2014
DOI: 10.1051/epjconf/20146602064
|View full text |Cite
|
Sign up to set email alerts
|

Nuclear charge-exchange excitations in localized covariant density functional theory

Abstract: Abstract. The recent progress in the studies of nuclear charge-exchange excitations with localized covariant density functional theory is briefly presented, by taking the fine structure of spin-dipole excitations in 16 O as an example. It is shown that the constraints introduced by the Fock terms of the relativistic Hartree-Fock scheme into the particle-hole residual interactions are straightforward and robust.

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
1

Citation Types

0
1
0

Year Published

2016
2016
2018
2018

Publication Types

Select...
2

Relationship

0
2

Authors

Journals

citations
Cited by 2 publications
(1 citation statement)
references
References 17 publications
(33 reference statements)
0
1
0
Order By: Relevance
“…We can solve the RMF equations either in the coordinate r space or in a complete basis. These equations and various extensions were already solved in r space for spherical nuclei, including the RMF equations [167,168], the relativistic Hartree-Bogoliubov (RHB) equations [169][170][171][172][173][174], the relativistic Hartree-Fock (RHF) equations [175][176][177][178][179][180], and the random phase approximation based on the RMF and RHF models [181][182][183]. For deformed nuclei, however, it is very difficult to do so because, in addition to conventional complications related to two-dimensional or three-dimensional spatial lattice techniques [184][185][186][187], one also has to deal with problems of the variational collapse 5 and fermion doubling in the relativistic framework.…”
Section: Formalismmentioning
confidence: 99%
“…We can solve the RMF equations either in the coordinate r space or in a complete basis. These equations and various extensions were already solved in r space for spherical nuclei, including the RMF equations [167,168], the relativistic Hartree-Bogoliubov (RHB) equations [169][170][171][172][173][174], the relativistic Hartree-Fock (RHF) equations [175][176][177][178][179][180], and the random phase approximation based on the RMF and RHF models [181][182][183]. For deformed nuclei, however, it is very difficult to do so because, in addition to conventional complications related to two-dimensional or three-dimensional spatial lattice techniques [184][185][186][187], one also has to deal with problems of the variational collapse 5 and fermion doubling in the relativistic framework.…”
Section: Formalismmentioning
confidence: 99%