The Skyrme-Hartree-Fock-Bogoliubov method: its application to finite nuclei and neutron-star crusts
N. Chamel, S. Goriely, J.M. Pearson

TL;DR
This paper reviews the Skyrme-Hartree-Fock-Bogoliubov method and demonstrates its application to modeling finite nuclei and neutron-star crusts, highlighting its versatility in nuclear physics.
Contribution
It provides a comprehensive overview of applying the HFB method with Skyrme interactions to diverse nuclear systems, from finite nuclei to neutron-star crusts.
Findings
Effective description of finite nuclei
Application to neutron-star crusts
Versatility of the HFB method
Abstract
After a brief review of the Hartree-Fock-Bogoliubov method with Skyrme effective interactions, we show how it can be applied to the description of various nuclear systems, from finite nuclei to neutron-star crusts.
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Taxonomy
TopicsNuclear physics research studies · Quantum, superfluid, helium dynamics · Quantum Chromodynamics and Particle Interactions
