Non-Stationary State Wavefunction - Normalized? <L^2>? Uncertainty on L^2?

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SUMMARY

The nonstationary state wavefunction \(\Psi = \sqrt{\frac{1}{3}}\Psi_{22-1} + \sqrt{\frac{2}{3}}\Psi_{110}\) is properly normalized, as confirmed by the calculation yielding \(\big< \Psi \, \big\lvert \, \Psi \big> = 1\). The expectation value of \(L^{2}\) can be calculated using the orthonormality of the states, resulting in \(\big = \frac{1}{3} \hbar^2 2(2+1) + \frac{2}{3} \hbar^2 1(1+1)\). The uncertainty in \(L^{2}\) is not zero, despite \(L^{2}\) being calculated from orthogonal states, as the uncertainty formula \(\Delta L^{2} = \sqrt{<(L^{2})^{2}> - ^{2}}\) must be applied.

PREREQUISITES
  • Understanding of quantum mechanics, specifically wavefunctions and their normalization.
  • Familiarity with angular momentum operators, particularly \(L^{2}\) in quantum systems.
  • Knowledge of orthonormality conditions for quantum states.
  • Ability to apply expectation value calculations in quantum mechanics.
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  • Study the concept of expectation values in quantum mechanics, focusing on operators like \(L^{2}\).
  • Learn about the properties of orthonormal states and their implications in quantum mechanics.
  • Explore the derivation and application of the uncertainty principle in quantum systems.
  • Investigate the role of radial potentials in quantum mechanics and their effect on wavefunctions.
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Students and professionals in quantum mechanics, particularly those studying angular momentum and wavefunction normalization. This discussion is beneficial for anyone seeking to deepen their understanding of nonstationary states and their properties in quantum systems.

mkosmos2
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Homework Statement



Consider the nonstationary state:

\Psi = \sqrt{\frac{1}{3}}\Psi_{22-1} + \sqrt{\frac{2}{3}}\Psi_{110}

Where \Psi_{22-1} and \Psi_{110} are normalized, orthogonal and stationary states of some radial potential. Is \Psi properly normalized? Calculate the expectation value of L^{2} and the uncertainty in L^{2} for a particle in this state.

Homework Equations



|a_{n_{1}l_{1}m_{1}}|^{2} + |a_{n_{2}l_{2}m_{2}}|^{2} = 1 (1)

&lt;L^{2}&gt; = \int_{all{}\Omega}\Psi^{*}(-\hbar^{2}\Lambda^{2})\Psi d\tau (2)

\Delta L^{2} = \sqrt{&lt;(L^{2})^{2}&gt; - &lt;L^{2}&gt;^{2}} (3)

The Attempt at a Solution



For the first part, I think it's safe in this situation to use equation (1) where the a_{nlm} terms are the two coefficients in \Psi, but I'm not sure if it applies when the quantum numbers aren't the same for the two stationary states.

For the second part, still not positive, but I think if I use equation (2), the L^{2} operator results in \hbar^{2}l(l+1) coming outside the integral, and because the two states are orthogonal, the integral and therefore L^{2} goes to 0.

The last part has me tripped up the most because I don't know whether L^{2} being zero automatically means the uncertainty is zero, but something tells me it's not that simple.

I'm just fuzzy on a lot of the concepts surrounding this topic so any clarification/confirmation will be much, much appreciated.

Thank you very much for your time, and if these answers are correct, sorry I wasted it :s

-Mike
 
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Ok, for the first part, all you need to know is that the states are orthogonal and normalized. This means
\big&lt; \Psi_{n&#039;l&#039;m&#039;} \big\lvert \, \Psi_{nlm} \big&gt; =\big&lt;n&#039;l&#039;m&#039; \big\lvert \,nlm\big&gt; = 0~~ \text{if}~~nlm=n&#039;l&#039;m&#039;;~1~~\text{if}~~nlm \ne n&#039;l&#039;m&#039;
So for your state, we have
\big&lt; \Psi \, \big\lvert \, \Psi \big&gt; =\bigg( \sqrt{ \frac{1}{3}} \Psi_{22-1}^*+ \sqrt{ \frac{2}{3}} \Psi_{110}^* \bigg)\bigg( \sqrt{ \frac{1}{3}} \Psi_{22-1}+ \sqrt{ \frac{2}{3}} \Psi_{110} \bigg)= \frac{1}{3}(1)+ \frac{2}{3}(1) + \frac{2}{6}(0)\frac{2}{6}(0)= \frac{3}{3} =1
So yes, it is normalized.
For the second part,
L^2 \big\lvert \,nlm \big&gt; = \hbar^2 l(l+1) \big\lvert \,nlm \big&gt;
or
\big&lt;n&#039;l&#039;m&#039; \big\lvert L^2 \big\lvert \,nlm \big&gt; = \big&lt;n&#039;l&#039;m&#039;\big\lvert \hbar^2 l(l+1) \big\lvert \,nlm \big&gt; = \hbar^2 l(l+1)~~\text{if}~ l=l&#039;;~~0~~ \text{if} ~~l \ne l&#039;
so,
\begin{multline}\big&lt;L^2 \big&gt; = \frac{1}{3} \big&lt;22-1 \big\lvert \,\hbar^2 2(2+1) \big\lvert 22-1 \big&gt; +\frac{2}{3} \big&lt;110 \big\lvert \,\hbar^2 1(1+1) \big\lvert 110 \big&gt;\\ = \frac{1}{3} \hbar^2 2(2+1) \big&lt;22-1 \big\lvert \ 22-1 \big&gt; +\frac{2}{3} \hbar^2 1(1+1) \big&lt;110 \big\lvert \, 110 \big&gt; = \frac{1}{3} \hbar^2 2(2+1) +\frac{2}{3} \hbar^2 1(1+1) \end{multline}

and etc. You get the idea. By the way, you need to do NO integration on this problem. That's the beauty of orthonormality.
 
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