Total moment density of electromagnetic fields

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SUMMARY

The forum discussion centers on calculating the total electromagnetic momentum of an infinite solenoid with a stationary current I and a uniform line charge with lineal density λ. The Poynting vector is defined as $$\mathbf{S}=\frac{1}{\mu_0}\mathbf{E}\times\mathbf{B}$$, leading to momentum density $$\mathbf{g}=\mu_0\epsilon_0\mathbf{S}$$. The user initially miscalculated the total momentum per unit longitude, finding $$\mathbf{G}=-\frac{\lambda n I}{2\pi\epsilon_0 c^2}$$, but later corrected this to $$\mathbf{G}=0$$ after recognizing the need to treat the unit vector $$\mathbf{\hat{\phi}}$$ as variable during integration. The total angular momentum was correctly calculated as $$\mathbf{L}=-\frac{\mu_0 nI\lambda a^2}{2}\mathbf{\hat{z}}$$.

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  • Proficiency in vector calculus, particularly cross products and integration in polar coordinates.
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987oscar
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Homework Statement


These is a problem from my textbook. You have an infinite solenoid with n turns per unit longitude, radius "a" and a stationary current I. In the axis there exits a uniform line charge with lineal density λ. Compute total electromagnetic momentum (lineal and angular).

Homework Equations


Poynting vector: $$\mathbf{S}=\frac{1}{\mu_0}\mathbf{E}\times\mathbf{B}$$.
Momentum density: $$\mathbf{g}=\mu_0\epsilon_0\mathbf{S}$$

The Attempt at a Solution


Well, I computed electric and magnetic fields as usual.
Electric field :
$$\mathbf{E}=\frac{\lambda}{2\pi\epsilon_0 r}\mathbf{\hat{r}}$$
Magnetic field (only exits inside solenoid):
$$\mathbf{B}=\mu_0 nI\mathbf{\hat{z}}$$
From here I find Poynting vector:
$$\mathbf{S}=\frac{-\lambda n I}{2\pi\epsilon_0 r}\mathbf{\hat{\phi}}$$
and momentum density:
$$\mathbf{g}=-\frac{\lambda n I}{2\pi\epsilon_0 c^2}\frac{1}{r}\mathbf{\hat{\phi}}$$
From here I have angular momentum ##\mathbf{l}=\mathbf{r}\times\mathbf{g}##:
$$\mathbf{l}=-\frac{\lambda nI}{2\pi\epsilon_0 c^2}\mathbf{\hat{z}}.$$
Integrating inside the solenoid for length 1 i find total angular momentum per unit longitude:
$$\mathbf{L}=\frac{-\lambda n Ia^2}{2\epsilon_0 c^2}\mathbf{\hat{z}}$$
When I try to compute total momentum per unit longitude I find:
$$\mathbf{G}=-\frac{\lambda n I}{2\pi\epsilon_0 c^2}\int_0^1dz\int_0^{2\pi}d\phi\int_0^a\frac{1}{r}rdr\mathbf{\hat{\phi}}=\frac{-\lambda nIa}{\epsilon_0 c^2}\mathbf{\hat{\phi}}$$.
Now the solution provided is ##\mathbf{G}=0## because momentum ##\mathbf{g}## forms closed lines ¿? Where is the mistake in my calculation?. I have been thinking about it but I can't find. Any idea? (##\mathbf{L}## calculation seems to be correct)

Thank you in advance!
 
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987oscar said:
$$\mathbf{S}=\frac{-\lambda n I}{2\pi\epsilon_0 r}\mathbf{\hat{\phi}}$$
and momentum density:
$$\mathbf{g}=-\frac{\lambda n I}{2\pi\epsilon_0 c^2}\frac{1}{r}\mathbf{\hat{\phi}}$$
Looks like you forgot the factor ##\mu_0 \epsilon_0## in going from S to g.
From here I have angular momentum ##\mathbf{l}=\mathbf{r}\times\mathbf{g}##:
Here, I think you have notational confusion. Angular momentum is calculated relative to the origin. You can let ##\mathbf{R}## be the position vector of a point relative to the origin. So, angular momentum density would be ##\mathbf{l}=\mathbf{R}\times\mathbf{g}##. Be sure to distinguish between ##\mathbf{R}## and ##\mathbf{r}##. You can write ##\mathbf{R}## in terms of ##\mathbf{r}##, ##\hat{k}##, and ##z##.
When I try to compute total momentum per unit longitude I find:
$$\mathbf{G}=-\frac{\lambda n I}{2\pi\epsilon_0 c^2}\int_0^1dz\int_0^{2\pi}d\phi\int_0^a\frac{1}{r}rdr\mathbf{\hat{\phi}}=\frac{-\lambda nIa}{\epsilon_0 c^2}\mathbf{\hat{\phi}}$$.
In your integration, you treated ##\mathbf{\hat{\phi}}## as a constant unit vector. Think about why this is not correct.
 
