Understanding Gauss's Law: Where Does the Argument Break Down?

In summary: Interesting question. Upon reflection, my guess is that the integral form of Gauss's Law rests on an unstated assumption that the average charge density outside of the closed surface is zero. In practice, that will usually be close enough to correct to ignore any inaccuracy. A re-stated Gauss's Law that coped with this thought experiment might replace Q, the charge inside the surface, by ##(Q-V\rho_0)## where ##V## is the volume inside the surface and ##\rho_0## is the average charge density across all space. Similarly, for the differential case, one could replace ##\rho## by ##\rho-\rho_0##.
  • #106
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.

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?
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.
 
  • Like
Likes NFuller
Physics news on Phys.org
  • #107
Orodruin said:
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.

I've not claimed that non-zero charge density solutions do not exist, I'm just trying to elaborate if physically meaningful solutions exist.

Orodruin said:
It is the type of prescription that you make that will give you the behaviour at infinity and therefore the boundary condition.

Ok, and which prescription would be physical if they give you different answers? Surely the physics should only depend on the physics, not on the mathematics.

Orodruin said:
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
That's trivial and I thought there would be more to the question. You can directly write down a bunch of solutions (also when I was misstaken and thought that Gauß' law wouldn't be applicable I did not state that there wouldn't be solutions to the differential equation), but since we are dealing with physics, I'm wondering which of these solutions can really be regarded as physical.

Orodruin said:
the original question: "If you have uniform non-zero charge distribution, what is the field?"

If this question does not incorporate physical meaning, than you're right, the question has already been answered. But then I want to extend the question ;)
 
  • #108
Metmann said:
Ok, and which prescription would be physical if they give you different answers? Surely the physics should only depend on the physics, not on the mathematics.

That depends on what you measure. I think you are seeing the boundary conditions as something to be imposed apart from the physical situation. They are not. Without them, you have not fully specified the physical situation. You can have different boundary conditions, leading to different fields, but they correspond to different physical situations, regardless of whether the charge density happens to be the same or not.

Metmann said:
I'm wondering which of these solutions can really be regarded as physical.
Sure they can. But the limiting behaviour is part of the physics and you need to take it into account. The limiting behaviour is physical precisely because it affects the fields.
 
  • #109
Orodruin said:
Sure they can. But the limiting behaviour is part of the physics and you need to take it into account. The limiting behaviour is physical precisely because it affects the fields.

Yes sure, if you assume that there are different things in the Universe than background charge and test charges. But you have to assume this additionally. All the time I have understood the question in the way I wrote before: infinite Universe filled with background, that's it. And then I wondered if there exists a non-trivial physical solution. The answer is of course: no.

Orodruin said:
I think you are seeing the boundary conditions as something to be imposed apart from the physical situation. They are not. Without them, you have not fully specified the physical situation. You can have different boundary conditions, leading to different fields, but they correspond to different physical situations, regardless of whether the charge density happens to be the same or not.

It depends: If we consider the Universe to be infinite and do not know anything about its "boundary" and if we assume that apart from test charges there is only background charge, then any boundary condition would be something additional! You can still solve the problem by the way I did, using symmetries. That's exactly what is done in Cosmology. Other boundary conditions assume implicitly that there is more physics apart from the specific situation considered.
But of course if you know e.g. that you can "earthen" the potential at some plane (due to aspects not incorporated in the "theory", namely Gauß's law + charge distribution (symmetry) + infinite universe, without any additional information), but I would call this "extrinsic" boundary conditions. An "intrinsic" "boundary" condition would be given be the symmetry.

I have to admit, that maybe I failed to make my point clear earlier, my language was probably not clear enough.

Finally we can conclude: The topic is now exhausted, everything has been said. Sorry for dragging it out.
 
  • #110
Metmann said:
All the time I have understood the question in the way I wrote before: infinite Universe filled with background, that's it.
But this is the point. It is not it. Without a specification of the boundary behaviour, you have not specified the physical situation.

Metmann said:
If we consider the Universe to be infinite and do not know anything about its "boundary" and if we assume that apart from test charges there is only background charge, then any boundary condition would be something additional!
If you do not know anything about the boundary, then you do not know the full physical situation and clearly in this case you cannot compute the field.

Metmann said:
You can still solve the problem by the way I did, using symmetries.
Not if none of the boundary conditions that are compatible with the differential equation breaks those symmetries. Then there is no physical situation with your assumed symmetric charge distribution that has those symmetries.

Metmann said:
An "intrinsic" "boundary" condition would be given be the symmetry.
But this is exactly the point. Given the charge distribution, there is no such boundary condition.

Metmann said:
Other boundary conditions assume implicitly that there is more physics apart from the specific situation considered.
Yet, those boundary conditions have to be compatible with the rest of the theory.

Metmann said:
Finally we can conclude: The topic is now exhausted, everything has been said. Sorry for dragging it out.
I really think that we actually agree on most points, the main ones being:
  • There are a multitude of solutions to Gauss's law with uniform non-zero charge density.
  • Those solutions are separated based on their behaviour at infinity
  • None of those solutions display the maximal symmetry of the charge distribution itself except in the case ##\rho = 0##, which is trivial.
 
