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Quasipinning and Extended Hartree-Fock Method based on Generalized Pauli Constraints

Series
Oxford Physics Academic Lectures
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It is now known that fermionic natural occupation numbers (NON) do not only obey Pauli’s exclusion principle but are even stronger restricted by the so-called generalized Pauli constraints (GPC).
So far, the nature of these constraints has been explored in some systems: a model of few spinless fermions confined to a one-dimensional harmonic potential, the lithium isoelectronic series and ground and excited states of some three-, four- and five-electron atomic and molecular systems. Whenever given NON lie on the boundary of the allowed region the corresponding N-fermion quantum state has a significantly simpler structure. By employing this structure a variational optimization method for few fermion ground states is elaborated. We quantitatively confirm its high accuracy for systems with the vector of NON in a small distance to the boundary of the polytope. In particular, we derive an upper bound on the error of the correlation energy given by the ratio of the distance to the boundary of the polytope and the distance of the vector of NON to the Hartree-Fock point. Moreover, these geometric insights shed some light on the concept of active spaces, correlation energy, frozen electrons and virtual orbitals.

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The Pauli exclusion principle has a strong impact on the properties and the behavior of most fermionic quantum systems. Remarkably, even stronger restrictions on fermionic natural occupation numbers follow from the fermionic exchange symmetry.
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Generalized Pauli Constraints in Reduced Density Matrix Functional Theory

Reduced Density Matrix Functional Theory is a method that relies on the 1-1 correspondence between the ground state wavefunction of many electron systems and the first order reduced density matrix(1RDM) and uses the second one as its fundamental valuable.
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Episode Information

Series
Oxford Physics Academic Lectures
People
Carlos Benavides-Riveros
Keywords
electrons
fermionic
numbers
Department: Department of Physics
Date Added: 11/10/2016
Duration: 00:52:02

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