QM 1-D Harmonic Oscillator Eigenfunction Problem

tis
Messages
2
Reaction score
0

Homework Statement


A particle of mass m moves in a 1-D Harmonic oscillator potential with frequency \omega.
The second excited state is \psi_{2}(x) = C(2 \alpha^{2} x^{2} + \lambda) e^{-\frac{1}{2} a^{2} x^{2}} with energy eigenvalue E_{2} = \frac{5}{2} \hbar \omega.

C and \lambda are constants. Show that the constant \lambda is not arbitrary.

NOTE: \int_{-\infty}^{\infty} e^{-\frac{1}{2} a x^{2}} dx = \sqrt{2\pi / a}, a > 0.

Homework Equations


That I can think of: TISE, normalization condition for wavefunctions.

The Attempt at a Solution


I assume there's a solution in substituting into the time-independent Schrodinger Equation and solving for \lambda, but the equation seems very difficult. And I have no idea how to utilize the hint provided; everything I've tried (normalization condition, etc.) just gives a dependence on C. I've scoured my textbooks with no luck, their only relevant info is using ladder operators and other methods to produce eigenfunctions.

Just after a point in the right direction. Thanks in advance for your help!
 
Physics news on Phys.org
Your idea to substitute this into the TISE seems like a good start. All you will have to do is take derivatives and rearrange some terms, and you will end up with an equation which determines lambda. Give it a try.
 
Figured it out. Take the ground state of the harmonic oscillator \psi_{0} = A e^{-\frac{1}{2}\alpha^{2} x^{2}} and use the orthogonality condition \int_{-\infty}^{\infty} \psi_{0}^{*} \psi_{2} \ dx = 0.

From there just expand, cancel out A* and C, and solve the integrals with integration by parts and the hint provided. Eventually you come to 0=2\alpha^{2}\frac{\sqrt{\pi}}{2\alpha^{3}}+\lambda\frac{\sqrt{\pi}}{ \alpha }, hence \lambda=-1.
 
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...
The value of H equals ## 10^{3}## in natural units, According to : https://en.wikipedia.org/wiki/Natural_units, ## t \sim 10^{-21} sec = 10^{21} Hz ##, and since ## \text{GeV} \sim 10^{24} \text{Hz } ##, ## GeV \sim 10^{24} \times 10^{-21} = 10^3 ## in natural units. So is this conversion correct? Also in the above formula, can I convert H to that natural units , since it’s a constant, while keeping k in Hz ?
Back
Top