The nuclear symmetry energy and stability of matter in neutron star

Astronomy and Astrophysics – Astrophysics

Scientific paper

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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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