Title: Prezentacja programu PowerPoint
1Spectroscopic-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 Satula, Tomek Werner,
Maciek Zalewski
DFT-UNEDF Workshop Joint Institute for Heavy Ion
Research, ORNL, Oak Ridge, TN-37831, USA January
22, 2008
2Outline
- 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.
3The 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.
4The Matrix SkP case
Skyrme binding energy, saturation density incompressibility, enhancement factor, isospin symmetry energy at ?0 and ?0/2 (6 parameters) Effective Mass Skyrme surface energy Spin-orbit strength W0 Average pairing matrix element
NM binding energy saturation density incompressibility, enhancement factor, isospin symmetry energy at ?0 and ?0/2 (6 observables) ?
1 ?
Binding energies of 16O and 208Pb ?
Binding energies of 120-132Sn ?
Average pairing gap ?
5Nuclear Energy Density Functional
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11(b) central
(a)
(c)
potential
?
(b)
(a) kinetic
?(potential)/?C0
40Ca
SLy5
(c) spin-orbit
R(fm)
12Mass, shape, and spin polarization effects
13Polarization effects for spin-orbit splitting
Fits of C0?J, C0J , and C1J
14Shell gaps
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