The two-electron atom is a physical system modeling an atom with two electron around and arbitrary nucleus. It is a generalization of the hydrogenic atom. The key challenge of the system is the indistinguishability of electrons and their effective interaction due to the Pauli exclusion principle. The Hamiltonian of the system is
Spin states#
The solved eigenfunction (in position representation) will be of the form , where and are the generalized coordinates of the electrons (containing both position and spin state). Electrons are Spin fermions and so must be an antisymmetric state: . Since does not directly depend on spin, we can factor out the spin and leave a coordinate-only and spin-only wavefunction:
The spin wavefunction can be constructed from the individual spin wavefunctions and . We denote and the spin operators of the electrons and by and their components. Each spin state is described by an eigenfunction, but since we are working with spin , there's only two possible functions per electron, one for spin up and one for spin down. We'll call these and respectively and denote which electron they refer to with a number. only acts on and , whereas only acts on and . In turn, this means that and commute.
The total spin is and the total component is . The square of the total is
since . Since the interaction between electrons is purely electromagnetic, it is independent of spin. As such, each electron's spin is simply either up or down without reference to the other, which leads to four distinct spin states:
Applying the spin operator to leads to
Clearly, the total spin over in the spin state is (in units). More generally, we have
By doing the math for all four functions, we find that , in that order. There's evidently some degeneracy on . Moreover, while and are symmetric under label exchange, and are not, and are also not antisymmetric. As such, the actual states must be normalized linear combinations of the two that are (anti)symmetric under label exchange:
The is symmetric, the is antisymmetric. These two functions are eigenstates of and , with eigenvalues and for and and for . We now have four spin states, divided in one state with and three states with . The former is called the singlet state
and is antisymmetric. The latter three are known as the triplet states
and are all symmetric. At this point, since the wave functions that describe a two-electron atom must be antisymmetric (because fermions must obey the Pauli exclusion principle), we only have two options:
- Parastates are wavefunctions where the spin component is antisymmetric (spin singlet) and the spatial component is symmetric.
- Orthostates are wavefunctions where the spin component is symmetric (spin triplet) and the spatial component is antisymmetric.
Independent particle model#
The electrons repel each other electrically due to having identical electric charge. However, as a first, somewhat qualitative approximation, we can solve the system by neglecting the interaction term. This is a so-called independent particle model[^1] This makes for two independent electrons around the same nucleus. Following perturbation theory, we rewrite the Hamiltonian as
where the electron-electron interaction
is the perturbation. We will choose to ignore this and deal with the consequences later.
Now that we no longer have coupling due to interaction, we can safely claim that the spatial wavefunction is the product of two independent, hydrogen atom wavefunctions
where for clearer notation.
must be invariant under particle exchange (to respect the indistinguishability of electrons. Since the spatial wavefunction can be either even or odd (since the spin state can also be either even or odd, so long it's the other kind), we can write the wavefunctions as one of two different linear combinations:
As before, is symmetric, is antisymmetric. A note: if , the antisymmetric combination vanishes. This is correct and what we'd hoped for. After all, this is really just the Pauli exclusion principle at play: two electrons cannot possibly have the same quantum numbers at the same time. In fact, if two electrons have the same spatial state, their spins must differ (i.e., be opposite), but if the spins are opposite then the total spin is zero (), which always ends up being a singlet state, a parastate.
We can now write an approximation of the parastates and orthostates. The parastates have singlet spin state and symmetric spatial state:
Orthostates have triplet spin state (a linear combination of them at least) and antisymmetric spatial state:
where is the degeneracy of that spin state. The values are Normalization constants.
In this approximation, symmetric and antisymmetric states have the same energy, which is the eigenvalue of and comes out to be
For parastates and orthostates to not have the same energy we must surrender the approximation and consider the actual interaction between electrons.
> > The error grows larger the smaller $Z$ is and becomes tolerable for large $Z$. For hydrogen ($Z=1$), the error is around 40%, but for carbon ($Z=6$) it's already down to about 10%. In some cases, this quite useful: provided that the [[valence shell]] of an atom (realistically an [[ion]]) is made up of only two electrons, this can be applied with decent results if the atom is large enough. ### Variational model Much better results can be obtained by applying the [[variational method]]. Specifically, we allow the nuclear charge $Z$ to be the variable quantity; it is no longer a constant and we are looking for an *effective* nuclear charge $Z_{e}$. To start, we need a trial function. We'll use\phi(r_{1},r_{2})=\frac{Z_{e}^{3}}{\pi a^{3}}e^{-Z_{e}(r_{1}+r_{2})/a}=\Psi_{1s}^{Z_{e}}(r_{1})\Psi_{1s}^{Z_{e}}(r_{2})
\psi_{1s}^{Z_{e}}(r)=\left( \frac{Z_{e}^{3}}{\pi a^{3}} \right)^{1/2}e^{Z_{e}r/a}
E(\phi)=\frac{\braket{ \phi | H|\phi }}{\braket{ \phi | \phi } } =\braket{ \phi | H | \phi }
since $\braket{ \phi | \phi }=1$. Ignoring the constants, our $H$ isH=\nabla_{1}^{2}+\nabla_{2}^{2}-\left( \frac{Z_{e}}{r_{1}}+ \frac{Z_{e}}{r_{2}}- \frac{1}{r_{12}} \right)
Since $\braket{ \phi | A+B | \phi }=\braket{ \phi | A | \phi }+\braket{ \phi | B | \phi }$, we can calculate these term separately. The "kinetic" terms (the first two) end up being\langle H \rangle {\phi}=2Z^{2}E{1}
\langle H \rangle {\phi}= 2(Z-2) \frac{e^{2}}{4\pi \varepsilon{0}} \left\langle \frac{1}{r_{12}} \right\rangle_{\phi} +\langle V_{ee} \rangle_{\phi}
\braket{ \phi | \frac{1}{r_{12}} | \phi } =\frac{5}{8}Z_{e}
Z_{e}=Z- \frac{5}{16}
As it happens, the effective charge is reduced by a constant. [^1]: For a full derivation, see Bransden & Joachaim § 6.4.