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

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SUMMARY

The discussion centers on the differences between the Pauli equation and the Schrödinger equation, particularly regarding the spin-dependent term in the Pauli equation. The term \(\frac{1}{2m}\left[\sigma\cdot\left(p-\frac{e}{c}A\right)\right]^2\) is analyzed to determine its equivalence to \(\frac{1}{2m}\left(p-\frac{e}{c}A\right)^2\). Participants conclude that the momentum operator and the electromagnetic potential do not commute, which complicates the derivation of the spin-dependent term. The final form of the equation includes additional terms that must be carefully considered, particularly the interaction of the electron's magnetic moment with the magnetic field.

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  • Understanding of quantum mechanics, specifically the Pauli equation and Schrödinger equation.
  • Familiarity with vector calculus, particularly curl and divergence operations.
  • Knowledge of quantum operators, including momentum and spin operators.
  • Basic understanding of electromagnetic theory, including vector potentials and magnetic fields.
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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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