Hubbard- corrected Hamiltonians for non-self-consistent random-phase approximation total-energy calculations: A study of ZnS, TiO, and NiO
arXiv:1601.07331 · doi:10.1103/PhysRevB.93.035133
Abstract
In non-self-consistent calculations of the total energy within the random-phase approximation (RPA) for electronic correlation, it is necessary to choose a single-particle Hamiltonian whose solutions are used to construct the electronic density and non-interacting response function. Here we investigate the effect of including a Hubbard- term in this single-particle Hamiltonian, to better describe the on-site correlation of 3 electrons in the transition metal compounds ZnS, TiO and NiO. We find that the RPA lattice constants are essentially independent of , despite large changes in the underlying electronic structure. We further demonstrate that the non-self-consistent RPA total energies of these materials have minima at nonzero . Our RPA calculations find the rutile phase of TiO to be more stable than anatase independent of , a result which is consistent with experiments and qualitatively different to that found from calculations employing -corrected (semi)local functionals. However we also find that the + term cannot be used to correct the RPA's poor description of the heat of formation of NiO.
31 pages, 10 figures
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- Assessing the performance of the Random Phase Approximation for exchange and superexchange coupling constants in magnetic crystalline solids
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