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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