[Submitted on 19 May 2020]
The thermal conductivity of "pastas" in neutron star matter
Claudio Dorso · Jonathan Dunn · Alejandro Strachan · Guillermo Frank
This investigation explores the phononic thermal conductivity of nuclear star matter as it undergoes the "topological" transition to the "pasta" regime, and further down to the solid-liquid phase transition. The study was carried out using molecular dynamics simulations with nuclear potentials embedded in an effective (i.e. Thomas-Fermi) Coulomb potential. The thermal conductivity experiences a dramatic change within a narrow temperature interval around T=1 MeV. This change accomplishes the "pasta" breakdown during a heating process. The thermal conductivity by flipping protons' or neutrons' velocity further shows a decoupling for asymmetric nuclear star matter.
- Comments:
- 11 pages, 20 figures
- Subjects:
- Nuclear Theory (nucl-th)
- arXiv:
- 2005.09142 [pdf]