nustar plans at fair
DESCRIPTION
NUSTAR plans at FAIR. Reiner Krücken for the NUSTAR collaboration Physik Department E12 Technische Universität München & Maier-Leibnitz-Laboratorium für Kern- und Teilchenphysik. Long Standing Questions of Nuclear Structure Physics. What are the limits for existence of nuclei? - PowerPoint PPT PresentationTRANSCRIPT
R.Krücken
NUSTAR plans at FAIR
Reiner Krückenfor the NUSTAR collaboration
Physik Department E12Technische Universität München
&Maier-Leibnitz-Laboratoriumfür Kern- und Teilchenphysik
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Long Standing Questions of Nuclear Structure Physics
• What are the limits for existence of nuclei?– Where are the proton and neutron drip lines
situated? – Where does Mendeleyev’s table end?
• How does the nuclear force depend on varying proton-to-neutron ratios?– What is the isospin dependence of the spin-orbit
force?– How does shell structure change far away from
stability?
• How to explain collective phenomena from individual motion?– What are the relevant degrees of freedom and
symmetries of the many-body system?
• How are complex nuclei built from their basic constituents?– What is the effective nucleon-nucleon interaction?– How does it connect to QCD?
• What are the nuclei relevant for astrophysical processes and what are their properties?
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Superheavy elementsNuclear Structure at the extremes
Halos
New shell gaps through residual interaction
Neutron skins
Soft collective modes
Shell quenching bydiffuse surface
New shell gaps through residual interaction
132SnP. Ring, TUM
ele
ctri
c dip
ole
str
eng
th
harmonic oscillator+ spin-orbit+centrifugal
diffuse surfaceneutron rich+ spin-orbit
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Lack of predictive power of mean-field models
from RIA Whitepaper
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FAIR: Facility for Antiproton and Ion Research
Primary Beams
• 1012/s; 1.5-2 GeV/u; 238U28+
• Factor 100-1000 over present in intensity• 2(4)x1013/s 30 GeV protons• 1010/s 238U73+ up to 35 GeV/u • up to 90 GeV protons
Secondary Beams
•Broad range of radioactive beams up to 1.5 - 2 GeV/u; up to factor 10 000 in
intensity over present •Antiprotons 3 - 30 GeV
Storage and Cooler Rings
UNILACSIS
FRS
ESR
SIS 100/300
HESRSuperFRS
NESR
CR
RESR FLAIR •Radioactive beams
•e- - A and Antiproton-A collider
•1011 stored and cooled 0.8 - 14.5 GeV antiprotons
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UNILACSIS
FRS
ESR
HESRSuperFRS
NESR
CR
RESR
NUSTAR facility(NUclear-STructure, -Astrophysics, and -
Reactions)
NUSTAR collaboration(ca. 450 scientists) chair / deputy:
W.B. Gelletly / R. Krücken
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SUPERconducting FRagment Separator
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Super-FRS – Low Energy Branch
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Low Energy Branch
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The AGATA project(Advanced GAmma-ray Tracking Array)
4-array based on 180 36-fold segmented Ge detectors
AGATA will give major improvements compared to current Ge detector arrays in detection efficiency, angular resolution and rate capabilities
Technology• highly segmented Ge detectors • fast digital electronics • pulse shape analysis and tracking
• determination of each interaction point, full
tracking
• position resolution < 5mm
• angular resolution < 1º
• FWHM (1 MeV, =0.5) < 5keV > 40keV
• efficiency (M=1,30) 50% / 27% 20% / 5%
• data rate (M=1,30) 3 / 0.3 MHz <1/0.05
MHz
Features:
today
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Decay spectroscopy (DESPEC)
• Decay properties of nuclei along the r-process
– -decay half-lives, -delayed neutron emission
• Test of the stability of shell closures and search for shell-quenching
• Decay-spectroscopy of isomeric states
• Measurement of nuclear moments and lifetimes using gamma-ray spectroscopy following -decay or isomeric decays
Spokesperson: B. Rubio
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High Energy Branch
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High Energy BranchReactions with Relativistic Radioactive Beams
(R3B)
• total absorption cross section
• knock-out reactions
• quasi-free scattering
• electromagnetic excitations
• charge-exchange reactions
• fission and spalation
• projectile fragmentation
Magnet partly financed through EU constructionproposal
Spokesperson: T. Aumann
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Ring Branch
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Mass measurements in the storage ring (ILIMA)
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Schottky Frequency Spectrum
Yu.A. Litvinov et al.
