Charge distribution of point charges in spherical coordinates

In summary, the conversation discusses the charge distribution of a set of point charges in spherical coordinates and the use of the three-dimensional Dirac delta function in this system. The discussion also addresses the confusion about whether to use primed or unprimed coordinates in the prefactor of the delta function, and the potential issues with using a coordinate system where the delta function lies on the boundary. Finally, there is a brief discussion about the use of basis vectors in different coordinate systems.
  • #1
schrodingerscat11
89
1

Homework Statement


Hi! This is not really a problem. I'm just confused on how to express the charge distribution of a set of point charges in spherical coordinates. From our discussion,
[itex]ρ(\vec{r})=\sum\limits_{i=1}^N q_i δ(\vec{r}-\vec{r}')[/itex]
where [itex]\vec{r}[/itex] is the position of the point where charge density is being evaluated and [itex]\vec{r}'[/itex] is the position of the point charge.

Three-dimensional Dirac delta function in general is
[itex]δ(\vec{r})= \frac{1}{h_1 h_2 h_3} δ(u_1 - u_1 ')δ(u_2 -u_2 ') δ(u_3 - u_3 ')[/itex]

So in spherical coordinates, it is
[itex]δ(\vec{r})= \frac{1}{r^2 sin(θ)} δ(r - r')δ(θ -θ') δ(\phi - \phi')[/itex]

The continuous charge distribution of these point charges is therefore
[itex]ρ(\vec{r})=\sum\limits_{i=1}^N \frac{1}{r^2 sin(θ)} δ(r - r'_i)δ(θ -θ'_i) δ(\phi - \phi'_i)[/itex]

So here's the part where I'm confused. For the factor [itex]\frac{1}{r^2 sin(θ)}[/itex]. do I retain it as is (i.e. r and θ are coordinates of position vector [itex]\vec{r}[/itex] or do I subsitute the coordinates of my point charge (i.e. the coordinates of [itex]\vec{r}'[/itex])? Thank you very much.

Homework Equations


See above.

The Attempt at a Solution


I've seen a problem and an online solution and it seems that he substituted the coordinates of [itex]\vec{r}'[/itex] but I can't reconcile it from the definition of 3-D Dirac delta function I've read where the coordinates of [itex]\vec{r}[/itex] are substituted instead. Thank you very much.
 
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  • #2
But it doesn't make a difference, whether you put the primed or unprimed coordinates into the prefactor, because with a grain of salt, [itex]\delta(x)=0[/itex] for [itex]x \neq 0[/itex]. Thus you always have
[tex]\frac{1}{r^2 \sin \theta} \delta(r-r') \delta(\theta-\theta') \delta(\phi-\phi')=\frac{1}{r'^2 \sin \theta'} \delta(r-r') \delta(\theta-\theta') \delta(\phi-\phi').[/tex]
Note, however, that you never should hit the singularities of the coordinate system, because there the Jacobian becomes 0 in the denominator.
 
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  • #3
Thanks vanhees71. :smile: By Jacobian, you mean [itex]\frac{1}{h_1 h_2 h_3}[/itex] right?

Also, about your answer. Sorry for asking again, but will it really not make a difference? I'm asking this question because I'm supposed to get the multipole moment of four charges with spherical coordinates [itex](a, \frac{\pi}{2}, 0) [/itex], [itex](a, \frac{\pi}{2}, -\frac{\pi}{2}) [/itex], [itex](a, \frac{\pi}{2}, -\pi) [/itex] and [itex](a, \frac{\pi}{2}, \frac{3\pi}{2}) [/itex] respectively.

The equation for multipole moment is [itex] q_{l m} = \int Y^*_{l m}(\theta', \phi')r^{'l}\rho(\vec{r}')d^3x'[/itex]. Therefore, if the factor [itex]\frac{1}{r^2 sin(\theta)}[/itex] is primed, it becomes part of the integration but if it is unprimed, I can take it out of the integral like a constant. So in this case, should the factor [itex]\frac{1}{h_1 h_2 h_3}[/itex] be primed or unprimed?

