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Atomic Orbitals Revisited

An orbital is a one-particle function, usually normalized, whose meaning depends on how it is constructed. State-to-state amplitudes called Dyson orbitals are an important exception to unit normalization. In an exact one-electron atom it can be the complete spatial state. In a many-electron calculation it may instead be a basis function, a variational ingredient in a Slater determinant, an eigenfunction of an auxiliary operator, an eigenvector of a reduced density matrix, or a state-to-state removal amplitude.

Those objects are related, but they are not interchangeable. Much confusion about “seeing,” “occupying,” or assigning energy to an orbital comes from moving a statement valid in one context into another without carrying its assumptions.

Required background. Atomic orbitals supplies hydrogenic functions and angular bases. Change of basis explains representation freedom; Slater determinants constructs the many-electron states used below.

Context Object called an orbital Invariant physical content Main caution
exact one-electron problem eigenstate of the one-particle Hamiltonian ray, density, currents, and matrix elements phase and degenerate-basis choices remain conventional
finite-basis expansion chosen one-particle basis function the spanned subspace after convergence a primitive basis function is not generally an eigenstate
Hartree–Fock optimized spin-orbital in a single determinant occupied projector and determinant occupied rotations preserve the determinant but need not preserve canonical eigenfunctions
Kohn–Sham theory orbital of an auxiliary noninteracting system density for the stated functional and solution most eigenvalues are not exact removal energies
natural-orbital analysis eigenfunction of the one-body density matrix occupation spectrum and eigenspaces degenerate occupations permit rotations
localized or hybrid analysis unitary combination chosen for locality or interpretation the retained orbital subspace localization is method- and criterion-dependent
ionization or attachment Dyson or quasiparticle amplitude state-specific spectral amplitude it is not a permanently occupied one-electron state

Whenever an article, plot, or program prints an “orbital,” first ask which row of this table applies.

For one spinless particle, an orbital may be written as a ket ∣ϕp⟩|\phi_p\rangle or a position-space wavefunction

ϕp(r)=⟨r∣ϕp⟩.\phi_p(\mathbf r)=\langle\mathbf r|\phi_p\rangle.

Including electron spin gives a spin-orbital

χp(x)=χp(r,σ),\chi_p(x)=\chi_p(\mathbf r,\sigma),

where xx abbreviates spatial and spin coordinates. In a collinear spin description it often factorizes as

χp(x)=ϕp(r)ωp(σ),\chi_p(x)=\phi_p(\mathbf r)\omega_p(\sigma),

with ωp\omega_p an α\alpha or β\beta spin function. Relativistic or noncollinear calculations use multicomponent spinors for which this product form need not hold.

Normalization means

⟨χp∣χp⟩=∑σ∫∣χp(r,σ)∣2 d3r=1.\langle\chi_p|\chi_p\rangle =\sum_\sigma\int |\chi_p(\mathbf r,\sigma)|^2\,d^3r=1.

An orthonormal set is convenient,

⟨χp∣χq⟩=δpq,\langle\chi_p|\chi_q\rangle=\delta_{pq},

but nonorthogonal atomic and molecular basis functions are also legitimate. They require an overlap matrix and a generalized eigenvalue problem; orthogonality is not part of the dictionary definition of an orbital.

For ideal hydrogen or a hydrogenic ion, the electron has no electronic partner with which to be entangled. A stationary orbital is then an exact eigenstate of the internal one-electron Hamiltonian, apart from the stated recoil, relativistic, radiative, and nuclear idealizations. Its energy is an eigenvalue of that Hamiltonian and its position probability density follows directly from the orbital.

This special case is conceptually clean but not generic. Once electron–electron interaction is present, the complete electronic state lives in an antisymmetric many-particle Hilbert space.

For NN electrons, the coordinate wavefunction is

Ψ(x1,x2,…,xN),\Psi(x_1,x_2,\ldots,x_N),

antisymmetric under exchange of any two arguments. In general it cannot be assigned as a list in which “electron 1 occupies orbital aa” and “electron 2 occupies orbital bb.” The electron labels are argument slots, not persistent particle identities.

A chosen spin-orbital set generates Slater determinants ∣ΦI⟩|\Phi_I\rangle. A correlated state can be expanded as

∣Ψ⟩=∑ICI∣ΦI⟩.|\Psi\rangle=\sum_I C_I|\Phi_I\rangle.

