fluidistic
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The problem was to give the charge distribution of a uniformly charged disk of radius R centered at the origin and perpendicular to the z-axis.
The professor explained us how to do so (though many parts were unclear to me and I couldn't copy everything that was on the blackboard because we were too much students and I couldn't see the bottom part of the blackboard).
For a punctual charge, the general form of the charge distribution is \rho (\vec x) = q \delta (x) \delta (y) \delta (z).
For a charged plane: \rho (\vec x) = q \delta (z) and for a charged line: \rho (x,y,z)=q \delta (x) \delta (y).
However for a finite (in extension) plane perpendicular to the z-axis, \rho (\vec x) = f(x,y)\delta (z). The professor told us that the Dirac's delta "reduces" the dimension (though I don't understand why/how. If you have any comment on his, this would be nice). That's why for a point-like charge we need 3 of these deltas, 1 for a plane and 2 for a line.
The purpose of the function f in the above example is to make the final value coincide with what it should be; that's what I understood.
Using cylindrical coordinates (\rho, z, \phi), for the uniformly charged disk of radius R we have that \rho (\vec x)=\delta (z) \theta (\rho -R) f(\rho) where \theta (\rho - R) = 1 for \rho \leq R and 0 for \rho \geq R. Thus the theta function is a constraint that delimit the disk of radius R.
Then I don't really know what the professor has done, some integration I believe and he reached a final result I couldn't copy.
In spherical coordinates (r, \theta, \phi ) and for the same problem, he reached that \rho (\vec x) =\frac{Q}{\pi R^2 r} \delta (\theta - \frac{\pi}{2}) \hat \theta (r-R) which looks different from the result he reached in cylindrical coordinates but it must be the same.
If I understand well the final result, it has no sense to ask for the charge distribution in a particular point in \mathbb{R}^3. However it makes sense to ask for the charge distribution in any surface element; though I don't know how to proceed. I think I should do an integration or so, but I'm not sure and an example would be welcome.
So the final answer to the question is a function that is ill defined because for example in the origin it is not defined nor at the boundaries although there are charges there.
And if I'm not wrong, if I do integrate the final answer over an area (or volume?!) A, then I should get \sigma _0 A ? Namely the amount of charges enclosed into this small area? Is this right?
Why is the function "ill defined" as I call it? Is it because we DO NOT assume charges like points but like a property of a non zero space extension?
If I have the problem "What is the charge distribution of a uniformly charged cube?", I'd rather answer \rho _0 for -a \leq x \leq a, -a \leq y \leq a, -a \leq y \leq a. 0 everywhere else.
My answer wouldn't be ill defined and I could give you the charge distribution in any particular point in space, unlike the method used in more complicated problems.
The professor explained us how to do so (though many parts were unclear to me and I couldn't copy everything that was on the blackboard because we were too much students and I couldn't see the bottom part of the blackboard).
For a punctual charge, the general form of the charge distribution is \rho (\vec x) = q \delta (x) \delta (y) \delta (z).
For a charged plane: \rho (\vec x) = q \delta (z) and for a charged line: \rho (x,y,z)=q \delta (x) \delta (y).
However for a finite (in extension) plane perpendicular to the z-axis, \rho (\vec x) = f(x,y)\delta (z). The professor told us that the Dirac's delta "reduces" the dimension (though I don't understand why/how. If you have any comment on his, this would be nice). That's why for a point-like charge we need 3 of these deltas, 1 for a plane and 2 for a line.
The purpose of the function f in the above example is to make the final value coincide with what it should be; that's what I understood.
Using cylindrical coordinates (\rho, z, \phi), for the uniformly charged disk of radius R we have that \rho (\vec x)=\delta (z) \theta (\rho -R) f(\rho) where \theta (\rho - R) = 1 for \rho \leq R and 0 for \rho \geq R. Thus the theta function is a constraint that delimit the disk of radius R.
Then I don't really know what the professor has done, some integration I believe and he reached a final result I couldn't copy.
In spherical coordinates (r, \theta, \phi ) and for the same problem, he reached that \rho (\vec x) =\frac{Q}{\pi R^2 r} \delta (\theta - \frac{\pi}{2}) \hat \theta (r-R) which looks different from the result he reached in cylindrical coordinates but it must be the same.
If I understand well the final result, it has no sense to ask for the charge distribution in a particular point in \mathbb{R}^3. However it makes sense to ask for the charge distribution in any surface element; though I don't know how to proceed. I think I should do an integration or so, but I'm not sure and an example would be welcome.
So the final answer to the question is a function that is ill defined because for example in the origin it is not defined nor at the boundaries although there are charges there.
And if I'm not wrong, if I do integrate the final answer over an area (or volume?!) A, then I should get \sigma _0 A ? Namely the amount of charges enclosed into this small area? Is this right?
Why is the function "ill defined" as I call it? Is it because we DO NOT assume charges like points but like a property of a non zero space extension?
If I have the problem "What is the charge distribution of a uniformly charged cube?", I'd rather answer \rho _0 for -a \leq x \leq a, -a \leq y \leq a, -a \leq y \leq a. 0 everywhere else.
My answer wouldn't be ill defined and I could give you the charge distribution in any particular point in space, unlike the method used in more complicated problems.