Also, I am using this equation number 19 from this reference: http://web.mst.edu/~hale/courses/411/411_notes/Chapter1.Appendix.Dirac.Delta.pdf which as you see, has unprimed factors for the three-dimensional Dirac delta function in spherical coordinates. Thanks again.
 
  • #4
Thanks vanhees71. :smile: By Jacobian, you mean [itex]\frac{1}{h_1 h_2 h_3}[/itex] right?

Also, about your answer. Sorry for asking again, but will it really not make a difference? I'm asking this question because I'm supposed to get the multipole moment of four charges with spherical coordinates [itex](a, \frac{\pi}{2}, 0) [/itex], [itex](a, \frac{\pi}{2}, -\frac{\pi}{2}) [/itex], [itex](a, \frac{\pi}{2}, -\pi) [/itex] and [itex](a, \frac{\pi}{2}, \frac{3\pi}{2}) [/itex] respectively.

The equation for multipole moment is [itex] q_{l m} = \int Y^*_{l m}(\theta', \phi')r^{'l}\rho(\vec{r}')d^3x'[/itex]. Therefore, if the factor [itex]\frac{1}{r^2 sin(\theta)}[/itex] is primed, it becomes part of the integration but if it is unprimed, I can take it out of the integral like a constant. So in this case, should the factor [itex]\frac{1}{h_1 h_2 h_3}[/itex] be primed or unprimed?

Also, I am using this equation number 19 from this reference: http://web.mst.edu/~hale/courses/411/411_notes/Chapter1.Appendix.Dirac.Delta.pdf which as you see, has unprimed factors for the three-dimensional Dirac delta function in spherical coordinates. Thanks again.
 
  • #5
As was said, it really does not matter. If you put the unprimed coordinates they will simply be replaced by the primed when you integrate.
 
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  • #6
Okay, I see. Thank you very much Orodruin. :)
 
  • #7
rude man said:
What is interesting is that, if r' = 0, δ(r-r') dr over 0 to ∞ = 1/2, not 1.
I also have some doubts about what happens if θ = +/-π/2 or 0, and/or φ = 0 or 2π.
This is a good example why you should never use a coordinate system that has your delta on the boundary. It is bound to lead to confusions like this one.

The only reasonable definition of the delta is in terms of a distribution. In this case, the three-dimensional delta distribution should satisfy
$$
\int_V \delta^{(3)}(\vec x) f(\vec x) dV = f(0).
$$
With your assertion that the integral of the one-dimensional delta at the boundary is 1/2 and not 1, you would get this result wrong. You have to look at what distribution you are actually considering. You should generally also treat the delta as a distribution rather than a function. The bottom line is: If you want to treat it as a function with the integral property, don't use a coordinate system such that your delta is on its boundary.
 
  • #8
rude man said:
What self-respecting coordinate system can't even express vector dot or cross-products?
What makes you think you can't do this in cylinder or spherical coordinates? It is just a matter of knowing what the metric tensor is. There is absolutely no need to go to Cartesian coordinates.

rude man said:
I hope to have settled the OP's question in the simplest of ways.
I believe the OP's question was settled satisfactorily three years ago.

rude man said:
And the unit vectors have non-zero time derivatives? Ugh.
This is simply not true. The basis vectors (which is what you really mean, a unit vector can have a non-zero time derivative regardless of the coordinate system) depend on the position, there is no "time" intrinsic to Euclidean space. If the position depends on time, yes, the basis will change with the position. However, the concept of having a basis that is independent of the position (such as a Cartesian basis) is something that is very particular to Euclidean space. As soon as you try to generalise this to more general spaces you will run into problems as the tangent spaces of different points are different. I would say it is even detrimental to try to cling to the concept of having "the same basis" at different points.
 
