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Saturation of Nuclear Matter and Roles of Many-Body Forces: nuclear matter in neutron stars probed by nucleus-nucleus scattering

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arxiv 1604.07632 v1 pith:V7KWOEDD submitted 2016-04-24 nucl-th hep-ph

classification nucl-thhep-ph
keywords nuclearmattersaturationdevelopmentsforcesneutronnucleus-nucleusproperty
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Yoichiro Nambu put a great foot print in nuclear physics in the era of its fundamental developments including his pioneering insight into essential ingredients of repulsive core of nuclear force and its relation to the saturation of nuclear matter. The present review article focuses onto recent developments of the interaction models between colliding nuclei in terms of Brueckner's G-matrix theory staring from realistic nuclear forces and the saturation property of symmetric nuclear matter as well as neutron-star matter. A recently proposed unique scenario of extracting the saturation property of nuclear matter and stiffness of neutron stars through the analysis of nucleus-nucleus elastic scattering in laboratories is presented in some detail.

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Cited by 1 Pith paper

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  1. On variational trial functions in the extended Thomas-Fermi method

    nucl-th 2024-11 accept novelty 6.0 of 10

    A kink in the trial nucleon density at the center of cylindrical or plane-parallel Wigner-Seitz cells makes the fourth-order extended Thomas-Fermi energy divergent; only spherical-cell kinks are harmless.

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