Hello TSny!
Thank you for your comments.
I used ##\mu_0\epsilon_0=\frac{1}{c^2}## for the ##\mathbf{g}## vector.

I used cylindrical coordinates as we have an infinite solenoid. I think angular momentum is relative to Z axis and so ##\mathbf{R}=\mathbf{r}##. I followed example 8.4 in Griffiths Introduction to Electrodynamics 4º Ed. He calls "s" "horizontal" distance from a point to Z axis and he makes a product independent of s. I don't know if these is correct for this problem.

Of course! I can't treat ##\mathbf{\hat{\phi}}## as constant. I found ##\mathbf{\hat{\phi}}=-\sin\phi\mathbf{\hat{x}}+\cos\phi\mathbf{\hat{y}}## and for angular integral I now have:
$$\int_0^{2\pi}-\sin\phi\mathbf{\hat{x}}d\phi+\int_0^{2\pi}\cos\phi\mathbf{\hat{y}}d\phi=0$$
and ##\mathbf{G}=0##:smile::smile::smile:

Thank you very much for your help!
 
987oscar said:
I used ##\mu_0\epsilon_0=\frac{1}{c^2}## for the ##\mathbf{g}## vector.
OK. I overlooked the ##c^2##.:oops:

I used cylindrical coordinates as we have an infinite solenoid. I think angular momentum is relative to Z axis and so ##\mathbf{R}=\mathbf{r}##. I followed example 8.4 in Griffiths Introduction to Electrodynamics 4º Ed. He calls "s" "horizontal" distance from a point to Z axis and he makes a product independent of s. I don't know if these is correct for this problem.
Looks like maybe Griffiths is using ##s## for your ##r##. For example, you wrote the electric field in terms of ##r## which implies that you are using ##r## for the perpendicular distance from the axis. But, when calculating the angular momentum density ##\mathbf{l}##, you need to use the vector from the origin to the point where you are calculating ##\mathbf{l}##. So, you need a different symbol for this vector, say ##\mathbf{R}##. For a general point inside the solenoid, you should find that ##\mathbf{l}## has both an ##\hat{r}## component as well as a ##\hat{z}## component.
upload_2017-5-28_18-36-32.png


Of course! I can't treat ##\mathbf{\hat{\phi}}## as constant. I found ##\mathbf{\hat{\phi}}=-\sin\phi\mathbf{\hat{x}}+\cos\phi\mathbf{\hat{y}}## and for angular integral I now have:
$$\int_0^{2\pi}-\sin\phi\mathbf{\hat{x}}d\phi+\int_0^{2\pi}\cos\phi\mathbf{\hat{y}}d\phi=0$$
and ##\mathbf{G}=0##:smile::smile::smile:
Yes. Good!
 
OK. I think finally I've understood it with your drawing.

I make ##\mathbf{R}=\mathbf{r}+\mathbf{z}=r\cos\phi\mathbf{\hat{x}}+r\sin\phi\mathbf{\hat{y}}+z\mathbf{\hat{z}}##.

Making ##C=\frac{-\mu_0nI\lambda}{2\pi}##, I find ##\mathbf{g}=\frac{-C}{r}\sin\phi\mathbf{\hat{x}}+\frac{C}{r}\cos\phi\mathbf{\hat{y}}##. And now ##\mathbf{l}=\mathbf{R}\times\mathbf{g}=-\frac{Cz}{r}\cos\phi\mathbf{\hat{x}}-\frac{Cz}{r}\sin\phi\mathbf{\hat{y}}+C\mathbf{\hat{z}}##.

We compute total angular momentum per unit length
$$\mathbf{L}=\int_0^1dz\int_0^ardr\int_0^{2\pi}\left(-\frac{Cz}{r}\cos\phi\mathbf{\hat{x}}-\frac{Cz}{r}\sin\phi\mathbf{\hat{y}}+C\mathbf{\hat{z}}\right)d\phi.$$ But, ##\int_0^{2\pi}\cos\phi\, d\phi=0##, and ##\int_0^{2\pi}\sin\phi \,d\phi=0##.
Finally we get:
$$\mathbf{L}=C\pi a^2\mathbf{\hat{z}}=-\frac{\mu_0 nI\lambda a^2}{2}\mathbf{\hat{z}}.$$

Thanks a lot for your help!:smile::smile::smile:
 
Yes, that looks very good.

You can shorten the work a little by using symmetry. It should be clear that the total angular momentum ##\mathbf{L}## only has a ##z## component. So, you only need the ##z## component of the angular momentum density ##\mathbf{l}##, which is what you actually calculated in your first post. So, you got the correct total angular momentum in your first post.
 
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Thank you. You have helped me a lot!
 

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