Full configuration interaction

Full configuration interaction[1] (or full CI) is a linear variational approach which provides numerically exact solutions (within the infinitely flexible complete basis set) to the electronic time-independent, non-relativistic Schrödinger equation.[2]

Explanation

It is a special case of the configuration interaction method in which all Slater determinants (or configuration state functions, CSFs) of the proper symmetry are included in the variational procedure (i.e., all Slater determinants obtained by exciting all possible electrons to all possible virtual orbitals, orbitals which are unoccupied in the electronic ground state configuration). This method is equivalent to computing the eigenvalues of the electronic molecular Hamiltonian within the basis set of the above-mentioned configuration state functions.

In a minimal basis set a full CI computation is very easy. But in larger basis sets this is usually just a limiting case which is not often attained. This is because exact solution of the full CI determinant is NP-complete, so the existence of a polynomial time algorithm is unlikely. The Davidson correction is a simple correction which allows one to estimate the value of the full CI energy from a limited configuration interaction expansion result.

Because the number of determinants required in the full CI expansion grows factorially with the number of electrons and orbitals, full CI is only possible for atoms or very small molecules with about a dozen or fewer electrons. Full CI problems including several million up to a few billion determinants are possible using current algorithms. Because full CI results are exact within the space spanned by the orbital basis set, they are invaluable in benchmarking approximate quantum chemical methods.[3] This is particularly important in cases such as bond-breaking reactions, diradicals, and first-row transition metals, where electronic near-degeneracies can invalidate the approximations inherent in many standard methods such as Hartree–Fock theory, multireference configuration interaction, finite-order Møller–Plesset perturbation theory, and coupled cluster theory.

Although fewer N-electron functions are required if one employs a basis of spin-adapted functions (Ŝ2 eigenfunctions), the most efficient full CI programs employ a Slater determinant basis because this allows for the very rapid evaluation of coupling coefficients using string-based techniques advanced by Nicholas C. Handy in 1980. In the 1980s and 1990s, full CI programs were adapted to provide arbitrary-order Møller–Plesset perturbation theory wave functions, and in the 2000s they have been adapted to provide coupled cluster wave functions to arbitrary orders, greatly simplifying the task of programming these complex methods.

gollark: Indeed.
gollark: I'm probably going to rewrite Wyvern yet again to communicate with a non-CC server to simplify item handling and make setup even more annoying.
gollark: The madman behind it (@Incin or something) made a HTML/CSS parser/renderer or something and made the shop use it.
gollark: I prefer Xenon. It's more flexible though configuration is harder.
gollark: You should not work on a shop if you need someone to explain the docs to you and write the code for you.

References
  1. Ross, I. G. (1952). "Calculations of the energy levels of acetylene by the method of antisymmetric molecular orbitals, including σ-π interaction". Transactions of the Faraday Society. 48. The Royal Society of Chemistry. pp. 973–991. doi:10.1039/TF9524800973.
  2. Foresman, James B.; Æleen Frisch (1996). Exploring Chemistry with Electronic Structure Methods (2nd ed.). Pittsburgh, PA: Gaussian Inc. pp. 266, 278–283. ISBN 0-9636769-3-8.
  3. Szabo, Attila; Neil S. Ostlund (1996). Modern Quantum Chemistry. Mineola, New York: Dover Publications, Inc. pp. 350–353. ISBN 0-486-69186-1.
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