Towards understanding astrophysical effects of nuclear symmetry energy

被引：160

作者：

Li, Bao-An ^{[1
]}

Krastev, Plamen G. ^{[2
]}

Wen, De-Hua ^{[3
]}

Zhang, Nai-Bo ^{[4
]}

机构：

[1] Texas A&M Univ, Dept Phys & Astron, Commerce, TX 75429 USA

[2] Harvard Univ, Fac Arts & Sci, Res Comp, Cambridge, MA 02138 USA

[3] South China Univ Technol, Sch Phys & Optoelect Technol, Guangzhou 510641, Guangdong, Peoples R China

[4] Shandong Univ, Inst Space Sci, Shandong Prov Key Lab Opt Astron & Solar Terr Env, Weihai 264209, Peoples R China

来源：

EUROPEAN PHYSICAL JOURNAL A | 2019年 / 55卷 / 07期

基金：

中国博士后科学基金; 中国国家自然科学基金;

关键词：

EQUATION-OF-STATE; RELATIVISTIC STELLAR MODELS; THOMAS-FERMI APPROACH; HEAVY-ION COLLISIONS; X-RAY OSCILLATIONS; PRECESSING RIGID BODIES; NEUTRON-STAR; GRAVITATIONAL-WAVES; DENSE MATTER; NONRADIAL OSCILLATIONS;

D O I：

10.1140/epja/i2019-12780-8

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

Determining the Equation of State (EOS) of dense neutron-rich nuclear matter is a shared goal of both nuclear physics and astrophysics. Except possible phase transitions, the density dependence of nuclear symmetry E-sym(rho) is the most uncertain part of the EOS of neutron-rich nucleonic matter especially at supra-saturation densities. Much progresses have been made in recent years in predicting the symmetry energy and understanding why it is still very uncertain using various microscopic nuclear many-body theories and phenomenological models. Simultaneously, significant progresses have also been made in probing the symmetry energy in both terrestrial nuclear laboratories and astrophysical observatories. In light of the GW170817 event as well as ongoing or planned nuclear experiments and astrophysical observations probing the EOS of dense neutron-rich matter, we review recent progresses and identify new challenges to the best knowledge we have on several selected topics critical for understanding astrophysical effects of the nuclear symmetry energy.

引用

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