  • #9
rude man said:
OK, given spherical vectors a = a1 r + a2 θ + a3 φ and b = b1 r + b2 θ + b3 φ, please give us a x b.
It is an orthonormal right-handed basis. It holds that
$$
\vec e_r \times \vec e_\theta = \vec e_\varphi
$$
and all cyclic permutations. So your case would be
$$
\vec a \times \vec b = (a_2 b_3 - a_3 b_2)\vec e_r + (a_3 b_1 - a_1 b_3)\vec e_\theta + (a_1 b_2 - a_2 b_1)\vec e_\varphi.
$$

rude man said:
And if tensors are required, that's another minus IMO. Haven't seen one of those in 50 years ...
If you have seen it or not is not really relevant. Tensors are central in many applications in physics. Anyway, it doesn't, so ...

rude man said:
So my Housner & Hudson (Caltech) textbook is wrong when they state that the unit vectors in sph. coord. have finite time derivatives in a rotating coordinate system? Wheras in cartesian they don't? Oh, OK ...
You never said anything about a rotating coordinate system, I think you are mixing things up. A rotating coordinate system will have time varying basis vectors - whether Cartesian or not.
 
  • #10
rude man said:
Quotes from my H&H text:
1. "In terms of the unit vectors i, j, k, which are constant ..."
2. "The unit vectors er and are not constant, but change direction with time" (referring to cylindrical coordinates to be precise).

Score: Cartesian 1 , Cylindrical (and spherical) 0?
This seems seriously taken out of context. If presented like this, it is simply wrong. A curvilinear coordinate system in itself has absolutely nothing to do with time. There is the possibility I alluded to in #10: For an object moving in a curvilinear coordinate system, the basis vectors will change with time because the position changes with time and the basis vectors change with position. This is not a drawback of curvilinear coordinates - it is a virtue. It can be used to describe things such as fictitious forces easily. Still, I would say that it is not good presentation to say that the basis vectors change with time - it would be more appropriate to say that they change with position (because they are functions of position, not time).
 
  • #11
So I found the text in the Caltech e-library.

It is exactly what I said. It is a book on dynamics and when they talk about cylinder coordinates they have implicitly assumed a motion of some object. I suggest reading a text that is actually about vector analysis and curvilinear coordinate systems.
 
  • #12
rude man said:
So in regard to "motion" what I said is true? Pretty important field, "motion"?
You are completely missing the point and your statement was a blanket one just generally stating:
rude man said:
What self-respecting coordinate system can't even express vector dot or cross-products? Or even add two vectors by their respective components without convetring to Cartesian first. And the unit vectors have non-zero time derivatives? Ugh.
All of those statements are false. A priori, there is not even a "time" connected to a curvilinear coordinate system at all. The coordinate system remains the same in time. However, if there is motion, then there is variation in space, which the basis vectors do depend on.

Furthermore, curvilinear coordinates are used for so much more than describing the motion of single point objects - what was being treated in this very thread being a prime example. I would also still call the statement in the H&H text misleading without further qualifiers and I believe that they assume that you have already had some introduction to curvilinear coordinate systems. You need to realize that you are not reading a book on the mathematics behind vector analysis. You are reading an excerpt from a book on dynamics, which is using vector analysis as a tool and within that context (and only within that context) can you trust what they say. Although the proper way of presenting it would be to state "the basis vectors change in space and so the basis at the point of the object changes with time due to the motion of the object".
 

Related to Charge distribution of point charges in spherical coordinates

1. What is the charge distribution of a point charge in spherical coordinates?

The charge distribution of a point charge in spherical coordinates refers to the way in which the electric charge is distributed or spread out around the point charge in three-dimensional space.

2. How is the charge distribution of a point charge in spherical coordinates different from that in Cartesian coordinates?

In spherical coordinates, the charge distribution is described in terms of spherical coordinates (radius, polar angle, and azimuthal angle), whereas in Cartesian coordinates, it is described in terms of the x, y, and z coordinates.

3. What is the significance of the charge distribution in spherical coordinates?

The charge distribution in spherical coordinates is important because it helps us understand and analyze how electric fields are created and behave around point charges in three-dimensional space.

4. Can the charge distribution of a point charge in spherical coordinates be visualized?

Yes, the charge distribution can be visualized using diagrams or computer simulations. These visualizations can help us better understand the behavior of electric fields around point charges in spherical coordinates.

5. How does the charge distribution affect the strength of the electric field around a point charge in spherical coordinates?

The charge distribution directly affects the strength of the electric field around a point charge in spherical coordinates. The more the charge is spread out, the weaker the electric field will be, and vice versa.

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