Sakura page 85: how to do this proof?

  • Context: Graduate 
  • Thread starter Thread starter omoplata
  • Start date Start date
  • Tags Tags
    Proof
Click For Summary

Discussion Overview

The discussion revolves around proving two equations from "Modern Quantum Mechanics" by J. J. Sakurai, specifically equations (2.2.23a) and (2.2.23b), which involve commutation relations in quantum mechanics. Participants explore methods to apply a specific commutation relation (1.6.50e) to derive the results, engaging in technical reasoning and mathematical expansions.

Discussion Character

  • Technical explanation
  • Mathematical reasoning
  • Debate/contested

Main Points Raised

  • One participant seeks clarification on how to prove the commutation relations using the provided equation (1.6.50e).
  • Another suggests using a Taylor expansion of the function F(p) and calculating the commutator [x, p^n].
  • A different participant emphasizes the need to expand F(p) and apply derivatives to the expansion in the context of the commutator.
  • Concerns are raised about ignoring higher-order terms in the expansion, questioning the validity of that approach.
  • One participant proposes explicitly calculating [x, p^n] for small n and then generalizing the result through induction.
  • Another participant suggests an alternative method involving the action of the commutator on wavefunctions in momentum and position space, arguing it may be simpler.
  • There is a discussion about the correctness of terms in the calculations, with participants correcting each other on the application of the commutation relation.
  • A participant expresses uncertainty about whether the procedure for a vector p differs from that for a scalar, noting potential complications in the Taylor expansion.

Areas of Agreement / Disagreement

Participants express differing views on the best approach to proving the equations, with some advocating for Taylor expansions while others suggest alternative methods. There is no consensus on the most effective or simplest method to arrive at the proof.

Contextual Notes

Participants note the complexity of dealing with vector quantities in the Taylor expansion and the implications for the overall proof process. The discussion also highlights the need for careful handling of higher-order terms and the application of the commutation relation.

omoplata
Messages
327
Reaction score
2
From "Modern Quantum Mechanics, revised edition" by J. J. Sakurai, page 85.

Eqn (2.2.23a),<br /> [x_i,F(\mathbf{p})] = i \hbar \frac{\partial F}{\partial p_i}<br />Eqn(2.2.23b)<br /> [p_i,G(\mathbf{x})] = -i \hbar \frac{\partial G}{\partial x_i}
It says "We can easily prove both formulas by repeatedly applying (1.6.50e)."

(1.6.50e) is,<br /> [A,BC]=[A,B]C+B[A,C]

I can't figure it out. How do I do this?
 
Physics news on Phys.org
Say you taylor expand the function. Then you just need to figure out what is e.g. [x,p^n]
 
Hi, in the case of

\begin{bmatrix}x,F(p)\end{bmatrix}

for the unidimensional variable x for example, you must write \textit{F(p)} as an expansion.

Then,

F(P) = sum Cn.p^n

Then apply the derivate to the expansion and replace in the commutator.

Keep trying and let us know if you could.

Regards
 
Thanks for the help.

Like this?
<br /> F(\mathbf{p}) = F(\mathbf{0}) + \Sigma_{n=1}^\infty \left( \frac{\partial^n F(\mathbf{p})}{\partial p^n} \right)_{\mathbf{p} = \mathbf{0}} \frac{\mathbf{p}^n}{n!}<br />
Then,<br /> \left[ x_i, F(\mathbf{p}) \right] = \left[ x_i, F(\mathbf{0}) + \Sigma_{n=1}^\infty \left( \frac{\partial^n F(\mathbf{p})}{\partial p^n} \right)_{\mathbf{p} = \mathbf{0}} \frac{\mathbf{p}^n}{n!}<br /> \right] = \left[ x_i, \Sigma_{n=1}^\infty \left( \frac{\partial^n F(\mathbf{p})}{\partial p^n} \right)_{\mathbf{p} = \mathbf{0}} \frac{\mathbf{p}^n}{n!}<br /> \right]<br />, and ignore second order and higher terms, and take \left( \frac{\partial F(\mathbf{p})}{\partial p} \right)_{\mathbf{p} = \mathbf{0}} to be a constant?
 
omoplata said:
and ignore second order and higher terms, and take \left( \frac{\partial F(\mathbf{p})}{\partial p} \right)_{\mathbf{p} = \mathbf{0}} to be a constant?
Why would you ignore the higher order terms? You will need to work out ##[x,p^{n}]##, as jeppetrost mentioned earlier.
Isn't \left( \frac{\partial F(\mathbf{p})}{\partial p} \right)_{\mathbf{p} = \mathbf{0}} a constant to begin with?
 
