Published March 2005 | Version v1
Journal article

Bridging the gap between X(5) and the interacting boson model

  • 1. Wright Nuclear Structure Laboratory, Yale University, New Haven, Connecticut 06520 (United States)
  • 2. National Institute of Physics and Nuclear Engineering, Bucharest-Magurele (Romania)

Description

Phase transitional behavior in the evolution of nuclear structure from spherical to deformed shapes is often investigated in two seemingly different contexts: within the framework of the interacting boson approximation (IBA) model, or using a geometric approach such as the X(5) or E(5) solutions. To study the connection between these two different models, two-parameter IBA-1 calculations were performed and compared to the parameter-free predictions of the X(5) model. The results show that the X(5) solution cannot be exactly reproduced by any point in the two-parameter space and that the best agreement is close to, but does not coincide with, the phase transitional region for a finite number of particles. Comparison of these two approaches with experimental data on X(5)-type nuclei shows that while X(5) and the two-parameter IBA can reproduce characteristic energy ratios in these nuclei, the IBA calculations give better agreement with the experimental electromagnetic transition strengths

Additional details

Identifiers

Publishing Information

Journal Title
Physical Review. C, Nuclear Physics
Journal Volume
71
Journal Issue
3
Journal Page Range
p. 034309-034309.6
ISSN
0556-2813
CODEN
PRVCAN

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
37011900
Subject category
S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
Descriptors DEI
COMPARATIVE EVALUATIONS; DEFORMED NUCLEI; ENERGY-LEVEL TRANSITIONS; INTERACTING BOSON MODEL; MATHEMATICAL SOLUTIONS; NUCLEAR STRUCTURE; PHASE TRANSFORMATIONS; SPACE; SPHERICAL CONFIGURATION
Descriptors DEC
CONFIGURATION; EVALUATION; MATHEMATICAL MODELS; NUCLEAR MODELS; NUCLEI; SHELL MODELS

Optional Information

Notes
(c) 2005 The American Physical Society