The Skyrme-Hartree-Fock-Bogoliubov method: its application to finite nuclei and neutron-star crusts

2010/01/29 by N. Chamel, Chamel, N., S. Goriely +5
Earth and Planetary Sciences · Physics and Astronomy · #FOS: Physical sciences #High-pressure geophysics and materials #Nuclear Theory (nucl-th) #Nuclear physics research studies #Quantum Chromodynamics and Particle Interactions #Quantum, superfluid, helium dynamics #nucl-th

paper · pdf · doi:10.48550/arxiv.1001.5377

7 pages, 1 figure, talk presented at the 28th International Workshop on Nuclear Theory, Rila Mountains, Bulgaria, June 22-27, 2009

arxiv created 2010/01/29 · openalex publication_date 2010/01/29 · arxiv updated 2010/02/26 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

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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