1. Nuclear Physics -- Today and Tomorrow From the infinitely strong –
Walter F. Henning
From the infinitely strong –
to the infinitely weak
1010 yrs -
10-5 yrs -
From the infinitely small –
to the infinitely large

2. Nucleon-Nucleon / Meson
Nuclear Matter
Hadrons
Deconfinement &
chiral transition
RHIC & LHC
FAIR
Quark Matter
Nuclei
QGP
LHC
RHIC
SPS
Condensate
Hadrons
QCD
Vacuum
Nucleon-Nucleon / Meson

4. QGP
Hadrons
QCD
Vacuum

5. Particle physics Nuclear physics
Transition from the perturbative to the non-perturbative regime of Quantum-Chromodynamics (QCD)
Particle physics Nuclear physics
perturbative:
QCD: aS << 1
non-perturbative:
QCD: aS  1 q
Gluon (g)
Hadrons:
Baryons, Mesons
Models, Lattice QCD
Quarks, Gluons
One-Gluon Exchange

6. Proton Charge and Magnetization The importance of the anti-quark sea
Baryon Structure
Proton Charge and Magnetization
The importance of the anti-quark sea
LA-LP-98-56
Lots of issues – not general agreement on what path is best
The distribution of charge and magnetization are different
There are more down-anti-down quark pairs than up-anti-up quarks pairs in the sea of the proton.

7. Advantages of 120 GeV Main Injector
The Nature of the Sea
The (very successful) past:
Fermilab E866/NuSea
Data in
1H, 2H, and nuclear targets
800 GeV proton beam
The future:
Fermilab E906
Data in
1H, 2H, and nuclear targets
120 GeV proton Beam
Fixed Target Beam lines
Tevatron 800 GeV
Cross section scales as 1/s
7 x that of 800 GeV beam
Backgrounds, primarily from J/ decays scale as s
7 x Luminosity for same detector rate as 800 GeV beam
50 x statistics!!
Main Injector 120 GeV
Advantages of 120 GeV Main Injector

8. Charmed Hadrons @ PANDA/FAIR2 4 6 8 12 15 10
Antiproton momentum [GeV/c]
Mass [GeV/c2]
Two body
thresholds
Quark molecules
Gluonic
excitations
qq Mesons 1 3 5
Hybrids
Hybrids+Recoil
Glueball
Glueball+Recoil ΛΛ ΣΣ ΞΞ
ΛcΛc
ΣcΣc
ΞcΞc
ΩcΩc ΩΩ DD
DsDs
qqqq
ccqq
nng,ssg
ccg
ggg,gg
light qq
π,ρ,ω,f2,K,K* cc
J/ψ, ηc, χcJ
ggg
conventional
charmonium
exotic

9. Nucleon-Nucleon / Meson
QGP
Hadrons
QCD
Vacuum
Nucleon-Nucleon / Meson

10. Hypernuclei: Extension of the Nuclear Chart
Strangeness
Neutron Number
JPARC & FAIR
Horst Lenske has nicely introduced!
… understanding the YN interaction

11. Nucleon-Nucleon / Meson
100 1 5 10 50
Bare Nucleon-Nucleon
Interaction
Mean Field Models
Neutron Number
Proton Number
Shell Model(s)
Microscopic
Ab Initio
(GFMC...)
Quark-Gluon
Effective
Interactions
QCD
Nuclei
QGP
Hadrons
QCD
Vacuum
Nucleon-Nucleon / Meson

12. |+ |- The Nuclear Landscape Applications in Nuclear Medicine1 2 3 4
Applications in
Nuclear Medicine
Nano Science &
Technology
|+
|-
Rare Isotopes as Laboratory:
Precision Tests of
Fundamental Symmetries
The Nuclear Landscape
Nuclear Astrophysics &
Explosive Nucleosynthesis:
Reaction Rates &
Nuclear Properties
Nuclear Matter Properties
& Structure of the Nuclear
Many-Body System

13. The Nuclear Landscape The Nuclear Physics of RI Beams rare isotopes
as a beam
stable particles
as target
The nature of the nuclear force
a strong manifestation of its tensor nature is in changes of shell structure
possible changes in effective interactions and correlations near the limits of stability
exploration of limits: driplines, super-heavy elements, fission barriers ….
The origin of (simple) patterns in nuclei
origin of collectivity
new collective modes, shapes and symmetries
nature of halos and skins, their influence on symmetries
decoupling of neutron degrees of freedom
The Nuclear Landscape

14. Low-lying soft modes in Sn isotopes
P. Adrich et al., PRL 95 (2005)
LAND Collaboration

15. Nuclear Astrophysics

16. The Technology for FRIB: 400kW HI Beams 200 MeV/u Uranium
Superconducting heavy-ion
driver linac
Radio frequency gas stopper
Liquid lithium target/stripper
Multiple charge-state operation
Key concepts conceived,
proposed and developed at ANL

17. Nucleon-Nucleon / Meson
neutron stars
supernovae
heavy-ion collisions
neutron excess (N-Z)/A
finite
nuclei
0.3
-0.3 1 ?
local matter density
0.6
neutron
halos &
skins
neutron drip line
protron
drip line
crust
Nuclear Matter
Nuclei
QGP
Hadrons
QCD
Vacuum
Nucleon-Nucleon / Meson

18. Nucleon-Nucleon / Meson
Nuclear Matter
Deconfinement &
chiral transition
RHIC & LHC
FAIR
Quark Matter
Nuclei
QGP
Hadrons
QCD
Vacuum
Nucleon-Nucleon / Meson
Systems

19. The Phases of QCD
Did the properties of the Quark Gluon Plasma and the quark-gluon to hadron phase transition affect the evolution of the universe?
Does the nature of the plasma and the quark-hadron transition give us new insight into QCD and confinement?
Do states of de-confined quark and gluon matter exist now, i.e. at the core of neutron stars?

20. Nucleon-Nucleon / Meson
Nuclear Matter
S y m m e t r i e s
Deconfinement &
chiral transition
RHIC & LHC
FAIR
Quark Matter
Nuclei
Nuclear Astrophysics
QGP
LHC
RHIC
SPS
Condensate
Hadrons
QCD
Vacuum
Nucleon-Nucleon / Meson
Systems

21. Nucleon-Nucleon / Meson
Nuclear Matter
Deconfinement &
chiral transition
RHIC & LHC
FAIR
Quark Matter
Congratulations
and Best Wishes
for Your Future
QGP
LHC
RHIC
SPS
Condensate
Nuclei
Hadrons
QCD
Vacuum
Nucleon-Nucleon / Meson