How to use geometrical symmetries -- general advice? (Vector potential)

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SUMMARY

This discussion focuses on the use of geometrical symmetries in calculating the magnetic flux density of an infinitely long hollow cylinder using the vector potential. The vector potential, denoted as ##\vec{A}(\vec{r})##, is shown to be independent of the ##z## and ##\varphi## coordinates due to the cylindrical symmetry of the current density ##\vec{j}(\vec{r}) = j \vec{e}_{z}##. The mathematical expression for the vector potential is derived using cylindrical coordinates, confirming that the magnetic field ##\vec{B}## remains cylindrically symmetric. The discussion emphasizes the importance of symmetry in simplifying calculations and understanding field behavior.

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The following is an example from my script. I always have trouble identifying useful symmetries. Can someone explain to me why (for example) the vector potential doesn't have a ##z## dependence? I understand that there is no ##\varphi## dependency.
I don't understand why the field of ##\vec{A}## has to be parallel to the ##z## axis. What about ##d^{3} \overrightarrow{r^{\prime}}##??? Is there a way to show mathematically that the vector potential is independent of the two variables ##z\varphi##?
In general, I have problems identifying symmetries and using them correctly.

Magnetic flux density of an infinitely long hollow cylinder

The hollow cylinder is homogeneously traversed by the current ##I##. Calculate the magnetic flux ##\vec{B}(\vec{r})## as the curl of the vector potential ##\vec{A}(\vec{r})##.

$$
\begin{aligned}
\vec{A}(\vec{r}) & =\frac{\mu_{0}}{4 \pi} \int \limits_{V} \frac{\vec{j}\left(\overrightarrow{r^{\prime}}\right)}{\left|\vec{r}-\overrightarrow{r^{\prime}}\right|} d^{3} \overrightarrow{r^{\prime}} \\
\vec{j}(\vec{r}) & =j \vec{e}_{z}
\end{aligned}
$$

Use cylindrical coordinates ##\vec{r}=(\rho, \varphi, z)##. Due to the symmetry, we have:
$$
\vec{A}(\vec{r})=A(\rho, \varphi, z) \vec{e}_{z}=A(\rho) \vec{e}_{z}
$$
 
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If you have an infinitely long cylindrical object then the field can't depend on either ##z## or ##\varphi## because the charge and current densities are symmetrical under rotation around the ##z## axis and translation along it. If the sources are symmetric like that, how can the fields be otherwise? If they were (e.g.) weaker at some ##z=z_0##, why there?

So the ##\vec B## field is cylindrically symmetric. What ways can a vector field be cylindrically symmetric? What does that tell you about ##\vec A##?
 
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There is no way to generally prove that the vector potential does not depend on particular coordinates since it is always possible to perform a gauge transformation ##\vec A \to \vec A + \nabla \phi## with the same resulting field for any scalar function ##\phi##.

Any symmetry argument must be based on this particular expression for the vector potential.
 
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