Quantum Physics - Probabilities

jazznaz
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Homework Statement



A tritium atom is in the ground state and undergoes beta emission, creating a positively charged Helium ion. Assuming the nuclear change is instantaneous and there are no recoil effects, calculate the probability that the Helium ion will be found in its ground state...

Homework Equations



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The Attempt at a Solution



I've already shown that the form of the ground state energy eigenfunction is:

\psi (r) = \sqrt{\frac{Z^{3}}{\pi a_{0}^{3}}} e^{-\frac{Zr}{a_{0}}}

where Z is the nuclear charge and a_{0} is the Bohr radius.

I know that the ground state energy for a hydrogenic atom is E_{1}= 13.6 eV.

However, despite looking through my notes and a few books, I can't seem to set up the required probability calculation.

Any help or pointers would be very much appreciated.
 
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I am not exactly sure how I would do this either, but I think I have an idea behind what the question is trying to say. If someone else can spot my reply as being wrong, tell him so I don't point him in the wrong direction. Let me ask you this: how many electrons does tritium have? How many does the helium ion product have then? What does this tell you about the states of helium? Post again if you are still confused!
 
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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...
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