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Metmann said:Sure, no doubt. But in the situation I describe, there is (in my opinion) no physical way to introduce such a condition without yielding ##\rho=0##. I mean a meaningful condition would definitely be, that the total energy should be finite (what you do with the cutoff), hence the potential should vanish at infinity. Can you solve ##\Delta \Phi = \rho = \text{const} \neq 0## with ##\lim_{|\vec{x}|\rightarrow \infty} \Phi(\vec{x}) = 0## without a cutoff? Spontaneously I cannot think of any other meaningful boundary condition within this setting.
With your assumptions, I agree that they imply ##\rho = 0##. However, that was not the original question of the thread. The original question of the thread was stating that you have a non-zero uniform charge density. Your assumptions, while reasonable at face value, clearly violate the statement of non-zero uniform charge density. That does not mean that solutions that include non-zero uniform charge density do not exist.
But where does this cutoff come frome? In the situation I described, there is no natural cutoff. Of course you can randomly introduce it, but why should that be physical if the charge density is filling the whole universe?
You have to introduce the limit of several cutoffs at increasing radius. Of course, you can take the limit in several ways, which will give you different results. It is a matter of definition of how the integral with ##r \to \infty## is considered. Since the integral is not convergent, different prescriptions will give you different results, but none will be translationally invariant. It is the type of prescription that you make that will give you the behaviour at infinity and therefore the boundary condition.
What you assume about your limiting behaviour is physical because it affects the field configuration.
This is not at all applicable to this thread. This is about electrostatics. The bottom line is that there exist solutions to the field equations that do satisfy the condition of having a uniform non-zero charge density. However, they do not display the same symmetries as the charge distribution. Since this symmetry breaking does not come from the differential equation, nor from the charge distribution, the only other place it can come from is the boundary conditions, i.e., the behaviour of the fields at infinity. In order to have a solution with uniform charge distribution, these boundary conditions must therefore break the symmetry. This was the original question: "If you have uniform non-zero charge distribution, what is the field?" The answer is that it depends on the specified behaviour at infinity and that that behaviour breaks the symmetry of the charge distribution. Of course, the question could have been "What kind of solutions exist with maximal symmetry?" In that case the answer would have been that the only such solution is ##\vec E = 0## and that this solution has zero charge density, but it would have been a different question.Of course, if you also consider special relativity, you can use as a cutoff the maximal distance a photon could have traveled since BB, but in classical physics?