How is spin exchange interaction generalised to many electrons?

In summary, the spin exchange interaction can be generalized to many electrons by considering the collective behavior of multiple spin-1/2 particles within a system. This involves extending the concept of pairwise interactions to include interactions among larger groups of spins, often described using many-body quantum mechanics. Techniques such as mean-field theory, perturbation theory, and the use of exchange operators help in formulating the effective Hamiltonians that capture the complexities of many-electron systems, accounting for factors like symmetry, correlations, and the overall spin state of the system. This generalization is crucial for understanding phenomena in condensed matter physics, such as magnetism and superconductivity.
  • #1
gaiussheh
15
2
TL;DR Summary
In solid state physics or statistical physics, the many-body spin Hamiltonian is written as ##-E_{i,j}\sum_{i,j} \hat{S}_{i}\cdot \hat{S}_j##. How is this generalised from the two-electron case?
In solid state physics or statistical physics, the many-body spin Hamiltonian is written as ##\sum_{i,j} \hat{S}_{i}\cdot \hat{S}_j##. I referred to many textbooks, and most of them just generalised this from the two-electron case ##\hat{S}_{1}\cdot \hat{S}_2##. While this seems natural, it is completely unlogical as this is not the magnetic dipole itself but the exchange interaction that arose from the symmetry of the spatial wave function.

Take a step back. Two electrons can form either a singlet or a triplet. For a singlet, ##\hat{S}_{1}\cdot \hat{S}_2=-\frac{3}{4}## and the spin part is symmetric, hence the spatial part is antisymmetric. For a triplet, ##\hat{S}_{1}\cdot \hat{S}_2=\frac{1}{4}## and the spin part is antisymmetric, hence the spatial part is asymmetric. This arise different energies ##E_{\rm S}=\langle\psi_{\rm S}|\hat{\mathcal{H}}|\psi_{\rm S}\rangle## and ##E_{\rm T}=\langle\psi_{\rm T}|\hat{\mathcal{H}}|\psi_{\rm T}\rangle##. However, both can be written as

##E_{\rm T} = \frac{1}{4}E_{\rm S}+\frac{3}{4}E_{T}-\frac{1}{4}(E_{\rm S}-E_{\rm T})##
##E_{\rm S} = \frac{1}{4}E_{\rm S}+\frac{3}{4}E_{T}+\frac{3}{4}(E_{\rm S}-E_{\rm T})##
Hence in any case ##E=\frac{1}{4}E_{\rm S}+\frac{3}{4}E_{T}-\hat{S}_{1}\cdot \hat{S}_2(E_{\rm S}-E_{\rm T})##
The energy due to spin is ##-E_{1,2}\hat{S}_{1}\cdot \hat{S}_{2}##, where ##E_{1,2} = E_{\rm S}-E_{\rm T}##.

I find it not that easy to generalise to a many-body system. In general, you will need a Slater determinant to describe the wave function and consider the effect of exchanging any two electrons. I don't even know if it is possible to write this into the form of ##\psi_{\rm spatial}[{\vec r}_1, {\vec r}_2, \cdots, {\vec r}_n]\cdot[{\rm spin~of~i~and~j}] \cdot[{\rm spin~of~other~electrons}]## etc. (Actually, I think you can't let the slater determinant be an eigenstate of ##\hat{S}_{i}\cdot \hat{S}_j## for all pair of ##i,j##).

How is this generalised at all?
 
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  • #2
Do you know second quantization? It was invented for this purpose.
 
Last edited:
  • #3
pines-demon said:
Do you know second quantization? It was invented for this purpose.
I know how this is done in a serious solid-state course, but I'm teaching second-year students, so better not to introduce that. Is there a way to fix it using simple QM?
 

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