Current status of the covariant density functional theory for nuclear structure

来源 :SINAP-CUSTIPEN Workshop on Clusters and Correlations in Nucl | 被引量 : 0次 | 上传用户:yangjianke
下载到本地 , 更方便阅读
声明 : 本文档内容版权归属内容提供方 , 如果您对本文有版权争议 , 可与客服联系进行内容授权或下架
论文部分内容阅读
Existence Limit of nucleus Birth of nuclear physics Around the turn of Nineteenth and Twentieth centuries,the discoveries of radioactivity by Becquerel and the Curies and the existence of a compact nucleus at the center of an atom by Rutherford et al.
其他文献
OUTLINE 1 Introduction Covariant density functional (CDF) theory with Fock terms Motivation:nuclear tensor interactions in Covariant EDF 2 Relativistic Formalis
会议
Summary 1.High-momentum components 2.Implications for symmetry energy 3.Pairing in neutron stars 4.Dineutron in dense matter Why short-range correlations?
会议
Fragments and clusters in heavy-ion collisions Collisions of two nuclei (e.g.,Xe+ Sn at 50 MeV/nucleon,b ≈0) Light-cluster correlations may be important at rel
会议
The p-shell nuclei region (4 < A ≤12) Light nuclei → exotic features:Halo structures - 6He,11Li,8Be Cigar/dineutron configurations - 8He Anti-bound state - 11L
会议
Electron screening (in stars) Debye-Hueckel screening (Salpeter 1959) Dynamical screening in stars Carraro,Schaefer,Koonin,ApJ 1988 Fluctuations in the Debye sp
会议
Outline 1.Brief remarks on the current status of Esym(ρ) from theories and experiments 2.Characteristics of single-nucleon momentum distribution n(k) with a hi
会议
Nucleon pair:isospin singlet/triplet Nuclear force is charge independent The Coulomb interaction doesnt play an important role in low-lying states
会议
In this talk … I will analyse the role of tensor & spin-spin terms of the NN force on Esym (ρ) & L(ρ) in the case of IANM Ssym(ρ) & LS(ρ) in the case of SP
会议
Contents Introduction Models used for EOS New version of EOS tables (∧) hyperon effects EOS for neutron stars Summary Introduction What is the status of EOS Fo
会议
会议