Energy–density functional plus quasiparticle–phonon model theory as a powerful tool for nuclear structure and astrophysics


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During the last decade, a theoretical method based on the energy–density functional theory and quasiparticle–phonon model, including up to three-phonon configurations was developed. The main advantages of themethod are that it incorporates a self-consistentmean-field and multi-configuration mixing which are found of crucial importance for systematic investigations of nuclear low-energy excitations, pygmy and giant resonances in an unified way. In particular, the theoretical approach has been proven to be very successful in predictions of new modes of excitations, namely pygmy quadrupole resonance which is also lately experimentally observed. Recently, our microscopically obtained dipole strength functions are implemented in predictions of nucleon-capture reaction rates of astrophysical importance. A comparison to available experimental data is discussed.

作者简介

N. Tsoneva

Frankfurt Institute for Advanced Studies (FIAS); Institut für Theoretische Physik; Institute for Nuclear Research and Nuclear Energy

编辑信件的主要联系方式.
Email: Nadia.Tsoneva@theo.physik.uni-giessen.de
德国, Frankfurt am Main; Gießen; Sofia

H. Lenske

Institut für Theoretische Physik

Email: Nadia.Tsoneva@theo.physik.uni-giessen.de
德国, Gießen

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