  • #111
Orodruin said:
This is why the boundary behaviour breaks translational invariance.
Well, I remember integrating painstakingly to find E field of a planar disc and letting the disc tend to infinity... to actually get E field value that agrees with gauss' law... (E field of infinite uniformly charged sheet)
I have done the same to a uniformly charged wire segment and letting length tend to infinity also to get an answer that agrees with gauss' law... (E field of infinite linear charge distribution)
No "broken transnational invarience" here...
But once we step into the case of 3d spheres with radius tending to infinity and we suddenly have "transnational invarience"? How do you justify that?
 
  • #112
anorlunda said:
Think of the integral form. Gauss' Law let's you calculate the field due to a charge within the surface. But that does not forbid other fields from charges outside the surface. For uniform density everywhere, I expect that the vector sums of all those forces to be zero because of the symmetry arguments the OP makes. So I agree with the OP and with @andrewkirk

NFuller said:
In the case of a spherical uniform charge distribution, you can use symmetry to argue that the electric field is radially symmetric at the Gaussian surface. Gauss's law then states that the Electric field at the surface is only a function of the charge enclosed by the surface.

To talk about the electric field (as opposed to the electric flux) at the surface aren't you assuming the spherical uniform charge distribution contains all the charges in the problem? A charge outside the sphere contributes no net flux through the surface of the sphere. It can still make a contribution to the electric field.

Now take the radius of the sphere to infinity. Apparently something about Gauss's law fails in this limit. My question is which part of the argument is failing here?
If the (net) electric field is zero on the surface of a sphere of finite radius (existing within the supposed uniform distribution of charge throughout space) then it is no surprise that it stays zero as the radius is increased. One amusing thought is to represent what takes place using two spheres. Use a big sphere with a uniform charge density to represent "the universe". Use a much smaller sphere inside it to represent "the sphere we are worried about". Then let the radius of both spheres approach infinity with the big sphere always containing the smaller one.
 
  • #113
Likith D said:
No "broken transnational invarience" here...
This is not true. Both a wire and a plane break translational invariance and rotational invariance in many of the directions and you cannot let the field go to zero at infinity in some of the directions. (Namely, along the wire/plane)

I also cannot see why you are surprised that different charge distributions lead to different requirements on the boundary conditions that are compatible with the charge distribution.
Likith D said:
and we suddenly have "transnational invarience"?
The charge distribution has translational invariance in all directions, just as the line charge has translational invariance in the direction of the line. However, you always have to look at what boundary conditions are compatible with the differential equation and you cannot impose boundary conditions that aren't. In the case of a uniform charge distribution, a boundary condition that preserves translational and rotational invariance is incompatible with Gauss' law.
 
  • Like
Likes Likith D
  • #114
I'm not an expert and it's a dead thead but I want to state my thoughts anyway.

Isn't Gauss's Law responsible for finding the E-fields at the boundaries of the enclosed volume due to the ENCLOSED charge? So due to the almost infinite amount of charge in our volume (let's say a sphere), we can assume E-field to be non-zero, radial, and uniform strength everywhere along the volume boundary.

But once you take into account the E-field from the infinite charges outside the boundary, they will counteract the E-field along the volume boundary, which were from the charges in the enclosed volume, giving us the expected effect of net 0 E-field everywhere.
 
Last edited:
  • #115
yosimba2000 said:
Isn't Gauss's Law responsible for finding the E-fields at the boundaries of the enclosed volume due to the ENCLOSED charge?
Gauss’ law is a tool, it is not responsible for anything. All it does is to tell you about the relation between the enclosed charge and the flux integral over a closed surface. In the case of a spherically symmetric charge distribution and spherically symmetric boundary conditions, you can use symmetry to argue that the field must be radial and therefore directly use Gauss’ law to relate the field to the enclosed charge. In the case of boundary conditions that are not spherically symmetric you cannot do this. The point is that, as already discussed in this thread, boundary conditions compatible with the differential equation for a constant charge distribution and spherically symmetric relative to one point will not be spherically symmetric relative to other points. Thus, there is only one point where you can use Gauss’ law to directly relate the field (rather than its integral) to the enclosed charge.

yosimba2000 said:
But once you take into account the E-field from the infinite charges outside the boundary, they will counteract the E-field along the volume boundary, which were from the charges in the enclosed volume, giving us the expected effect of net 0 E-field everywhere.
No. The shell theorem tells you that the effect from any shell outside your sphere is zero. The external effect can also not have a divergence inside your sphere and thus not affect Gauss’ law. A constant zero field would clearly violate Gauss’ law. To have zero E everywhere is therefore certainly not expected. What you are missing is the contribution from the boundary at infinity, which can only be spherically symmetric relative to a single point (and that assumes no higher multipoles, see above).
 
  • #116
yosimba2000 said:
I'm not an expert and it's a dead thead but I want to state my thoughts anyway.

Isn't Gauss's Law responsible for finding the E-fields at the boundaries of the enclosed volume due to the ENCLOSED charge? So due to the almost infinite amount of charge in our volume (let's say a sphere), we can assume E-field to be non-zero, radial, and uniform strength everywhere along the volume boundary.
.
You're thinking of the total freely-MOVING charge in a sphere (if it's a conductor), but Gauss's law specifies that only NET free charge causes the surface integral enclosing said free charge to be non-zero. There are just as many protons as electrons in an uncharged object!
 

Similar threads

Replies
4
Views
1K
Replies
1
Views
498
Replies
1
Views
1K
Replies
26
Views
1K
Replies
5
Views
3K
Replies
5
Views
2K
Replies
5
Views
1K
Back
Top