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Configuration Interaction

Also known as: CI, configuration interaction method, CI calculations

OriginatorClemens RoothaanYear1960Sources2Related methods4

Configuration Interaction (CI) is a post-Hartree-Fock quantum chemistry method that improves upon mean-field molecular orbital theory by treating electron correlation through a linear combination of electronic configurations. Introduced by Roothaan in 1960, CI corrects for the fundamental limitation of single-determinant theory by allowing the wavefunction to be a superposition of excited-state Slater determinants, systematically accounting for electron-electron interactions.

Key highlights

  • Systematic improvement: truncation order (S, D, T, ...) directly controls accuracy
  • Excited states: ground and excited state energies and properties from a single calculation
  • Electron correlation: explicitly accounts for electron-electron interaction neglected in HF
  • Size-consistent variants: QCI, EOM-CCSD avoid size-consistency errors of standard CI

Intuition

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How it works

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When to use it

Apply CI to compute excitation energies, ionization potentials, and electron affinities where electron correlation is important. CI is ideal for small to medium molecules (< 20 heavy atoms) and systems where excited-state properties are needed. CIS is fastest (singles only); CISD is more accurate but scales as O(N^6); CISDT and higher become prohibitively expensive.

Strengths & limitations

Strengths
  • Systematic improvement: truncation order (S, D, T, ...) directly controls accuracy
  • Excited states: ground and excited state energies and properties from a single calculation
  • Electron correlation: explicitly accounts for electron-electron interaction neglected in HF
  • Size-consistent variants: QCI, EOM-CCSD avoid size-consistency errors of standard CI
Limitations
  • Computational cost grows rapidly: CIS is O(N^4), CISD is O(N^6), CISDT is O(N^8)
  • Size-consistency problem: standard CI is size-inconsistent (energy per fragment in dissociation incorrect)
  • Slow convergence: many configurations needed for chemical accuracy
  • Integrals storage: four-index electron repulsion integrals dominate storage and compute time

Common pitfalls

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Applications

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Frequently asked

What is the difference between CIS, CISD, CISDT, and full CI?

CIS includes only single excitations (one electron promoted from occupied to virtual orbital); CISD includes singles and doubles (two electrons promoted); CISDT includes up to triples, etc. Full CI includes all possible excitations and is exact (within the basis set). Each step improves accuracy but increases computational cost.

Why is standard CI size-inconsistent?

For two separated fragments A and B, the correct energy is E(AB) = E(A) + E(B). In standard CI, truncation at a fixed excitation level (e.g., CISD) treats the combined system differently than two separate calculations, breaking this additivity. EOM-CCSD and QCI fix this by proper summation.

When should I use CI instead of DFT?

CI is preferred for excited-state properties, systems with significant multi-reference character, and benchmarking calculations. DFT is faster (O(N^4) scaling) and often sufficient for ground-state properties and structure. CI is more accurate but computationally expensive, so use for chemically important systems where accuracy is critical.

Sources

  1. 1.
    Roothaan, C. C. J. (1960). New developments in molecular orbital theory. Reviews of Modern Physics, 32(2), 179-185.
  2. 2.
    Szabo, A., & Ostlund, N. S. (1996). Modern Quantum Chemistry: Introduction to Advanced Electronic Structure Theory. Dover Publications.

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Cite this page

ScholarGate. (2026, June 3). Configuration Interaction. ScholarGate. https://scholargate.app/spectroscopy/configuration-interaction

Configuration Interaction | ScholarGate