λ. This would allow you to determine the time duration within an interval section by section and then add this to the previous ones to obtain the age of the respective layer. However, this would require a constant thickness per year for each interval. However, since this is most likely not the case, my next consideration was that the age must be the integral of a 1/λ(z) function, which I cannot model.
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