The coefficients and orbitals jointly represent the state. Changing the one-particle basis changes the determinant expansion, even when the many-electron vector represented by the full expansion does not change. Slater Determinants develops this antisymmetric basis.

Saying that a determinant “occupies orbitals i,j,ki,j,k” means that those spin-orbitals define its occupied antisymmetric subspace. It does not attach a named electron to each function. In a superposition of determinants, even the occupation of a chosen orbital can be noninteger as an expectation value.

Occupation language remains useful when the reference determinant dominates or when an occupation-number basis has been explicitly chosen. It becomes misleading if it is promoted into a hidden classical assignment.

Electron Configurations develops the atomic subshell notation, Aufbau heuristic, core–valence partitions, and basis dependence of configuration weights built from these orbitals.

For an exact one-electron spatial state,

ρ(r)=∣ϕ(r)∣2\rho(\mathbf r)=|\phi(\mathbf r)|^2

is the position probability density. For a spin-orbital, sum over spin components. An isosurface drawn at ∣ϕ∣2=c|\phi|^2=c or ∣ϕ∣=c|\phi|=c is a visualization choice, not a wall, trajectory, or boundary of the atom.

For a determinant of orthonormal occupied spin-orbitals, the spin-resolved one-particle density is a sum,

ρ(x)=∑i∈occ∣χi(x)∣2.\rho(x)=\sum_{i\in\mathrm{occ}}|\chi_i(x)|^2.

The spatial electron density is obtained by summing over spin. Individual orbitals may have nodal planes while the total density remains nonzero there because other occupied orbitals contribute. It is therefore wrong to infer a node of the atom or molecule from a node in one chosen orbital.

Write X=(x2,…,xN)X=(x_2,\ldots,x_N) and dX=dx2⋯dxNdX=dx_2\cdots dx_N. The one-body reduced density matrix is

γ(x,x′)=N∫dX Ψ(x,X)Ψ∗(x′,X).\gamma(x,x') =N\int dX\, \Psi(x,X)\Psi^*(x',X).

Its diagonal gives the one-particle density,

ρ(x)=γ(x,x),∫ρ(x) dx=N.\rho(x)=\gamma(x,x), \qquad \int \rho(x)\,dx=N.

This density is basis-independent. Decomposing it into orbital contributions is not unique unless an additional prescription, such as natural-orbital diagonalization, is stated.

Suppose a subspace S\mathcal S has orthonormal basis {∣ϕp⟩}\{|\phi_p\rangle\}. Any unitary matrix UU defines another orthonormal basis,

∣ϕ~a⟩=∑p∣ϕp⟩Upa,U†U=I.|\widetilde\phi_a\rangle =\sum_p|\phi_p\rangle U_{pa}, \qquad U^\dagger U=I.

Real px,py,pzp_x,p_y,p_z functions and complex Y1mY_1^m functions are familiar examples of different bases for the same angular-momentum subspace. Real orbitals display nodal planes conveniently; complex spherical harmonics diagonalize LzL_z.

Same subspace does not mean same individual state

Section titled “Same subspace does not mean same individual state”

A basis rotation preserves the subspace but generally changes each basis vector. If one electron is deliberately prepared in pxp_x rather than pyp_y, those are different states and can produce different directional probabilities. The convention enters when no physical preparation, perturbation, or measurement distinguishes one basis within a degenerate subspace.

If two orbitals have different nondegenerate eigenvalues, their arbitrary linear combinations still span the same two-dimensional space but are not stationary eigenstates. “Any rotation is equivalent” is therefore a statement about a representation or occupied subspace, not a license to erase dynamics.

In the absence of a vector potential, a one-particle wavefunction has probability current

j=ℏmeIm⁡(ϕ∗∇ϕ).\mathbf j =\frac{\hbar}{m_e} \operatorname{Im}(\phi^*\nabla\phi).

A real stationary orbital has zero current under this formula, while a complex LzL_z eigenstate can carry azimuthal current. Two basis choices can describe the same degenerate subspace, but selecting one complex state rather than a real superposition can change current-related observables. The canonical continuity-equation treatment is Probability Current.

Hybrid orbitals are linear combinations chosen to point along useful directions. Starting from orthonormal functions s,px,py,pzs,p_x,p_y,p_z, one tetrahedral convention is

2h1=s+px+py+pz,2h2=s+px−py−pz,2h3=s−px+py−pz,2h4=s−px−py+pz.\begin{aligned} 2h_1&=s+p_x+p_y+p_z,\\ 2h_2&=s+p_x-p_y-p_z,\\ 2h_3&=s-p_x+p_y-p_z,\\ 2h_4&=s-p_x-p_y+p_z. \end{aligned}

The four hih_i are orthonormal and span exactly the same four-dimensional space as the original ss and pp set. This is the mathematical content of idealized sp3sp^3 hybridization.

