Why isn't the Pauli equation equivalent to the Schrodinger equation?

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Discussion Overview

The discussion centers on the relationship between the Pauli equation and the Schrödinger equation, particularly focusing on the implications of spin and the role of various terms in the equations. Participants explore the mathematical structure and physical interpretations of these equations, including operator commutation and the treatment of electromagnetic potentials.

Discussion Character

  • Technical explanation
  • Mathematical reasoning
  • Debate/contested

Main Points Raised

  • One participant presents a calculation suggesting that the spin-dependent term in the Pauli equation could be equivalent to a term in the Schrödinger equation, questioning the nature of spin dependence.
  • Another participant challenges this by suggesting that the vector B should be treated as a vector operator, indicating that the commutation relations complicate the equivalence.
  • A later reply acknowledges the issue of non-commuting operators and expresses a belief that this is the source of confusion in the original calculation.
  • Further contributions explore the final form of the Pauli equation, questioning whether certain terms are typically neglected and seeking clarification on their significance.
  • Participants discuss the implications of the curl of the vector potential and its relation to the magnetic field, with one noting the importance of being careful with operator combinations.
  • There is a suggestion that the treatment of the curl operator should be viewed in the context of its action on wave functions, rather than as a direct multiplication by the magnetic field.

Areas of Agreement / Disagreement

Participants express differing views on the equivalence of terms in the Pauli and Schrödinger equations, with some agreeing on the complexity introduced by non-commuting operators while others remain uncertain about the implications of certain terms. The discussion does not reach a consensus on the nature of spin dependence or the treatment of specific terms.

Contextual Notes

Limitations include assumptions about operator commutation and the treatment of vector potentials, which are not fully resolved in the discussion. The mathematical steps involved in the derivations are also not completely worked out, leaving some ambiguity in the conclusions drawn by participants.

pellman
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The Pauli equation (seen here) contains its spin dependence in the term which reads

\frac{1}{2m}\left[ \sigma\cdot\left(p-\frac{e}{c}A\right)\right]^2

So let B be any vector. Then

\left( \sigma\cdot B\right)^2
=\left(\sigma_1 B_1 +\sigma_2 B_2 + \sigma_3 B_3\right)\left(\sigma_1 B_1 +\sigma_2 B_2 + \sigma_3 B_3\right)
=\sigma_1^2 B_1^2 +\sigma_2^2 B_2^2+\sigma_3^2 B_3^2 + (\sigma_1\sigma_2+\sigma_2\sigma_1)B_1 B_2 + (\sigma_1\sigma_3+\sigma_3\sigma_1)B_1 B_3 + (\sigma_3\sigma_2+\sigma_2\sigma_3)B_3 B_2
=1\cdot B_1^2 + 1\cdot B_2^2 + 1\cdot B_3^2 + 0 + 0 +0
=B^2

So isn't the sigma-dependent term in the Pauli equation identically equal to

\frac{1}{2m}\left(p-\frac{e}{c}A\right)^2

?

if yes, then in what sense is it spin-dependent? If no, then where did I go wrong?
 
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I have only briefly looked at your calculation and it looks correct, but I don't think you are calculating what you really want. (By the way, I assume that the identity matrix is implied in your notation.)

Try to do the same, but now assume that B is a vector operator. So in general \sigma_1\sigma_2B_1B_2 + \sigma_2\sigma_1B_2B_1 \neq (\sigma_1\sigma_2 + \sigma_2\sigma_1)B_1B_2, since you don't always have [B_1,B_2] = 0.
 
Thanks, element4. I get it now. The momentum operator and the EM potential do not commute since the latter is a function of position, so the B^2 terms in my derivation are not so simple. Haven't worked it out yet, but I'm pretty sure that's it.
 
