Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-11-23
Phys.Rev.C76:025801,2007
Astronomy and Astrophysics
Astrophysics
5 pages, 4 figures
Scientific paper
10.1103/PhysRevC.76.025801
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.
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