Two-electron atom


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

H^=22mr12Ze24πε0r1Electron 122mr22Ze24πε0r2Electron 2+e24πε0r12ee interaction\hat{H}=\underbrace{ - \frac{\hbar^{2}}{2m}\nabla ^{2}_{r_{1}}- \frac{Ze^{2}}{4\pi \varepsilon_{0}r_{1}} }_{ \text{Electron 1} }\underbrace{ - \frac{\hbar^{2}}{2m}\nabla ^{2}_{r_{2}}- \frac{Ze^{2}}{4\pi \varepsilon_{0}r_{2}} }_{ \text{Electron 2} }+ \underbrace{ \frac{e^{2}}{4\pi \varepsilon_{0}r_{12}} }_{ e-e\text{ interaction} }

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Spin states

The solved eigenfunction (in position representation) will be of the form ΨΨ(q1,q2)\Psi\equiv \Psi(q_{1},q_{2}), where q1q_{1} and q2q_{2} are the generalized coordinates of the electrons (containing both position and spin state). Electrons are Spin 1/21/2 fermions and so Ψ\Psi must be an antisymmetric state: Ψ(q1,q2)=Ψ(q2,q1)\Psi(q_{1},q_{2})=-\Psi(q_{2},q_{1}). Since H^\hat{H} does not directly depend on spin, we can factor out the spin and leave a coordinate-only and spin-only wavefunction:

Ψ(q1,q2)=ψ(r1,r2)χ(1,2)\Psi(q_{1},q_{2})=\psi (\mathbf{r}_{1},\mathbf{r}_{2})\chi(1,2)

The spin wavefunction χ(1,2)\chi(1,2) can be constructed from the individual spin wavefunctions χ1/2,mS(1)\chi_{1/2,m_{S}}(1) and χ1/2,mS(2)\chi_{1/2,m_{S}}(2). We denote S1\mathbf{S}_{1} and S2\mathbf{S}_{2} the spin operators of the electrons and by (S1)z(S_{1})_{z} and (S2)z(S_{2})_{z} their zz components. Each spin state is described by an eigenfunction, but since we are working with spin 1/21/2, there's only two possible functions per electron, one for spin up and one for spin down. We'll call these α\alpha and β\beta respectively and denote which electron they refer to with a number. S1\mathbf{S}_{1} only acts on α(1)\alpha(1) and β(1)\beta(1), whereas S2\mathbf{S}_{2} only acts on α(2)\alpha(2) and β(2)\beta(2). In turn, this means that S1\mathbf{S}_{1} and S2\mathbf{S}_{2} commute.

The total spin is S=S1+S2\mathbf{S}=\mathbf{S}_{1}+\mathbf{S}_{2} and the total zz component is Sz=(S1)z+(S2)zS_{z}=(S_{1})_{z}+(S_{2})_{z}. The square of the total is

S2=S12+S22+2S1S2=32+2S1S2\mathbf{S}^{2}=\mathbf{S}_{1}^{2}+\mathbf{S}_{2}^{2}+2\mathbf{S}_{1}\cdot \mathbf{S}_{2}=\frac{3}{2}+2\mathbf{S}_{1}\cdot \mathbf{S}_{2}

since S12=S22=3/4\mathbf{S}_{1}^{2}=\mathbf{S}_{2}^{2}=3/4. Since the interaction between electrons is purely electromagnetic, it is independent of spin. As such, each electron's spin is simply either up ()(\uparrow) or down ()(\downarrow) without reference to the other, which leads to four distinct spin states:

χ1(1,2)=α(1)α(2)χ2(1,2)=α(1)β(2)χ3(1,2)=β(1)α(2)χ4(1,2)=β(1)β(2)\begin{align} \chi_{1}(1,2)&=\alpha(1)\alpha(2)&\uparrow\uparrow \\ \chi_{2}(1,2)&=\alpha(1)\beta(2)&\uparrow\downarrow \\ \chi_{3}(1,2)&=\beta(1)\alpha(2)&\downarrow\uparrow \\ \chi_{4}(1,2)&=\beta(1)\beta(2)&\downarrow\downarrow \end{align}

Applying the zz spin operator to χ1\chi_{1} leads to

Szχ1(1,2)=[(S1)z+(S2)z]α(1)α(2)=[(S1)zα(1)]α(2)+α(1)[(S2)zα(2)]=12α(1)α(2)+12α(1)α(2)=α(1)α(2)=χ1(1,2)\begin{align} S_{z}\chi_{1}(1,2)&=[(S_{1})_{z}+(S_{2})_{z}]\alpha(1)\alpha(2) \\ &=[(S_{1})_{z}\alpha(1)]\alpha(2)+\alpha(1)[(S_{2})_{z}\alpha(2)] \\ &=\frac{1}{2}\alpha(1)\alpha(2)+ \frac{1}{2}\alpha(1)\alpha(2) \\ &=\alpha(1)\alpha(2) \\ &=\chi_{1}(1,2) \end{align}

Clearly, the total spin over zz in the χ1\chi_{1} spin state is 11 (in \hbar units). More generally, we have

Szχ=mSχS_{z}\chi=m_{S}\chi

By doing the math for all four χi\chi_{i} functions, we find that mS=1,0,0,1m_{S}=1,0,0,-1, in that order. There's evidently some degeneracy on mS=0m_{S}=0. Moreover, while χ1\chi_{1} and χ4\chi_{4} are symmetric under label exchange, χ2\chi_{2} and χ3\chi_{3} are not, and are also not antisymmetric. As such, the actual mS=0m_{S}=0 states must be normalized linear combinations of the two that are (anti)symmetric under label exchange:

