Title: Theoretical Remarks
1 Theoretical Remarks
http//unedf.org
- N. Schunck
- Department of Physics ? Astronomy, University of
Tennessee, Knoxville, TN-37996, USA - Physics Division, Oak Ridge National Laboratory,
Oak Ridge, TN-37831, USA
Gretina Science Workshop, LBNL, April 23-24 2009
2Theoretical Nuclear Structure
1
Inter-Nucleon NN, NNN Interactions AV18, EFT,
Vlow-k
Theory of Light Nuclei Verification
NCSMGFMCCC Validation Nuclei with A 6
Density functional Theory Improved
functionals Remove computationally-imposed
constraints Global properties of nuclei with A gt
16
Low-energy Reactions Hauser-Feshbach Feshbach-Kerm
an-Koonin Fission Mass and energy distributions
Dynamic Extensions of DFT LACM, GCM, TDDFT, QRPA,
CI, CC Level densities
3Modern Challenges in DFT
2
- Development of new generations of energy
functionals - Explore functionals that go beyond Skyrme or
Gogny - Use of a larger, more constraining, experimental
dataset - Remove artificial CPU limitations by using
high-performance computing - Construction of a sound theoretical framework
- Kohn-Sham theorem for self-bound systems
- Passage from NN, NNN, etc. interaction to
functional form - Inclusion of beyond mean-field correlations on a
large scale - Clarify their role formal aspects as well as
practical ones - Systematically benchmark with experiment
4On the relevance of shell structure
3
- Among other things, shell structure is behind
- Magicity
- Existence of deformed nuclei (Jahn-Teller
effect), including exotic ones (like tetrahedral
nuclei) - Position of rotational bands with respect to g.s.
band - Gives fine-tuning correction to masses
- Evolution of s.p. levels with respect to any
symmetry-breaking term dictated, to a large
extent, by symmetries, i.e. quantum numbers, and
relative position of levels
Remark Shell structure directly impacts pairing
correlations large shell gaps cause pairing
collapse
Tensor
Spin-orbit
Skyrme Functional
Vanishes for even-even nuclei
5Why odd nuclei are useful
4
- Probe time-odd terms
- Give detailed, relatively model-independent
information on shell structure near the Fermi
level - Help probe pairing properties
- What could help
- Have bandhead excitation energies in superheavies
(limit of large A) - Have spectroscopic information (Nilsson labels)
6Why deformed nuclei are useful
5
- Good old Strutinsky theorem
- EHF Emacro dEshell
- How to disantangle the macroscopic and
microscopic contribution ? - Poor deformation properties of current
functionals - Fission, hyper-deformation, exotic deformations
like tetrahedral, hindered by macroscopic effects
- What could help
- Spins of the Jacobi shape transition (critically
dominated by macroscopic behavior) - Discrete ? transitions in the HD well probe
extreme deformations - More linking transitions from (HD), SD to g.s.
band
7Why superheavy nuclei are useful
6
M. Bender et al., Phys. Rev. C 60, 034304 (1999)
Macroscopic Deformation Energy ELD(def)
Z122
- SH good playground to test
- Extrapolability of interactions
- Bulk properties vs. shell effects
- What could help
- Single-particle structure in odd-mass SH gives a
snapshot of the shell structure - Rotational bands up to very high spins exploring
collective properties
Z124
Z126
Z128
Z130
N184
8Experimental data
7
- Bottom lines are
- We want to be sure that every term of the
functional is properly constrained - We need to control errors (experimental and
theoretical) - We want as much data as possible at the DFT
level, but some of it clearly will have to go
beyond
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