The Sudden Approximation: Examining Perturbations on Atomic Electron Motion

  • Thread starter Thread starter bon
  • Start date Start date
  • Tags Tags
    Approximation
bon
Messages
547
Reaction score
0

Homework Statement



In the beta decay of tritium (1 proton, 2 neutron) to helium, the emitted electron has a kinetic energy of 19keV. We will consider the effects on the motion of the the atomic electron (the one orbiting the nucles) which we assume is initially in the ground state of tritium.

(a) show that the perturbation is sudden by considering the location of the emmitted electron at a time around T = 5x10^-7 s after emission. How does T compare with the time scale on which the wavefunciton changes.

Homework Equations





The Attempt at a Solution



Well I've worked out the electron would have traveled 3.75 x 10^-9 m. And i know the time scale the wavefn changes is hbar/E but which E do i use? the one for the atomic electron or the other electron? What is this meant to show?

Thanks
 
Physics news on Phys.org
anyone?
 
You're trying to see whether the perturbation on the atomic electron, by the emitted electron, is sudden. To do this, the question gives a time T by which the emitted electron would be very far from the nucleus. You're trying to compare T with the timescale on which the atomic electron's wavefunction changes, so it only makes sense to use the atomic electron's E.
 
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