中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Constraining properties of neutron stars with heavy-ion reactions

文献类型:会议论文

作者Li, Bao-An; Chen, Lie-Wen; Ko, Che Ming; Steiner, A. W.
出版日期2006-11
关键词neutron stars nuclear reaction models equation of state
卷号52
期号4
页码56-61
英文摘要Nuclear reactions induced by stable and/or radioactive neutron-rich nuclei provide the opportunity to pin down the equation of state of neutron-rich matter, especially the density (rho) dependence of its isospin-dependent part, i.e., the nuclear symmetry energy E(sym). A conservative constraint, 32(rho/rho(0))(0.7) < E(sym)(rho) < 32(rho/rho(0))(1.1), around the nuclear matter saturation density rho(0) has recently been obtained from the isospin diffusion data in intermediate energy heavy-ion collisions. We review this exciting result and discuss its consequences and implications on nuclear effective interactions, radii and cooling mechanisms of neutron stars.
会议录REVISTA MEXICANA DE FISICA
会议录出版者SOC MEXICANA FISICA
会议录出版地APARTADO POSTAL 70-348, COYOACAN 04511, MEXICO
语种英语
WOS研究方向Physics
WOS记录号WOS:000244651700011
源URL[http://119.78.100.186/handle/113462/58600]  
专题中国科学院近代物理研究所
通讯作者Li, Bao-An
作者单位1.Arkansas State Univ, Dept Chem & Phys, State Univ, AR 72467 USA
2.Shanghai Jiao Tong Univ, Inst Theoret Phys, Shanghai 200240, Peoples R China
3.Natl Lab Heavy Ion Accelerator, Ctr Theoret Nucl Phys, Lanzhou 730000, Peoples R China
4.Texas A&M Univ, Inst Cyclotron, College Stn, TX 77843 USA
5.Texas A&M Univ, Dept Phys, College Stn, TX 77843 USA
6.Los Alamos Natl Lab, Div Theoret, Los Alamos, NM 87545 USA
推荐引用方式
GB/T 7714
Li, Bao-An,Chen, Lie-Wen,Ko, Che Ming,et al. Constraining properties of neutron stars with heavy-ion reactions[C]. 见:.

入库方式: OAI收割

来源:近代物理研究所

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