中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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
DOI10.1103/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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