A density can organize the ground-state problem
A two-electron wavefunction depends on both electron positions and spins. The density depends on one position and tells us the expected number of electrons per unit volume. It discards much visible detail, so it is surprising that ground-state energy can be formulated in terms of the density.
The Hohenberg–Kohn formulation establishes an exact density variational principle for electrons in an external potential. An exact universal functional exists under the stated ground-state conditions. That result changes how the problem can be organized, but it does not hand us a tractable exact formula for every molecule.
Practical density functional approximations supply specific formulas. Their accuracy must be evaluated as approximations. A failure of PBE on a stretched molecule reveals a limitation of that particular approximation and its chosen solution.
Reading: Sandbox Physics · P. Hohenberg and W. Kohn
Kohn–Sham orbitals separate the difficult energy
Kohn–Sham theory introduces an auxiliary noninteracting system with the desired density. Its orbital kinetic energy is . Add attraction to the nuclei and the classical Coulomb self-energy of the total density. Everything still needed to recover the interacting energy belongs to , the exchange-correlation functional. This includes the difference between interacting and auxiliary kinetic energies.
Minimizing the energy yields self-consistent one-electron equations. They resemble HF equations, but the effective exchange-correlation potential comes from the chosen functional. The orbitals are computational tools for constructing the density. Their energies are not a list of independent interacting-electron energies to be summed into a total.
Reading: Sandbox Physics · W. Kohn and L. J. Sham
Select a functional and preserve its numerical settings
PBE is a generalized-gradient approximation. It uses spin densities and their spatial gradients to approximate exchange-correlation energy. Its published form is fixed; choosing PBE does not mean fitting its parameters to the small hydrogen data shown here.
The saved comparison uses spin-restricted Kohn–Sham PBE in STO-3G, generated with PySCF 2.14.0 and Libxc 7.1.2. The unpruned atomic integration grid has 99 radial points and 590 angular points per shell. The energy-convergence tolerance is one trillionth of a hartree. The repository preserves a denser-grid check and a reproducible input script.
Spin-restricted and spin-unrestricted Kohn–Sham calculations are different searches. Allowing different alpha and beta orbitals can change the dissociation curve, just as extra spin freedom matters in HF. The plotted PBE reference always uses the restricted search, so the spin constraint remains fixed throughout the functional comparison.
Reading: Sandbox Physics · J. P. Perdew · W. Kohn and L. J. Sham
A lower PBE number has a different meaning
At bohr, restricted PBE/STO-3G gives approximately hartree. Same-basis FCI is . The PBE number is lower because the approximate functional energy is not the expectation of the same Hamiltonian in a normalized trial wavefunction. The wavefunction upper-bound argument therefore does not apply.
This example does not rank PBE by proximity to an experimental molecular energy: both the small basis and the approximate functional affect that different question. It compares method behavior at a fixed geometry and basis. To understand why restricted approximate functionals struggle at dissociation, the final chapter examines a sharper condition on a single hydrogen atom with fractional spin.
Reading: Sandbox Physics · J. P. Perdew · A. J. Cohen