中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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。