Ok. So I worked through it and have one more nagging question. The final form I get is

\left\{\frac{1}{2m}\left(\vec{p}-\frac{e}{c}\vec{A}\right)^2-\frac{e\hbar}{2mc}\vec{\sigma}\cdot\vec{B}+e\Phi-i\hbar\frac{\partial}{\partial t}\right\}\Psi-\frac{e\hbar}{mc}\vec{\sigma}\cdot\left(\vec{A}\times\nabla\right)\Psi=0

The part in the braces is familiar and can also be seen on the wikipedia page: http://en.wikipedia.org/wiki/Pauli_equation#Special_Cases What about the last term? Is it something typically neglected? Why? Or did I screw up the derivation?
 
The correct result is not AXdel. It should be curl A, which equals B because the curl does not act on psi. This just gives -mu.B, the interaction of the electron magnetic moment with B. This result also derives the g=2 for electron magnetic moment. Be more careful with the combination -[del.A + A.del]psi.
 
Thanks, Meir Achuz. But the term containing

\frac{1}{2m}\left[ \sigma\cdot\left(p-\frac{e}{c}A\right)\right]^2

when expanded results in both A\times\nabla and \nabla\times A terms (I think). I have the \nabla\times A covered above in the term containing B. But I don't know what to do with the A\times\nabla term
 
Bump.

Just one little bump.
 
I did not work this through, but I think the del X A term does not equal B. It's the same way with [P, X] = (d/dx)*x - x*(d/dx) != 1 - x*(d/dx).
 
Last edited:
yangjong said:
I did not work this through, but I think the del X A term does not equal B. It's the same way with [P, X] = (d/dx)*x - x*(d/dx) != 1 - x*(d/dx).

thank you for your reply, yangjong. And welcome to the board!

I think what you are suggesting is that when I see \nabla\times A I should not read this as "multiply by B" but rather consider it an operator: when acting on a function \Psi it yields \nabla\times (A\Psi).

That is, where I wrote

\left\{\frac{1}{2m}\left(\vec{p}-\frac{e}{c}\vec{A}\right)^2-\frac{e\hbar}{2mc}\vec{\sigma}\cdot\vec{B}+e\Phi \Psi -i\hbar\frac{\partial}{\partial t}\right\}\Psi-\frac{e\hbar}{mc}\vec{\sigma}\cdot\left(\vec{A}\times\nabla\right)\Psi=0

above, it should be instead

\left\{\frac{1}{2m}\left(\vec{p}-\frac{e}{c}\vec{A}\right)^2\Psi-\frac{e\hbar}{2mc}\vec{\sigma}\cdot\left(\nabla\times [\vec{A}\Psi]\right)+e\Phi\Psi -i\hbar\frac{\partial\Psi}{\partial t}\right\}-\frac{e\hbar}{mc}\vec{\sigma}\cdot\left(\vec{A}\times\nabla\right)\Psi=0

\left\{\frac{1}{2m}\left(\vec{p}-\frac{e}{c}\vec{A}\right)^2\Psi-\frac{e\hbar}{2mc}\vec{\sigma}\cdot\left(\nabla\Psi\times \vec{A} +\Psi\nabla\times \vec{A}\right)+e\Phi\Psi -i\hbar\frac{\partial\Psi}{\partial t}\right\}-\frac{e\hbar}{mc}\vec{\sigma}\cdot\left(\vec{A}\times\nabla\right)\Psi=0

\left\{\frac{1}{2m}\left(\vec{p}-\frac{e}{c}\vec{A}\right)^2\Psi-\frac{e\hbar}{2mc}\vec{\sigma}\cdot\left(\Psi\nabla\times \vec{A}\right)+e\Phi\Psi -i\hbar\frac{\partial\Psi}{\partial t}\right\}=0

\left\{\frac{1}{2m}\left(\vec{p}-\frac{e}{c}\vec{A}\right)^2-\frac{e\hbar}{2mc}\vec{\sigma}\cdot\vec{B}+e\Phi-i\hbar\frac{\partial}{\partial t}\right\}\Psi =0

That's it. Thank you!
 

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