English

Three-dimensional calculation of inhomogeneous structure in low-density nuclear matter

Nuclear Theory 2015-03-19 v1 Solar and Stellar Astrophysics

Abstract

In low-density nuclear matter which is relevant to the crust region of neutron stars and collapsing stage of supernovae, non-uniform structures called "nuclear pasta" are expected. So far, most works on nuclear pasta have used the Wigner-Seitz cell approximation with anzats about the geometrical structures like droplet, rod, slab and so on. We perform fully three-dimensional calculation of non-uniform nuclear matter for some cases with fixed proton ratios and in beta-equilibrium based on the relativistic mean-field model and the Thomas-Fermi approximation. In our calculation typical pasta structures are observed. However, there appears some difference in the density region of each pasta structure.

Keywords

Cite

@article{arxiv.1106.3407,
  title  = {Three-dimensional calculation of inhomogeneous structure in low-density nuclear matter},
  author = {Minoru Okamoto and Toshiki Maruyama and Kazuhiro Yabana and Toshitaka Tatsumi},
  journal= {arXiv preprint arXiv:1106.3407},
  year   = {2015}
}

Comments

Proceedings for Research workshops on Nucleation Theory and Applications 2011