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Reach of ILIMA mass measurements
Spokesperson: Y. Novikov
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Exotic nuclei studied in light-ion reactions at the NESR storage ring (EXL)
Reactions at low momentum transfer:
• Elastic Proton-Scattering • Quasi-free scattering• Transfer Reactions• Charge-exchange reactions• etc.
Spokesperson: M. Chartier
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Electron-Ion scattering in a Storage Ring (eA collider) (ELISe)
• charge densities from elastic electron scattering• collective modes via inelastic electron scattering • single-particle structure from (e,e’N) reactions
5 %
0.15 fm
132Sn(e,e)
Simulation for 1 week
Spokesperson: H. Simon
point-like probe + clean interaction precision studies in exotic nuclei
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Antiproton Ion Collider (AIC )Spokesperson: R. Krücken Project Manager: P. Kienle
P. Kienle, Nucl. Instr. Meth. B 214 (2004) 193
A A-1
p132Sn 131In132Sn 131Sn
z
-0.0
075
0.0
128
132Sn
Acceptancelimit of NESR
• annihilation of single nucleon in quasi-free process
• detection of A-1 products via Schottky Method or particle detectors
• measure• total absorption cross-section • absorption on neutrons and protons separately
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Radii and cross sections
AIC goal:rnp on the order of <10%
Determine proton and neutron radii independently in the same experiment
H. Lenske, P. Kienle, nucl-th/0502065
theoryfrom Cwith
2
2
2
ppR
nnR
pntotalR
rA
ZC
rA
NC
rC
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Summary and Outlook
• The FAIR facility is the central future project for the European Nuclear and Hadron Physics Communities
• The NUSTAR Facility with the Super-FRS covers a wide range of topics concerning the investigation of exotic nuclei in the areas of: Nuclear Structure, Nuclear Astrophysics, Nuclear Reactions
• NUSTAR will address fundamental questions concerning:
– the Structure und Dynamics of the many-body system atomic nucleus
– the Nature of the effective nucleon-nucleon interaction• relevant components, isospin dependence, correlations
– Nuclear Astrophysics and the Origin of the Elements
• The Super-FRS is part of the first stage of FAIR construction
• There will be a continuous transition from the current FRS program to the future activities at FAIR
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11 NUSTAR Technical Proposals
NUclear-STructure, -Astrophysics, and -Reactions Collaboration(includes ongoing GSI program at FRS, ESR, SHIP, and a strong theory community)
1.) Low Energy Branch (LEB) coord.: C.Scheidenberger GSI
High-resolution In-Flight Spectroscopy (HISPEC) Zs. Podolyak Surrey
Decay Spectroscopy with Implanted Ion Beams (DESPEC) B. Rubio Valencia
Precision Measurements of very short-lived Nuclei using an
Advanced Trapping System for highly-charged Ions (MATS) K.Blaum Uni. Mainz
LASER Spectroscopy for the Study of Nuclear Properties (LASPEC) P. Campbell Manchester
Neutron Capture Measurements (NCAP) M.Heil FZ Karlsruhe
Antiprotonic Radioactive Nuclides (Exo+pbar) M. Wada RIKEN
2.) High Energy Branch (R3B)
A Universal Setup for Kinematical Complete Measurements of
Reactions with Relativistic Radioactive Beams (R3B) T. Aumann GSI
3.) Ring Branch (STORIB)
Study of Isomeric Beams, Lifetimes and Masses (ILIMA) Y. Novikov St. Petersburg
Exotic Nuclei Studied in Light-Ion Induced Reactions
at the NESR Storage Ring (EXL) M. Chartier Liverpool
Electron-Ion Scattering in a Storage Ring (e-A Collider) (ELISe) H. Simon GSI
Antiproton-Ion Collider: A Tool for the Measurement of Neutron and
Proton rms radii of Stable and Radioactive Nuclei (AIC) R. Krücken TU Munich
>450 people