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Nuclear density functional theory

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Abstract

An understanding of atomic nuclei is crucial for a complete nuclear theory, for the nuclear astrophysics, for performing new experimental tasks, and for various other applications. Within a density functional theory, the total binding energy of the nucleus is given by a functional of the nuclear density matrices and their derivatives. The variation of the energy density functional with respect to particle and pairing densities leads to the Hartree-Fock-Bogoliubov equations. The “Universal Nuclear Energy Density Functional” (UNEDF) SciDAC project to develop and optimize the energy density functional for atomic nuclei using state-of-the-art computational infrastructure, is briefly described. The ultimate goal is to replace current phenomenological models of the nucleus with a well-founded microscopic theory with minimal uncertainties, capable of describing nuclear data and extrapolating to unknown regions.

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Talk at International Bogoliubov Conference, “Problems of Theoretical and Mathematical Physics”, Moscow-Dubna, Russia, August 21–27, 2009.

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Stoitsov, M. Nuclear density functional theory. Phys. Part. Nuclei 41, 868–873 (2010). https://doi.org/10.1134/S1063779610060092

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