1997
DOI: 10.1103/physrevc.55.1767
|View full text |Cite
|
Sign up to set email alerts
|

Elimination of the vacuum instability for finite nuclei in the relativisticσ-ωmodel

Abstract: The -model of nuclei is studied at leading order in the 1/N expansion thereby introducing the selfconsistent Hartree approximation, the Dirac sea corrections and the one fermion loop meson self-energies in a unified way. For simplicity, the Dirac sea is further treated within a semiclassical expansion to all orders. The well-known Landau pole vacuum instability appearing in this kind of theory is removed by means of a scheme recently proposed in this context. The effect of such a removal on the low momentum ef… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
3

Citation Types

0
4
0

Year Published

2001
2001
2017
2017

Publication Types

Select...
4

Relationship

0
4

Authors

Journals

citations
Cited by 4 publications
(4 citation statements)
references
References 26 publications
(43 reference statements)
0
4
0
Order By: Relevance
“…Intrinsic problems of the perturbative calculations as the ghost poles or the associated vacuum instabilities must be studied, and their implications for the phenomenology clearly stated. Perhaps the association of the procedure adopted in the present work to treat the amplitudes with procedures devoted to the elimination of vacuum instabilities may give us adequate answer to such questions [32]. Having this in mind, it would be interesting to apply the formulation of the NJL model presented here to the SU(3) version.…”
Section: Discussionmentioning
confidence: 99%
“…Intrinsic problems of the perturbative calculations as the ghost poles or the associated vacuum instabilities must be studied, and their implications for the phenomenology clearly stated. Perhaps the association of the procedure adopted in the present work to treat the amplitudes with procedures devoted to the elimination of vacuum instabilities may give us adequate answer to such questions [32]. Having this in mind, it would be interesting to apply the formulation of the NJL model presented here to the SU(3) version.…”
Section: Discussionmentioning
confidence: 99%
“…A procedure for eliminating such instabilities was presented in Ref. [31]. The significant fact that the model breaks down at length scales 0.2 fm, smaller than the nucleon size, could indicate the emergence of substructure effects.…”
Section: Discussionmentioning
confidence: 99%
“…The approach proposed neglects divergent contributions from the Dirac sea, as it is a common practice in QHD calculations. It must be taken into account that QHD models exhibit vacuum instabilities [29,30,31] which appear for transferred momentum above 2 − 3 GeV [29], when Dirac contributions to the diagram in Fig. 1(c) are included.…”
Section: Discussionmentioning
confidence: 99%
“…Note that, in order to perform this on the lagrangian level, nonperturbative and nonlocal counterterms would have to be added to the theory. However the status of such a counterterms is not clear, cf [47]…”
mentioning
confidence: 99%