An implementation of realistic, finite-temperature nuclear-matter models in neutron-star seismology.
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Updated
Apr 17, 2025 - Julia
An implementation of realistic, finite-temperature nuclear-matter models in neutron-star seismology.
Applying Bayesian Model Mixing to the dense matter equation of state (EOS) in beta-equilibrated asymmetric nuclear matter. The work supported by this repository can be found at: https://arxiv.org/abs/2505.18921.
Repository containing the work done in arXiv:2404.06323, where we apply Bayesian model mixing (BMM) to the isospin-symmetric dense matter equation of state (EOS).
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
Numerical calculation of effective mass within QHD framework
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