Neutron Star Matter and Baryonic Interactions


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The properties of neutron-star matter up to the appearance of hyperons are calculated with the aid of Skyrme potentials. The conditions for the appearance of Λ hyperons in matter and values of the density at the point of their appearance are analyzed for various parametrizations of nucleon-nucleon and hyperon-nucleon interactions. The dependence of the results on the magnitude of density-dependent forces, the degree of nonlocality, the behavior of the symmetry energy, and incompressibility of nuclear matter is examined.

作者简介

L. Imasheva

Department of Physics

Email: tretyakova@sinp.msu.ru
俄罗斯联邦, Moscow, 119991

D. Lanskoy

Department of Physics

Email: tretyakova@sinp.msu.ru
俄罗斯联邦, Moscow, 119991

T. Tretyakova

Skobeltsyn Institute of Nuclear Physics

编辑信件的主要联系方式.
Email: tretyakova@sinp.msu.ru
俄罗斯联邦, Moscow, 119991

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