How to Adjust Wave Function for a Particle in an Infinite Tube?

  • Thread starter Thread starter eit32
  • Start date Start date
  • Tags Tags
    Box Particle
eit32
Messages
21
Reaction score
0
If I know how to get a wave function for a 3-dimensional particle in a box problem, what adjustments must I make to solve the same problem for a particle traveling in the +z direction in a tube of infinite length?

Box:
0<x<a
0<y<b
0<z<c

Tube:
0<x<a
0<y<a
0<z<infinity
 
Physics news on Phys.org
Thats the basic idea. The primary effect of that, is that the wave number in the z direction won't have the same bounds.
Most likely the wave will be a real exponential (decaying or growing) -> and clearly it can't be growing unbounded.

Does that help? Try throwing the new boundary conditions into the differential wave equation.
 
well i think i problem I'm running into is that the wave function for the box isin the form of a sine function Asin((n pi x)/a)sin((n pi y)/b). sin((n pi z)/c). But if i just sub in my infinity then that doesn't really make sense, it just goes to sin(0).
 
the z portion is no longer a sin; its going to be e^ -kz for some constant k that you have to find from solving the wave equation with separation of variables.
 
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