An implementation of realistic, finite-temperature nuclear-matter models in neutron-star seismology.
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Updated
Dec 9, 2024 - Julia
An implementation of realistic, finite-temperature nuclear-matter models in neutron-star seismology.
calculate chiral nucleon-nucleon interaction matrix elements under momentum plane-wave basis, as an input for infinite nuclear matter calculations
The vault of references of Megrez Lu in BibLaTeX
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