What hybridization does and does not claim

Section titled “What hybridization does and does not claim”

In an isolated atom, ss and pp orbitals usually have different energies, so a hybrid is not a stationary eigenstate of the spherical atomic Hamiltonian. In a molecular environment, directional combinations may be useful for constructing a basis or interpreting a self-consistent occupied subspace.

Hybridization is therefore a representation adapted to geometry and bonding, not a literal time sequence in which an atom first promotes and mechanically mixes orbitals before a bond can form. Different localization schemes can produce different hybrids while preserving the same total wavefunction, density, or occupied projector. Valence Bond Theory shows how such directional bases enter localized, spin-coupled molecular structures.

Hartree–Fock optimizes a single Slater determinant. Its canonical spin-orbitals satisfy a self-consistent equation

f[P]∣ϕp⟩=ϵp∣ϕp⟩,f[P]|\phi_p\rangle =\epsilon_p|\phi_p\rangle,

where the Fock operator depends on the occupied projector PP. For NN occupied spin-orbitals,

P=∑i=1N∣ϕi⟩⟨ϕi∣.P=\sum_{i=1}^{N} |\phi_i\rangle\langle\phi_i|.

A unitary rotation among occupied orbitals leaves PP unchanged. The determinant changes only by the overall phase det⁡U\det U, so its density and energy are unchanged. Canonical and localized occupied orbitals can therefore represent the same Hartree–Fock state. An arbitrary occupied rotation generally makes the Fock matrix nondiagonal; it preserves canonical eigenfunctions only inside equal-eigenvalue subspaces.

Canonical virtual orbitals are even less intrinsic: they complete a convenient eigenbasis of the converged Fock operator but are not occupied particles. The full variational derivation, exchange operator, occupied-subspace invariance, and stability tests belong to Hartree–Fock Approximation; the radial, asymptotic, and open-shell atomic interpretation belongs to Hartree–Fock for Atoms.

Kohn–Sham density-functional theory constructs an auxiliary noninteracting system whose ground-state density matches the interacting density for the exact functional. Its orbitals solve one-particle equations and are indispensable computational objects, but the auxiliary determinant is not generally the exact interacting wavefunction.

For an isolated bound ground state and an exact local Kohn–Sham potential tending to zero at infinity, the ionization theorem gives ϵHOMO=−I\epsilon_{\mathrm{HOMO}}=-I, with I=E(N−1)−E(N)I=E(N-1)-E(N). The potential zero matters because adding a constant shifts every orbital eigenvalue. This does not turn every occupied and virtual eigenvalue of an approximate functional into an exact photoelectron or excitation energy. Functional error, derivative discontinuities, symmetry breaking, and the chosen generalized Kohn–Sham framework matter.

Natural spin-orbitals diagonalize the one-body reduced density matrix:

∫γ(x,x′)φk(x′) dx′=nkφk(x).\int \gamma(x,x')\varphi_k(x')\,dx' =n_k\varphi_k(x).

The eigenvalues nkn_k are natural occupation numbers. With a spin-orbital convention,

0≤nk≤1,∑knk=N.0\le n_k\le1, \qquad \sum_k n_k=N.

A single determinant has NN occupations equal to one and the rest zero. A correlated pure state generally has fractional occupations. An ensemble mixture, including a thermal state of noninteracting electrons, can also have fractional occupations; fractionality alone therefore does not establish interaction-induced correlation. In a spin-summed spatial-orbital convention, the upper bound is two instead; the convention must be stated.

Natural occupations are basis-independent eigenvalues of γ\gamma. Natural orbitals are unique up to phase only when their occupations are nondegenerate. Within a degenerate occupation subspace, unitary rotations remain allowed.

Localized orbitals are usually obtained by rotating an occupied or selected active subspace to optimize a criterion: spatial spread, atomic charge separation, bond localization, or another functional. Boys, Pipek–Mezey, intrinsic, and Wannier constructions do not generally produce the same orbitals.

Localization can make chemical structure and embedding approximations easier to interpret. It does not create a new many-electron state when the transformation is unitary within a complete occupied subspace. Report the localization criterion and the subspace to which it was applied.

