[Submitted on 12 Dec 2015]
Impacts of the Nuclear Symmetry Energy on Neutron Star Crusts
Shishao Bao🇨🇳 · Hong Shen🇨🇳
Using the relativistic mean-field theory, we adopt two different methods, namely, the coexisting phase method and the self-consistent Thomas-Fermi approximation, to study the impacts of the nuclear symmetry energy on properties of neutron star crusts within a wide range of densities. It is found that the nuclear symmetry energy and its density slope play an important role in determining the pasta phases and the crust-core transition.
- Comments:
- 4 pages, 2 figures
- Subjects:
- Nuclear Theory (nucl-th)
- arXiv:
- 1512.03870 [pdf]