Extended Skyrme interactions for nuclear matter, finite nuclei, and neutron stars
文献类型:期刊论文
作者 | Zhang, Zhen1,2; Chen, Lie-Wen1,2,3 |
刊名 | PHYSICAL REVIEW C |
出版日期 | 2016-12-28 |
卷号 | 94页码:17 |
ISSN号 | 2469-9985 |
DOI | 10.1103/PhysRevC.94.064326 |
英文摘要 | Recent progress in theory, experiment, and observation challenges the mean-field models by using the conventional Skyrme interaction, suggesting that the extension of the conventional Skyrme interaction is necessary. In this work, by fitting the experimental data of a number of finite nuclei together with a few additional constraints on nuclear matter using the simulated annealing method, we construct three Skyrme interaction parameter sets; namely, eMSL07, eMSL08, and eMSL09, based on an extended Skyrme interaction which includes additional momentum and density-dependent two-body forces to effectively simulate the momentum dependence of the three-body force. The three new interactions (i) can reasonably describe the ground-state properties and the isoscalar giant monopole resonance energies of various spherical nuclei used in the fit as well as the ground-state properties of many other spherical nuclei, (ii) nicely conform to the current knowledge on the equation of state of asymmetric nuclear matter, (iii) eliminate the notorious unphysical instabilities of symmetric nuclear matter and pure neutron matter up to a very high density of 1.2 fm(-3), and (iv) simultaneously support heavier neutron stars with mass larger than two times the solar mass. One important difference of the three new interactions involves the prediction of the symmetry energy at supra-saturation densities, and these new interactions are thus potentially useful for the future determination of the largely uncertain high-density symmetry energy. In addition, the predictions of nuclear matter, finite nuclei, and neutron stars made using the three new interactions are compared with those made using the three typical interactions BSk22, BSk24, and BSk26 from the Brussels group. |
WOS关键词 | EQUATION-OF-STATE ; GIANT MONOPOLE RESONANCE ; HEAVY-ION REACTIONS ; MEAN-FIELD MODELS ; X-RAY BINARIES ; KAON PRODUCTION ; DENSE MATTER ; FREE-PATH ; RADII ; DENSITIES |
资助项目 | Major State Basic Research Development Program (973 Program) in China[2013CB834405] ; Major State Basic Research Development Program (973 Program) in China[2015CB856904] ; NNSF of China[11625521] ; NNSF of China[11275125] ; NNSF of China[11135011] ; Shanghai Municipal Education Commission ; Shanghai Education Development Foundation ; Program for Professor of Special Appointment (Eastern Scholar) at Shanghai Institutions of Higher Learning ; Key Laboratory for Particle Physics, Astrophysics and Cosmology, Ministry of Education, China ; Science and Technology Commission of Shanghai Municipality[11DZ2260700] |
WOS研究方向 | Physics |
语种 | 英语 |
出版者 | AMER PHYSICAL SOC |
WOS记录号 | WOS:000391015500001 |
资助机构 | Major State Basic Research Development Program (973 Program) in China ; NNSF of China ; Shanghai Municipal Education Commission ; Shanghai Education Development Foundation ; Program for Professor of Special Appointment (Eastern Scholar) at Shanghai Institutions of Higher Learning ; Key Laboratory for Particle Physics, Astrophysics and Cosmology, Ministry of Education, China ; Science and Technology Commission of Shanghai Municipality |
源URL | [http://119.78.100.186/handle/113462/44088] |
专题 | 中国科学院近代物理研究所 |
通讯作者 | Chen, Lie-Wen |
作者单位 | 1.Shanghai Jiao Tong Univ, Dept Phys & Astron, Shanghai 200240, Peoples R China 2.Shanghai Jiao Tong Univ, Shanghai Key Lab Particle Phys & Cosmol, Shanghai 200240, Peoples R China 3.Natl Lab Heavy Ion Accelerator, Ctr Theoret Nucl Phys, Lanzhou 730000, Peoples R China |
推荐引用方式 GB/T 7714 | Zhang, Zhen,Chen, Lie-Wen. Extended Skyrme interactions for nuclear matter, finite nuclei, and neutron stars[J]. PHYSICAL REVIEW C,2016,94:17. |
APA | Zhang, Zhen,&Chen, Lie-Wen.(2016).Extended Skyrme interactions for nuclear matter, finite nuclei, and neutron stars.PHYSICAL REVIEW C,94,17. |
MLA | Zhang, Zhen,et al."Extended Skyrme interactions for nuclear matter, finite nuclei, and neutron stars".PHYSICAL REVIEW C 94(2016):17. |
入库方式: OAI收割
来源:近代物理研究所
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