For ionization from an NN-electron state ΨN\Psi_N to a specified (N−1)(N-1)-electron state ΨN−1(a)\Psi_{N-1}^{(a)}, the Dyson orbital is the overlap amplitude

Ia(x)=∫dX ΨN−1(a)∗(X)ΨN(x,X),ϕD(a)(x)=N Ia(x).\begin{aligned} \mathcal I_a(x) &=\int dX\, \Psi_{N-1}^{(a)*}(X)\Psi_N(x,X),\\ \phi_D^{(a)}(x) &=\sqrt N\,\mathcal I_a(x). \end{aligned}

It connects two many-electron eigenstates and enters approximations to photoionization and electron-removal amplitudes. It need not coincide with a Hartree–Fock, Kohn–Sham, or natural orbital. Its norm measures state-specific one-electron character under the adopted normalization; correlation can distribute removal strength among many ionic channels.

Calling a reconstructed photoelectron amplitude “the orbital that the electron occupied” discards this state-to-state meaning.

Photoelectron Spectroscopy develops the measurement-level consequences: binding-energy conventions, Koopmans-style assignments, pole strengths, satellites, and continuum angular distributions.

An orbital does not carry an energy unless the method supplies an operator or convention that assigns one.

Orbital type Meaning of a quoted energy
exact one-electron eigenstate eigenvalue of the stated one-electron Hamiltonian
central-field model orbital eigenvalue of the chosen effective potential; model-dependent
canonical Hartree–Fock orbital eigenvalue of the Fock Lagrange-multiplier operator
Kohn–Sham orbital eigenvalue of an auxiliary density-reproducing system
natural orbital no intrinsic energy follows from diagonalizing γ\gamma
localized or hybrid orbital any assigned energy requires an additional localization or block-partition convention
Dyson orbital paired with a many-body removal energy, not its own eigenvalue in general

Koopmans’ frozen-orbital relation makes −ϵiHF-\epsilon_i^{\mathrm{HF}} an approximation to an ionization energy. Relaxation, correlation, state reorganization, and relativistic effects break a literal identification. Virtual Hartree–Fock energies are still less direct estimates of electron addition or neutral excitation.

An orbital picture becomes physically interpretable by stating the generating method, chosen subspace, and plotted quantity. A density or photoelectron measurement constrains that model through a forward calculation. It does not select a unique orbital basis independently of the model. Pair correlations also contain information that a one-body density cannot recover.

Let {∣ϕi⟩}i=1N\{|\phi_i\rangle\}_{i=1}^{N} be orthonormal occupied orbitals and define

∣ϕ~a⟩=∑i=1N∣ϕi⟩Uia,|\widetilde\phi_a\rangle =\sum_{i=1}^{N}|\phi_i\rangle U_{ia},

where UU is unitary. Show that the occupied projector is unchanged.

Solution

The rotated projector is

P~=∑a∣ϕ~a⟩⟨ϕ~a∣=∑aij∣ϕi⟩UiaUja∗⟨ϕj∣.\begin{aligned} \widetilde P &=\sum_a|\widetilde\phi_a\rangle \langle\widetilde\phi_a|\\ &=\sum_{aij}|\phi_i\rangle U_{ia}U_{ja}^*\langle\phi_j|. \end{aligned}

Unitarity gives

∑aUiaUja∗=δij,\sum_aU_{ia}U_{ja}^*=\delta_{ij},

so

P~=∑i∣ϕi⟩⟨ϕi∣=P.\widetilde P =\sum_i|\phi_i\rangle\langle\phi_i|=P.

Any determinant built from the complete occupied set changes only by the phase det⁡U\det U. Observables depending on the determinant or occupied projector are therefore unchanged, although plots of the individual rotated orbitals may look very different.

Assume s,px,py,pzs,p_x,p_y,p_z are orthonormal. Verify that the four hih_i defined in the hybrid-orbital section are normalized and mutually orthogonal. What has changed physically when this basis is adopted?

Solution

Each hybrid has four coefficients of magnitude 1/21/2, so

⟨hi∣hi⟩=4(12)2=1.\langle h_i|h_i\rangle =4\left(\frac12\right)^2=1.

For example,

⟨h1∣h2⟩=14(1+1−1−1)=0.\langle h_1|h_2\rangle =\frac14(1+1-1-1)=0.

Every other distinct pair has two matching and two opposite signs, so its inner product also vanishes. The coefficient matrix is a normalized Hadamard matrix and is unitary.

