The nuclear symmetry energy and stability of matter in neutron star
classification
🌌 astro-ph
keywords
energyneutronstarsymmetrymatternuclearstabilitybehavior
read the original abstract
It is shown that behavior of the nuclear symmetry energy is the key quantity in the stability consideration in neutron star matter. The symmetry energy controls the position of crust-core transition and also may lead to new effects in the inner core of neutron star.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.