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Jacek Dobaczewski University of Warsaw & University of Jyväskylä

Spectroscopic-quality energy density functional and how to get there. Jacek Dobaczewski University of Warsaw & University of Jyväskylä. Jyväskylä : Gillis Carlsson, Markus Kortelainen , Kazuhito Mizuyama, Jussi Toivanen Warsaw : Wojtek Satuła, Tomek Werner,

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Jacek Dobaczewski University of Warsaw & University of Jyväskylä

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  1. Spectroscopic-quality energy density functional and how to get there Jacek Dobaczewski University of Warsaw & University of Jyväskylä Jyväskylä: Gillis Carlsson, Markus Kortelainen, Kazuhito Mizuyama, Jussi Toivanen Warsaw: Wojtek Satuła, Tomek Werner, Maciek Zalewski DFT-UNEDF Workshop Joint Institute for Heavy Ion Research, ORNL, Oak Ridge, TN-37831, USA January 22, 2008

  2. Outline • The Matrix for SkP. • Dependence of single-particle energies on coupling constants. • Fits of spin-orbit and tensor coupling constants. • Error analysis in mass fits. • Extensions in density dependence and stability conditions. • Extensions to higher powers of derivatives. • Extensions to higher powers of densities.

  3. The bottom line • Spectroscopic-quality energy density functional  correct description of positions and evolution of single-particle levels. • Single-particle levels  correct description of one-particle separation energies with all polarization effects included. • Within the EDF method, shape and spin polarization effects in doubly-magic nuclei are relatively small – much smaller than deviations from data. • Dependence of total and single-particle energies on coupling constants is very linear. • No fits without error estimates and error propagation! • Extensions beyond the simple Skyrme functionals are mandatory.

  4. The Matrix – SkP case

  5. Nuclear Energy Density Functional

  6. (c) spin-orbit  (density)/C0 (b) particle 40Ca SLy5 (b) (a) density (a) kinetic (c) R(fm)

  7. (b) central (a) (c) potential  (b) (a) kinetic (potential)/C0 40Ca SLy5 (c) spin-orbit R(fm)

  8. Mass, shape, and spin polarization effects

  9. Polarization effects for spin-orbit splitting Fits of C0J, C0J , and C1J

  10. Shell gaps

  11. =1/6

  12. =1/4

  13. =1/6

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