An implementation of realistic, finite-temperature nuclear-matter models in neutron-star seismology.
-
Updated
Mar 29, 2026 - 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
Cheat Sheets for many-body perturbation theory up to high orders
The work of mine under the supervision of Dr. Ngo Hai Tan and Prof. Dao Tien Khoa with the neutron star problem.
The vault of references of Megrez Lu in BibLaTeX
Numerical calculation of effective mass within QHD framework
Add a description, image, and links to the nuclear-matter topic page so that developers can more easily learn about it.
To associate your repository with the nuclear-matter topic, visit your repo's landing page and select "manage topics."