Published March 2005 | Version v1
Journal article

Self-consistent description of multipole strength in exotic nuclei: Method

  • 1. Joint Institute for Heavy-Ion Research, Oak Ridge, Tennessee 37831 (United States)
  • 2. Physics Division, Oak Ridge National Laboratory, Post Office Box 2008, Oak Ridge, Tennessee 37831 (United States)
  • 3. Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996 (United States)
  • 4. Department of Physics and Astronomy, CB3255, University of North Carolina, Chapel Hill, North Carolina 27599-3255 (United States)
  • 5. Physics Division, Argonne National Laboratory, Argonne, Illinois 60439 (United States)
  • 6. Institute of Theoretical Physics, Warsaw University, ul. Hoza 69, 00-681 Warsaw (Poland)
  • 7. Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996 (United States) and Physics Division, Oak Ridge National Laboratory, Post Office Box 2008, Oak Ridge, Tennessee 37831 (United States)
  • 8. Institute of Nuclear Research and Nuclear Energy, Bulgarian Academy of Science, Sofia 1784 (Bulgaria)

Description

We use the canonical Hartree-Fock-Bogoliubov basis to implement a self-consistent quasiparticle-random-phase approximation (QRPA) with arbitrary Skyrme energy density functionals and density-dependent pairing functionals. The point of the approach is to accurately describe multipole strength functions in spherical even-even nuclei, including weakly bound drip-line systems. We describe the method and carefully test its accuracy, particularly in handling spurious modes. To illustrate our approach, we calculate isoscalar and isovector monopole, dipole, and quadrupole strength functions in several Sn isotopes, both in the stable region and at the drip lines. We also investigate the consequences of neglecting the spin-orbit or Coulomb residual interactions in the QRPA

Additional details

Publishing Information

Journal Title
Physical Review. C, Nuclear Physics
Journal Volume
71
Journal Issue
3
Journal Page Range
p. 034310-034310.15
ISSN
0556-2813
CODEN
PRVCAN

Optional Information

Notes
(c) 2005 The American Physical Society