You use (1.6.50e) to find ##[x,p^n]##. The proper way is to do it explicitly for the first few values of n, then guess the formula for arbitrary n, and finally prove by induction that your guess is correct.
 
OK, I almost got it this time.
<br /> \begin{eqnarray}<br /> \left[ x_i, F(\mathbf{p}) \right] &amp; = &amp; \left[ x_i, F(\mathbf{0}) + \Sigma_{n=1}^\infty \left( \frac{\partial^n F(\mathbf{p})}{\partial p^n} \right)_{\mathbf{p} = \mathbf{0}} \frac{\mathbf{p}^n}{n!} \right]\\<br /> &amp; = &amp; \left[ x_i, \Sigma_{n=1}^\infty \left( \frac{\partial^n F(\mathbf{p})}{\partial p^n} \right)_{\mathbf{p} = \mathbf{0}} \frac{\mathbf{p}^n}{n!} \right]\\<br /> &amp; = &amp; \Sigma_{n=1}^\infty \left( \frac{\partial^n F(\mathbf{p})}{\partial p^n} \right)_{\mathbf{p} = \mathbf{0}} \frac{1}{n!} \left[x_i, \mathbf{p}^n \right]<br /> \end{eqnarray}<br />
Then,
<br /> \left[x_i,\mathbf{p}^n \right]<br /> = \left[x_i,\mathbf{p} \cdot \mathbf{p}^{n-1} \right] = \left[x_i,\mathbf{p} \right] \mathbf{p}^{n-1} + x_i \left[\mathbf{p}, \mathbf{p}^{n-1} \right] = i \hbar \mathbf{p}^{n-1}<br />
Plugging this back in,
<br /> \begin{eqnarray}<br /> \left[ x_i, F(\mathbf{p}) \right]<br /> &amp; = &amp; i \hbar \Sigma_{n=1}^\infty \left( \frac{\partial^n F(\mathbf{p})}{\partial p^n} \right)_{\mathbf{p} = \mathbf{0}} \frac{\mathbf{p}^{n-1}}{n!}\\<br /> &amp; = &amp; i \hbar \Sigma_{n=1}^\infty \left( \frac{\partial^{n-1} \left( \frac{ \partial F(\mathbf{p})}{\partial p} \right) } {\partial p^{n-1}} \right)_{\mathbf{p} = \mathbf{0}} \frac{\mathbf{p}^{n-1}}{n!}\\<br /> &amp; = &amp; i \hbar \Sigma_{n=0}^\infty \left( \frac{\partial^{n} \left( \frac{ \partial F(\mathbf{p})}{\partial p} \right) } {\partial p^{n}} \right)_{\mathbf{p} = \mathbf{0}} \frac{\mathbf{p}^{n}}{(n+1)!}<br /> \end{eqnarray}<br />
If I somehow changed that (n+1) to an n, that would be the answer. Where did I go wrong?
 
omoplata said:
<br /> \left[x_i,\mathbf{p}^n \right]<br /> = \left[x_i,\mathbf{p} \cdot \mathbf{p}^{n-1} \right] = \left[x_i,\mathbf{p} \right] \mathbf{p}^{n-1} + x_i \left[\mathbf{p}, \mathbf{p}^{n-1} \right]
That last term is wrong. Look at (1.6.50e) again.
 
I'm pretty sure there are other, easier, ways to solve this problem. For example one could consider the action of the commutator on the wavefunction in momentum space for Eqn (2.2.23a), and in position space for Eqn (2.2.23b).