χ±=12[α(1)β(2)±α(2)β(1)]\chi_{\pm}=\frac{1}{\sqrt{ 2 }}[\alpha(1)\beta(2)\pm\alpha(2)\beta(1)]

The ++ is symmetric, the - is antisymmetric. These two functions are eigenstates of S2\mathbf{S}^{2} and SzS_{z}, with eigenvalues Sz=1S_{z}=1 and mS=0m_{S}=0 for ++ and Sz=0S_{z}=0 and mS=0m_{S}=0 for -. We now have four spin states, divided in one state with Sz=0S_{z}=0 and three states with Sz=1S_{z}=1. The former is called the singlet state

χ0,0=12[α(1)β(2)α(2)β(1)]\chi_{0,0}=\frac{1}{\sqrt{ 2 }}[\alpha(1)\beta(2)-\alpha(2)\beta(1)]

and is antisymmetric. The latter three are known as the triplet states

χ1,1=α(1)α(2)χ1,0=12[α(1)β(2)+α(2)β(1)]χ1,1=β(1)β(2)\begin{align} \chi_{1,1}&=\alpha(1)\alpha(2) \\ \chi_{1,0}&=\frac{1}{\sqrt{ 2 }}[\alpha(1)\beta(2)+\alpha(2)\beta(1)] \\ \chi_{1,-1}&=\beta(1)\beta(2) \end{align}

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

H=H0+HH=H_{0}+H'

where the electron-electron interaction

H=e24πε0r12H'=\frac{e^{2}}{4\pi \varepsilon_{0}r_{12}}

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

ψ0(r1,r2)=ψn1,l1,m1(r1)ψn2,l2,m2(r2)\psi_{0}(\mathbf{r}_{1},\mathbf{r}_{2})=\psi_{n_{1},l_{1},m_{1}}(\mathbf{r}_{1})\psi_{n_{2},l_{2},m_{2}}(\mathbf{r}_{2})

where mmlm\equiv m_{l} for clearer notation.

H0H_{0} 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:

ψ±0(r1,r2)=12[ψn1,l1,m1(r1)ψn2,l2,m2(r2)±ψn1,l1,m1(r2)ψn2,l2,m2(r1)]\psi^{0}_{\pm}(\mathbf{r}_{1},\mathbf{r}_{2})=\frac{1}{\sqrt{ 2 }}[\psi_{n_{1},l_{1},m_{1}}(\mathbf{r}_{1})\psi_{n_{2},l_{2},m_{2}}(\mathbf{r}_{2})\pm \psi_{n_{1},l_{1},m_{1}}(\mathbf{r}_{2})\psi_{n_{2},l_{2},m_{2}}(\mathbf{r}_{1})]

As before, ++ is symmetric, - is antisymmetric. A note: if n1,l1,m1=n2,l2,m2n_{1},l_{1},m_{1}=n_{2},l_{2},m_{2}, 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 (Sz=0S_{z}=0), 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:

Ψpara(q1,q2)=A+ψ+0(r1,r2)χ0,0(1,2)\Psi _\text{para}(q_{1},q_{2})=A_{+}\psi_{+}^{0}(\mathbf{r}_{1},\mathbf{r}_{2})\chi_{0,0}(1,2)

Orthostates have triplet spin state (a linear combination of them at least) and antisymmetric spatial state:

Ψortho(q1,q2)=Aψ0(r1,r2)mSχ1,mS(1,2)dmS\Psi _\text{ortho}(q_{1},q_{2})=A_{-}\psi_{-}^{0}(\mathbf{r}_{1},\mathbf{r}_{2})\sum_{m_{S}}\chi_{1,m_{S}}(1,2)d_{m_{S}}

where dmSd_{m_{S}} is the degeneracy of that spin state. The A±A_{\pm} values are Normalization constants.

In this approximation, symmetric and antisymmetric states have the same energy, which is the eigenvalue of H0Ψ±0(r1,r2)=En1,n20Ψ±0(r1,r2)H_{0}\Psi^{0}_{\pm}(\mathbf{r}_{1},\mathbf{r}_{2})=E^{0}_{n_{1},n_{2}}\Psi^{0}_{\pm}(\mathbf{r}_{1},\mathbf{r}_{2}) and comes out to be

En1,n2=mZ222e4(4πϵ0)2(1n12+1n22)\boxed{E_{n_1, n_2} = - \frac{mZ^{2}}{2\hbar^{2}} \frac{ e^{4} }{(4 \pi \epsilon_{0})^{2}} \left( \frac{1}{n_{1}^{2}} + \frac{1}{n_{2}^{2}} \right)}

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})

wherewhere

\psi_{1s}^{Z_{e}}(r)=\left( \frac{Z_{e}^{3}}{\pi a^{3}} \right)^{1/2}e^{Z_{e}r/a}

WeneedtoevaluateWe need to evaluate

E(\phi)=\frac{\braket{ \phi | H|\phi }}{\braket{ \phi | \phi } } =\braket{ \phi | H | \phi }

since $\braket{ \phi | \phi }=1$. Ignoring the constants, our $H$ is

H=\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}

ThelatterthreebecomesThe latter three becomes

\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}

ThedistanceaverageisThe distance average is

\braket{ \phi | \frac{1}{r_{12}} | \phi } =\frac{5}{8}Z_{e}

???Puttingitalltogetherweget??? Putting it all together we get

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.