The one-particle subspace has not changed. Only its basis has been rotated. If a complete occupied or active-space treatment is transformed consistently, invariant observables are unchanged. The directional hybrids can still be more convenient for interpretation or approximation.

Use the spectral representation of the one-body density matrix to show that its natural occupations sum to NN. Then explain why a single determinant has only occupations zero or one in a spin-orbital convention.

Solution

The spectral representation is

γ=∑knk∣φk⟩⟨φk∣.\gamma =\sum_k n_k|\varphi_k\rangle \langle\varphi_k|.

Taking the trace gives

Tr⁡γ=∑knk=N,\operatorname{Tr}\gamma =\sum_k n_k=N,

because the diagonal density integrates to the electron number.

For a determinant, γ\gamma is the occupied projector PP. Projectors are idempotent:

P2=P.P^2=P.

Applying this equation to an eigenvector gives nk2=nkn_k^2=n_k, whose only real solutions are nk=0n_k=0 and nk=1n_k=1. Fractional natural occupations therefore exclude a single pure spin-orbital determinant. They do not distinguish a correlated pure state from an ensemble mixture; purity, spin convention, and numerical accuracy must also be specified.

Let

ϕ(r,θ,φ)=f(r,θ)eimφ,\phi(r,\theta,\varphi) =f(r,\theta)e^{im\varphi},

where ff is real. Derive its azimuthal probability current. Compare it with a real linear combination proportional to fcos⁡(mφ)f\cos(m\varphi).

Solution

Only the phase gradient contributes to the imaginary part:

∇(mφ)=mrsin⁡θ eφ.\nabla(m\varphi) =\frac{m}{r\sin\theta}\,\mathbf e_\varphi.

Therefore

j=ℏmmersin⁡θ∣ϕ∣2eφ.\mathbf j =\frac{\hbar m}{m_e r\sin\theta} |\phi|^2\mathbf e_\varphi.

The real function fcos⁡(mφ)f\cos(m\varphi) has zero probability current wherever the wavefunction is smooth because ϕ∗∇ϕ\phi^*\nabla\phi is real. It is a superposition of opposite mm components rather than an LzL_z eigenstate with eigenvalue mℏm\hbar. The complex and real bases span the same m,−mm,-m subspace, but preparing one particular vector can change current and angular-momentum observables.

Two orthonormal occupied spatial orbitals are rotated according to

ϕ~1=cos⁡α ϕ1+sin⁡α ϕ2,ϕ~2=−sin⁡α ϕ1+cos⁡α ϕ2.\begin{aligned} \widetilde\phi_1 &=\cos\alpha\,\phi_1+\sin\alpha\,\phi_2,\\ \widetilde\phi_2 &=-\sin\alpha\,\phi_1+\cos\alpha\,\phi_2. \end{aligned}

Show pointwise that their summed density is invariant. What does this imply about interpreting a node in one localized or canonical orbital?

Solution

Expanding both squared magnitudes gives

∣ϕ~1∣2=cos⁡2α∣ϕ1∣2+sin⁡2α∣ϕ2∣2+2sin⁡αcos⁡αRe⁡(ϕ1∗ϕ2),∣ϕ~2∣2=sin⁡2α∣ϕ1∣2+cos⁡2α∣ϕ2∣2−2sin⁡αcos⁡αRe⁡(ϕ1∗ϕ2).\begin{aligned} |\widetilde\phi_1|^2 &=\cos^2\alpha|\phi_1|^2 +\sin^2\alpha|\phi_2|^2 +2\sin\alpha\cos\alpha \operatorname{Re}(\phi_1^*\phi_2), \\ |\widetilde\phi_2|^2 &=\sin^2\alpha|\phi_1|^2 +\cos^2\alpha|\phi_2|^2 -2\sin\alpha\cos\alpha \operatorname{Re}(\phi_1^*\phi_2). \end{aligned}

Adding cancels the cross terms and uses sin⁡2α+cos⁡2α=1\sin^2\alpha+\cos^2\alpha=1:

∣ϕ~1∣2+∣ϕ~2∣2=∣ϕ1∣2+∣ϕ2∣2.|\widetilde\phi_1|^2+|\widetilde\phi_2|^2 =|\phi_1|^2+|\phi_2|^2.

Individual nodal surfaces can move under the rotation while the occupied-space density stays fixed. A node in one plotted orbital is therefore not automatically a node in the total electron density or a basis-independent boundary.

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