<br /> [p_i,G(\mathbf{x})]\psi \leftrightarrow -i\hbar \frac{\partial }{\partial x_i} \left( G(\mathbf{x})\psi(\mathbf{x})\right) - G(\mathbf{x}) \left( -i\hbar \frac{\partial }{\partial x_i}\psi(\mathbf{x}) \right) = -i\hbar\left.\frac{\partial G}{\partial x_i}\right|_{\mathbf{x}} \psi(\mathbf{x})

There is no loss of rigor doing it this way. From the result above [p_i,G(\mathbf{x})] clearly has the \mathbf{x} eigenbasis with eigenvalues -i\hbar\left.\frac{\partial G}{\partial x_i}\right|_{\mathbf{x}}.
 
Last edited:
  • #10
That's an interesting approach MisterX. I think it requires a deeper understanding of what we're allowed to do, so I'm not sure I can agree that it's easier (for a typical student of Sakurai), but your solution is certainly much shorter.
 
  • #11
Fredrik said:
That last term is wrong. Look at (1.6.50e) again.

Yeah, thanks. Correcting that,
<br /> \begin{eqnarray}<br /> \left[x_i,\mathbf{p}^n \right] &amp;<br /> = &amp; \left[x_i,\mathbf{p} \cdot \mathbf{p}^{n-1} \right]<br /> = \left[x_i,\mathbf{p} \right] \mathbf{p}^{n-1} + \mathbf{p} \left[x_i, \mathbf{p}^{n-1} \right]\\<br /> <br /> \left[x_i,\mathbf{p}^{n-1} \right] &amp;<br /> = &amp; \left[x_i,\mathbf{p} \cdot \mathbf{p}^{n-2} \right]<br /> = \left[x_i,\mathbf{p} \right] \mathbf{p}^{n-2} + \mathbf{p} \left[x_i, \mathbf{p}^{n-2} \right]\\<br /> &amp; \dots &amp; \\<br /> \end{eqnarray}<br />
So,
<br /> [x_i,\mathbf{p}^n] = n i \hbar \mathbf{p}^{n-1}<br />
Therefore,
<br /> \begin{eqnarray} <br /> \left[ x_i, F(\mathbf{p}) \right] <br /> &amp; = &amp; i \hbar \Sigma_{n=1}^\infty \left( \frac{\partial^n F(\mathbf{p})}{\partial p^n} \right)_{\mathbf{p} = \mathbf{0}} \frac{\mathbf{p}^{n-1}}{(n-1)!}\\ <br /> &amp; = &amp; i \hbar \Sigma_{n=1}^\infty \left( \frac{\partial^{n-1} \left( \frac{ \partial F(\mathbf{p})}{\partial p} \right) } {\partial p^{n-1}} \right)_{\mathbf{p} = \mathbf{0}} \frac{\mathbf{p}^{n-1}}{(n-1)!}\\ <br /> &amp; = &amp; i \hbar \Sigma_{n=0}^\infty \left( \frac{\partial^{n} \left( \frac{ \partial F(\mathbf{p})}{\partial p} \right) } {\partial p^{n}} \right)_{\mathbf{p} = \mathbf{0}} \frac{\mathbf{p}^{n}}{n!}\\<br /> &amp; = &amp; \frac{\partial F(\mathbf{p})}{\partial p}\\<br /> \end{eqnarray}<br />
,which is the solution.

One small final question. I think \mathbf{p} here is a vector. In the above, I did the same as I would do for a scalar. Would the procedure be different for a vector.
 
  • #12
omoplata said:
One small final question. I think \mathbf{p} here is a vector. In the above, I did the same as I would do for a scalar. Would the procedure be different for a vector.
Yes, the Taylor expansion would more complicated, and that makes the rest of it more complicated as well. You can still use the same idea, but the notation will be a pain. The multi-index notation used here can probably reduce that pain.
 
Last edited:

Similar threads

  • · Replies 5 ·
Replies
5
Views
998
  • · Replies 3 ·
Replies
3
Views
1K
  • · Replies 1 ·
Replies
1
Views
977
  • · Replies 0 ·
Replies
0
Views
1K
  • · Replies 11 ·
Replies
11
Views
2K
  • · Replies 5 ·
Replies
5
Views
3K
  • · Replies 7 ·
Replies
7
Views
2K
  • · Replies 3 ·
Replies
3
Views
4K
  • · Replies 19 ·
Replies
19
Views
4K
  • · Replies 2 ·
Replies
2
Views
2K