Nuclear energy density optimization: Shell structure

M. Kortelainen, J. McDonnell, W. Nazarewicz, E. Olsen, P.-G. Reinhard, J. Sarich, N. Schunck, S. M. Wild, D. Davesne, J. Erler, and A. Pastore
Phys. Rev. C 89, 054314 – Published 15 May 2014
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Abstract

Background: Nuclear density functional theory is the only microscopical theory that can be applied throughout the entire nuclear landscape. Its key ingredient is the energy density functional.

Purpose: In this work, we propose a new parametrization unedf2 of the Skyrme energy density functional.

Methods: The functional optimization is carried out using the pounders optimization algorithm within the framework of the Skyrme Hartree-Fock-Bogoliubov theory. Compared to the previous parametrization unedf1, restrictions on the tensor term of the energy density have been lifted, yielding a very general form of the energy density functional up to second order in derivatives of the one-body density matrix. In order to impose constraints on all the parameters of the functional, selected data on single-particle splittings in spherical doubly-magic nuclei have been included into the experimental dataset.

Results: The agreement with both bulk and spectroscopic nuclear properties achieved by the resulting unedf2 parametrization is comparable with unedf1. While there is a small improvement on single-particle spectra and binding energies of closed shell nuclei, the reproduction of fission barriers and fission isomer excitation energies has degraded. As compared to previous unedf parametrizations, the parameter confidence interval for unedf2 is narrower. In particular, our results overlap well with those obtained in previous systematic studies of the spin-orbit and tensor terms.

Conclusions: unedf2 can be viewed as an all-around Skyrme EDF that performs reasonably well for both global nuclear properties and shell structure. However, after adding new data aiming to better constrain the nuclear functional, its quality has improved only marginally. These results suggest that the standard Skyrme energy density has reached its limits, and significant changes to the form of the functional are needed.

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  • Received 6 December 2013
  • Revised 28 April 2014

DOI:https://doi.org/10.1103/PhysRevC.89.054314

©2014 American Physical Society

Authors & Affiliations

M. Kortelainen1,2,3, J. McDonnell2,3,4, W. Nazarewicz2,3,5, E. Olsen2, P.-G. Reinhard6, J. Sarich7, N. Schunck2,3,4, S. M. Wild7, D. Davesne8,9,10, J. Erler11, and A. Pastore12

  • 1Department of Physics, University of Jyväskylä, P.O. Box 35 (YFL), FI-40014 Jyväskylä, Finland
  • 2Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USA
  • 3Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
  • 4Physics Division, Lawrence Livermore National Laboratory, Livermore, California 94551, USA
  • 5Institute of Theoretical Physics, Warsaw University, ul. Hoża 69, PL-00681 Warsaw, Poland
  • 6Institut für Theoretische Physik, Universität Erlangen, D-91054 Erlangen, Germany
  • 7Mathematics and Computer Science Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
  • 8Université de Lyon, F-69622 Lyon, France
  • 9Université de Lyon 1, Villeurbanne, France
  • 10CNRS/IN2P3, Institut de Physique Nucléaire de Lyon, Lyon, France
  • 11Division of Biophysics of Macromolecules, German Cancer Research Center (DKFZ), Im Neuenheimer Feld 580, D-69120 Heidelberg, Germany
  • 12Institut d'Astronomie et d'Astrophysique, Université Libre de Bruxelles, Code Postal 226, 1050 Brussels, Belgium

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Issue

Vol. 89, Iss. 5 — May 2014

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