Title: Les jeunots en physique nucl
1Les jeunots en physique nucléaire de basse
énergie Some remarks on current theoretical
activities France vs the rest of the
world Thomas Duguet (SPhN)
2Theory of Nuclei
- Goals
- Comprehensive and unified description of all
nuclei - Low-energy reaction and structure properties
- From basic interactions between protons and
neutrons - Understand different states of nuclear matter in
astrophysics environments - Difficulties
- Self-bound, two-component quantum many-fermions
system - Complicated interaction from low-energy regime of
QCD - Tensor and spin-orbit components
- Unnaturally large scattering lengths (2-body
virtual and bound states) - NNN unavoidable
- Repulsive core and strong tensor at short
distances? - Properties of finite and bulk nucleonic matter
- Deuteron to SHE nuclei to neutron stars and
nuclear (strange) matter - Need to extrapolate to unknown regions
- Some trivial facts
- No one size fits all theory for nuclei
3Selection of advances in the recent years
- Ab-initio (NCSMGFMC) methods allowed for
interaction tests - Consistent proof of the role of NNN interaction
in light nuclei - Nuclear interactions c-EFT provides missing
links - Explains hierarchy NN gt NNN gt NNNN 2N-3N, ?N,
??, consistency - Chiral symmetry breaking of QCD encoded gt
constrains ?N interaction - Renormalization Group provides gentle NN
(Vlowk) NNN - Use relevant degrees of freedom/energy scales for
low energy nuclear physics - Many-body problem becomes (mostly) perturbative
(HUGE practical implications) - Quantitative microscopic nuclear structure
- CI calculations into the fp shell sSD608 140
keV! - LACM shape coexistence and fission
- Transfermiums as a window on SHE nuclei
- First EDF mass tables (SR) and systematics of
correlations (MR) in heavy nuclei - Multipole strength S(El)/b-decay from fully
self-consistent (deformed!) QRPA - Shell evolution towards drip-lines role of
tensor force raised - Integration of structure and reaction for light
nuclei - Multistep reactions calculations using coupled
discretized continuum channels - GSM, CSM and SMEC to incorporate (many-body)
continuum in CI - Use of nuclear inputs into reaction models e.g.
JLM optical model
4Selection of challenges for the coming years
- Bridge between hadrons and nuclei
- e.g., lattice QCD with smaller pion masses match
?PT with lattice results - NNN interaction
- Test NNN (NNNN) from c-EFT at N3LO through NCSM
calculations of light nuclei - Role in medium mass nuclei through CC and
spectroscopy through CI and EDF - Interplay of phenomenological and non-empirical
EDF - Constructed from low-momentum interactions/c-EFT
and benchmarked against CC - Predictability (theoretical error bars) and
accuracy (new (re)fitting protocols) - Strong focus on spectroscopy
- Coherent formulation of SR and MR EDF methods
from first principle - Superfluidity
- Nature of pairing correlations in finite nuclei
- Pairing in asymmetric systems e.g.
neutron-proton pairing, polarized cold atoms - Shell position/evolution in stable/neutron rich
nuclei - Role of tensor, NNN, spin-orbit (matter
diffusivity), other? - LACM coexistence, fusion and fission
- Quantitative methods including both diabatic and
adiabatic effects - Integration of structure and reaction
- Advance GSM/CCSD (interaction) and apply to
complex open light nuclei
5Some useful experimental data (not exhaustive!!)
- Fission
- Barriers and life-time
- Mass and kinetic energy distributions of
fragments - Evaporated neutrons and gs
- Systematic data into the next major shell (few
mass units) - Mass differences e.g. shell evolution and
pairing - First 2, B(E2) and Qs e.g. deformation and
shell evolution - Single-particle energies and spectroscopic
factors i.e. shell evolution - Pair transfer e.g. quantitative information on
pairing? - Data at large deformations (low and high J)
- Beta-decay and charge-exchange reactions e.g.
pin down theories for weak rates - Transfermiums
- Rotational bands i.e. pairing and shell
positioning - K-isomers i.e. pairing and shell positioning
- Neutron radii
- Parity violation from e- scattering (208Pb) at
JLAB i.e. Rn-Rp ltgt asym(rsat)/P(rsat/2) - Same in more (neutron-rich) nuclei might be of
interest - Neutron star observations
- Thermal X-ray emission for cooling
6Young french theorists activities by
methods/subjects
STRUCTURE Heavy / Light REACTION Heavy / Light ASTRO NS / n Symmetry Model stand. TOTAL
(TD)EDF 11,75 / - 2 / - 1,5 / - 0,25 15,5
CI 0,5 / 2 - / - - / 1 - 3,5
GSM - / 0,5 - / 0,5 - / - - 1
Opt. Pot. - / - 1 / - - / - - 1
CChannel - / - - / 1 - / - - 1
GFMC - / - - / - - / - - -
NCSM - / - - / - - / - - -
CCluster - / - - / - - / - - -
SCGF - / - - / - - / - - -
NN/NNN - / - - / - - / - - -
TOTAL 12,25 / 3 3 / 1,5 1,5 / 0,5 0,25 22
7Are we well positioned for the next 10/15 years?
- Community extremely biased towards EDF methods
- Chance to propose a coherent effort
- Promising future as experimental facilities move
to medium-mass exotic nuclei - Cultural advantage but US and Japan now put
strong emphasis on EDF e.g. UNEDF - Our expertise suggest to
- Push MREDF methods e.g. QRPA,
GCM/Projection-like methods - Develop further and systematize the use of
Time-Dependent EDF methods - Push cross-fertilization between EDF and CI
e.g. ESNT workshop on April 7-10 - Such a bias carries the danger to miss the big
picture - E.g., somewhat true about ab-initio methods and
nuclear interactions in the 80/90s - Could be detrimental as overlap/benchmarks are
envisioned e.g. with CC - Might need to recruit a few theorists with
different expertise - Interplay between structure and reaction e.g.
GSM - Hard core reaction theory e.g. issue with
extracting spectroscopic factors - Promising ab-initio method for medium mass
nuclei Coupled Cluster
8Geography
- Strong on-going theoretical collaborations
- GANIL-IPNO
- CENBG-GANIL-IPNL-SPhN
- GANIL-SPhN
- Future
- Projects will naturally follow historical
collaborations - But new ones will hopefully arise