I Valid to use <1/r3> to get spin-orbit correction to H? (perturbation)

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The discussion focuses on the validity of using the expression <1/r^3> for spin-orbit correction in hydrogen, specifically questioning the appropriateness of the eigenstate ψ_{nlm} in perturbation theory. It is noted that ψ_{nlm} is not a "good state" due to its dependence on the m index, while "good states" are linear combinations of these eigenstates. Despite this, the value of <1/r^3> remains independent of m, leading to the conclusion that the linear combination will yield the same value. The conversation also addresses the concern about cross terms in the perturbation calculation, ultimately confirming that these terms are indeed zero. The thread emphasizes the nuances of applying perturbation theory to spin-orbit coupling in quantum mechanics.
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<1/r^3> uses the standard wavefunctions ψ_nlm of hydrogen, which are not good states to use in perturbation theory because the Hamiltonian (under spin-orbit interaction) no longer commutes with L. So shouldn't we solve for the simultaneous eigenstates of L^2, S^2, J^2 and J_z first? And then use those to find <1/r^3>?
Below is the derivation of E1so, the first-order correction to the Hamiltonian due to spin-orbit coupling of the election in hydrogen atom. My question is whether it's valid to use [6.64] (see below). ##<\frac{1}{r^3}>## I believe is ##<\psi_{nlm}|\frac{1}{r^3}|\psi_{nlm}>##, but ##\psi_{nlm}## is NOT a good state to use in perturbation theory, because ##\psi_{nlm}## is an eigenstate of ##L_{z}## but H'so does not commute with ##L## (as mentioned in the paragraph above [6.62]-[6.63]).

Screenshot 2024-06-24 at 1.46.49 AM.png

Screenshot 2024-06-24 at 1.46.24 AM.png

For elaboration, the phrase "good state" relates to the following theorem:

Screenshot 2024-06-24 at 1.53.20 AM.png

Screenshot 2024-06-24 at 1.53.34 AM.png

Ordinary first-order perturbation theory means using [6.9] below, with ##\psi^{0}_{n}## replaced with a good state.

Screenshot 2024-06-24 at 1.57.15 AM.png
 
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Happiness said:
Below is the derivation
Where is this from? Please give a reference.
 
PeterDonis said:
Where is this from? Please give a reference.
Introduction to Quantum Mechanics, 2nd edition, by David J. Griffiths
 
Indeed, the ##\psi_{nlm}## are not "good" functions, because of the ##m## index, and the "good" functions will be linear combinations of ##\psi_{nlm}## with different ##m##. However, the value of ##\braket{1/r^3}## is independent of ##m##, therefore you you know that the linear combination will have the given value, whichever ##m## states are combined.
 
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DrClaude said:
Indeed, the ##\psi_{nlm}## are not "good" functions, because of the ##m## index, and the "good" functions will be linear combinations of ##\psi_{nlm}## with different ##m##. However, the value of ##\braket{1/r^3}## is independent of ##m##, therefore you you know that the linear combination will have the given value, whichever ##m## states are combined.

But how do you know that the "cross terms" are zero?

Suppose a good state ##\psi^{0}=\alpha\psi_{a}+\beta\psi_{b}## , where ##\psi_{a}## and ##\psi_{b}## are some ##\psi_{nlm}## .

##\braket{\frac{1}{r^3}}=\braket{\alpha\psi_{a}+\beta\psi_{b}|\frac{1}{r^3}|\alpha\psi_{a}+\beta\psi_{b}}##

##=\alpha^2\braket{\psi_{a}|\frac{1}{r^3}|\psi_{a}}+\beta^2\braket{\psi_{b}|\frac{1}{r^3}|\psi_{b}}+\alpha^*\beta\braket{\psi_{a}|\frac{1}{r^3}|\psi_{b}}+\alpha\beta^*\braket{\psi_{b}|\frac{1}{r^3}|\psi_{a}}##

How do you know the cross terms ##\braket{\psi_{a}|\frac{1}{r^3}|\psi_{b}}## and ##\braket{\psi_{b}|\frac{1}{r^3}|\psi_{a}}## are zero?
 
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Happiness said:
How do you know the cross terms ##\braket{\psi_{a}|\frac{1}{r^3}|\psi_{b}}## and ##\braket{\psi_{b}|\frac{1}{r^3}|\psi_{a}}## are zero?
Ok, I've tried calculating them. They are indeed zero.
 
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