Two-electron Ground State of a Spin-Independent Hamiltonian is a singlet

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SUMMARY

The discussion focuses on proving that the lowest energy state of a two-electron system governed by the Hamiltonian \(\mathcal{H} = -\frac{\hbar^2}{2m}(∇_1^2 + ∇_2^2) + V(r_1, r_2)\) is the singlet ground state energy \(E_s\) when symmetric wavefunctions are used, and the triplet ground state energy \(E_t\) when antisymmetric wavefunctions are employed. The proof involves analyzing the properties of the orbital wavefunction \(\psi(\mathbf{r}_1, \mathbf{r}_2)\) in a six-dimensional space, demonstrating that the absence of nodes in the wavefunction leads to a unique positive ground state. The conclusion is that the spin state must be antisymmetric, confirming that the only viable antisymmetric spin state for two electrons is the singlet state.

PREREQUISITES
  • Understanding of quantum mechanics principles, particularly the Schrödinger equation.
  • Familiarity with wavefunction properties and symmetries in quantum systems.
  • Knowledge of antisymmetry and symmetry in multi-particle quantum states.
  • Basic concepts of kinetic and potential energy in quantum mechanics.
NEXT STEPS
  • Study the implications of the Pauli exclusion principle in quantum mechanics.
  • Explore the properties of antisymmetric and symmetric wavefunctions in multi-particle systems.
  • Learn about the Euler-Lagrange equation and its applications in quantum mechanics.
  • Investigate the concept of nodes in wavefunctions and their impact on energy states.
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Students and educators in quantum mechanics, particularly those studying multi-electron systems, as well as researchers interested in the foundational aspects of quantum theory and wavefunction behavior.

wc2351
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Homework Statement


The problem is from Ashcroft&Mermin, Ch32, #2(a). (This is for self-study, not coursework.)

The mean energy of a two-electron system with Hamiltonian
\mathcal{H} = -\frac{\hbar^2}{2m}(∇_1^2 + ∇_2^2) + V(r_1, r_2)
in the state ψ can be written (after an integration by parts) in the form:
<br /> E = \int d{\bf r}_1 d{\bf r}_2 \left[\frac{\hbar^2}{2m}\{|∇_1\psi|^2 + |∇_2\psi|^2\} + V({\bf r}_1,{\bf r}_2)|\psi|^2 \right]<br />

Show that the lowest value of the above equation assumes over all normalized antisymmetric differentiable wavefunctions ψ that vanish at infinity is the triplet ground-state energy E_t, and that when symmetric functions are used the lowest value is the singlet ground-state energy E_s.

Homework Equations


Just basic knowledge of quantum mechanics? The proof should be elementary it seems...

The Attempt at a Solution



Before proving this theorem, it seemed natural to me that the ground state should be singlet because if the spin state is triplet, it is symmetric so the spatial wavefunction is anti-symmetric, and thus the existence of a node indicates that it has higher energy than the singlet wavefunction.

But I don't know how to proceed from the statement of the problem. Naive applicatin of the Euler-lagrange equation gives me Schrödinger's equation with zero energy. I don't know how I should use the parity of wavefunction since it is enclosed by the absolute signs.

Thank you for your help in advance.
 
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Hi wc2351,

it just so happens that I just solved this problem for the class I am TAing.

You have the right idea for the proof, but let me lay down the final steps in order for the benefit of anyone who might read it. The key is that the two-electrons Schrödinger equation for the orbital wavefunction \psi(\mathbf{r}_1,\mathbf{r}_2) can be viewed as the single-particle Schrödinger equation in 6 dimensions. Therefore, all we know about the single particle wavefunction also applies here.

I) As you point out, the orbital ground state cannot have any nodes because a node costs more kinetic energy than it can decrease the potential energy.

II) Because the Schrödinger equation is real, the eigenfunctions can always be chosen real. More precisely, if \psi is a solution to the time-independent Schrödinger equation, then so is \psi + \psi^*. Because the orbital ground state wavefunction has no nodes, it can then always be chosen positive.

III) As a bonus, this shows that the orbital ground state wavefunction is unique, because two positive wavefunctions cannot be orthogonal.

IV) Because the potential is symmetric under interchange of particles, we must have:

|\psi(\mathbf{r}_1,\mathbf{r}_2)|^2 = |\psi(\mathbf{r}_2,\mathbf{r}_1)|^2

But the wavefunction is real so:

\psi(\mathbf{r}_1,\mathbf{r}_2)^2= \psi(\mathbf{r}_2,\mathbf{r}_1)^2

and it can be chosen positive so we can take the square root:

\psi(\mathbf{r}_1,\mathbf{r}_2)= \psi(\mathbf{r}_2,\mathbf{r}_1)

i.e. the orbital ground state is symmetric.

V) By Pauli exclusion, the spin ground state must therefore be antisymmetric. But for two electrons, the only antisymmetric spin state is the singlet. That completes the proof.

B.D.
 

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