Solving Charge Distribution for Spheres with Different Material Properties

IxRxPhysicist
Messages
34
Reaction score
0
Hey all,
So the question in Jackson 1.4 is that I have 3 spheres that all have a total charge Q on them, but each sphere has different material properties. For instance, I have a conducting sphere, a sphere with a uniform charge distribution, and one with a charge distribution that has a charge distribution that varies as rn. It's the last one I am having trouble with, how can I get an r dependence in ρ without screwing up the units? I tried something like:

ρ(r) ∝ ρo*(rn+1/rn)

buuuuut that still leaves me some messed up units.

Also, ρ0 = 3Q/(4πr3)

Any ideas?
 
Physics news on Phys.org
You can have \rho(r) = \rho_0 \, r^n, but the units of \rho_0 will not be \rm \frac{Coulombs}{cm^3}, they will be \rm \frac{Coulombs}{cm^{3+n}},. And then you have to determine \rho_0 by integrating the total charge over the sphere to give Q.
 
Whoa whoa ρ can take on arbitrary units? Like Coulombs/cm3+n? The units just have to balance out in ∫ ρ dV = Q?...Also as an aside, are you using LaTex or something because I like the format in your response.
 
Yes, \rho_0 is just a constant in your equations that can have whatever units it needs to to make the units come out right. In that case it's not a charge density any more.

This link shows you how to include latex in your posts.
 
Interesting, learned something new. I just learned mathematica so I guess I will put LaTex on my to do list. Thanks!
 
Hello everyone, I’m considering a point charge q that oscillates harmonically about the origin along the z-axis, e.g. $$z_{q}(t)= A\sin(wt)$$ In a strongly simplified / quasi-instantaneous approximation I ignore retardation and take the electric field at the position ##r=(x,y,z)## simply to be the “Coulomb field at the charge’s instantaneous position”: $$E(r,t)=\frac{q}{4\pi\varepsilon_{0}}\frac{r-r_{q}(t)}{||r-r_{q}(t)||^{3}}$$ with $$r_{q}(t)=(0,0,z_{q}(t))$$ (I’m aware this isn’t...
Hi, I had an exam and I completely messed up a problem. Especially one part which was necessary for the rest of the problem. Basically, I have a wormhole metric: $$(ds)^2 = -(dt)^2 + (dr)^2 + (r^2 + b^2)( (d\theta)^2 + sin^2 \theta (d\phi)^2 )$$ Where ##b=1## with an orbit only in the equatorial plane. We also know from the question that the orbit must satisfy this relationship: $$\varepsilon = \frac{1}{2} (\frac{dr}{d\tau})^2 + V_{eff}(r)$$ Ultimately, I was tasked to find the initial...
Back
Top