Induced Pairing Interaction in Neutron Star Matter
文献类型:期刊论文
作者 | Lombardo, U.1,2; Schulze, H. -J.3; Zuo, W.4; Broglia, RA; Zelevinsky, V |
刊名 | FIFTY YEARS OF NUCLEAR BCS: PAIRING IN FINITE SYSTEMS |
出版日期 | 2013 |
页码 | 338-347 |
英文摘要 | The three superfluid phases supposed to occur in neutron stars are reviewed in the framework of the generalized BCS theory with the induced interaction. The structure of neutron stars characterized by beta-stable asymmetric nuclear matter in equilibrium with the gravitational force discloses new aspects of the pairing mechanism. Some of them are discussed in this report, in particular the formation in dense matter of Cooper pairs in the presence of three-body forces and the interplay between repulsive and attractive polarization effects on isospin T = 1 Cooper pairs embedded into the neutron and proton environment. Quantitative estimates of the energy gaps are reported and their sensitivity to the medium effects, i.e., interaction and polarization, is explored. |
WOS关键词 | SUPERFLUIDITY ; NUCLEI ; PARAMETERS |
WOS研究方向 | Physics |
语种 | 英语 |
出版者 | WORLD SCIENTIFIC PUBL CO PTE LTD |
WOS记录号 | WOS:000341264100026 |
源URL | [http://119.78.100.186/handle/113462/56564] |
专题 | 中国科学院近代物理研究所 |
通讯作者 | Lombardo, U. |
作者单位 | 1.INFN LNS, I-95123 Catania, Italy 2.Univ Catania, I-95123 Catania, Italy 3.INFN Sez Catania, I-95123 Catania, Italy 4.Inst Modern Phys, Lanzhou 730000, Peoples R China |
推荐引用方式 GB/T 7714 | Lombardo, U.,Schulze, H. -J.,Zuo, W.,et al. Induced Pairing Interaction in Neutron Star Matter[J]. FIFTY YEARS OF NUCLEAR BCS: PAIRING IN FINITE SYSTEMS,2013:338-347. |
APA | Lombardo, U.,Schulze, H. -J.,Zuo, W.,Broglia, RA,&Zelevinsky, V.(2013).Induced Pairing Interaction in Neutron Star Matter.FIFTY YEARS OF NUCLEAR BCS: PAIRING IN FINITE SYSTEMS,338-347. |
MLA | Lombardo, U.,et al."Induced Pairing Interaction in Neutron Star Matter".FIFTY YEARS OF NUCLEAR BCS: PAIRING IN FINITE SYSTEMS (2013):338-347. |
入库方式: OAI收割
来源:近代物理研究所
浏览0
下载0
收藏0
其他版本
除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。