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Challenges for EURISOL and the EURISOL Design Study. Yorick Blumenfeld. OUTLINE. The « Standard » scientific case The EURISOL concept and performances Technical Challenges and the Design Study Task 10 : Physics and Instrumentation Goals of the Workshop. The Nuclear Chart and Challenges.
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Challenges for EURISOL and the EURISOL Design Study Yorick Blumenfeld
OUTLINE • The « Standard » scientific case • The EURISOL concept and performances • Technical Challenges and the Design Study • Task 10 : Physics and Instrumentation • Goals of the Workshop
ab initio calculations for light nuclei • Systematic study of light nuclei (A<12) shows the necessity of including a 3-body force R.B. Wiringa and S.C. Pieper, Phys. Rev. Lett. 89 (2002) 182501
4 3 2 20Ca 1 12Mg 16S 0 N 12 16 20 24 Modification of magic numbers far from stability E* (MeV) Lowest 2+ state
46Ar(d,p) 10 MeV/A @ SPIRAL with MUST L. Gaudefroy, thèse
Neutron-proton pairing • n-p pairing can occur in 2 different states: T=0 and T=1. The former is unique to n-p. It can be best studied in N=Z nuclei through spectroscopy and 2-nucleon transfer reactions.
Collective Modes • Atomic nuclei display a variety of collective modes in which an assembly of neutrons moves coherently [e.g Low-lying vibrations and rotations. • Challenge:Will new types of collective mode be observed in neutron-rich nuclei in particular? • Will the nucleus become a three- fluid system-made up of a proton and neutron core plus a skin of neutrons? We will then get collective modes in which the skin moves relative to the core. From W. Gelletly
~80% ~20% Two-proton decay Q2p = 1.14 MeV T1/2 = 3.8 ms Two-proton radioactivity near the proton drip-line Proton energy and angle correlations di-proton emission? J. Giovinazzo et al., PRL89 (2002) 102501
Super heavy elements : discovery and spectroscopy GSI Z112 RIKEN Z=113 DUBNA Z to 118? 294118 • Synthesis of new elements/isotopes (Z 120) • Spectroscopy of Transfermium elements (Z 108) • Shell structure of superheavy nuclei
Studying the liquid-gas phase transition far from stability Muller Serot PRC 1995 Neutron rich nuclei: isospin distillation pressure Bonche Vautherin NPA 1984 asymmetry rp/rn Proton rich nuclei: vanishing limiting temperatures From Ph. Chomaz and F. Gulminelli
Radioactive beam production: Two complementary methods GANIL/SISSI, GSI, RIKEN, NSCL/MSU High energy, large variety of species, Poor optical qualities, lack of energy flexibility GANIL/SPIRAL, REX/ISOLDE, ISAAC/TRIUMF good beam qualities, flexibility, intensity Low energy, chemistry is difficult
The NuPECC Recommendation NuPECC recommends the construction of 2 ‘next generation’ RIB infrastructures in Europe, i.e. one ISOL and one in-flight facility. The in-flight machine would arise from a major upgrade of the current GSI facility, while EURISOL would constitute the new ISOL facility
The EURISOL Road Map • Vigorous scientific exploitation of current ISOL facilities : EXCYT, Louvain, REX/ISOLDE, SPIRAL • Construction of intermediate generation facilities : MAFF, REX upgrade, SPES, SPIRAL2 • Design and prototyping of the most specific and challenging parts of EURISOL in the framework of EURISOL_DS.
The EURISOL Concept Total cost : 613 M€
Some beam intensities Calculations for EURISOL : Helge Ravn 6He 5X1013 pps 18Ne 5X1012 pps
Intensity (pps) Yields after acceleration Comparison between facilities a) Kr isotopes a) Yield for in-flight production of fission fragments at relativistic energy
Experimental Areas Astrophysics Structure Low Energy Reactions
The Major Technological Challenges for EURISOL • 5 MW proton accelerator also capable of accelerating A/Q = 2. • Target(s) sustaining this power and allowing fast release of nuclei • Efficient and selective ion sources producing multi-charged ions • Multi charge state acceleration of radioactive beams with minimal losses • Radioprotection and safety issues
The EURISOL_DS in the 6th framework • Detailed engineering oriented studies and technical prototyping work • 21 participants from 14 countries • 21 contributors from Europe, Asia and North America • Total Cost : 33 M€ • Contribution from EU : 9.16 M€
11 Tasks • Physics, beams and safety • Physics and instrumentation (Liverpool) • Beam intensity calculations (GSI) • Safety and radioprotection (Saclay) • Accelerators : Synergies with HIPPI (CARE) • Proton accelerator design (INFN Legnaro) • Heavy ion accelerator design (GANIL) • SC cavity development (IPN Orsay): SC cavity prototypes and multipurpose cryomodule • Targets and ion sources : Synergies with spallation sources • Multi-MW target station (CERN) : mercury converter • Direct target (CERN) : Several target-ion source prototypes • Fission target (INFN Legnaro) : UCx target • BB : Synergies with BENE • Beam preparation (Jyväskylä) : 60 GHz ECR source • Beta-beam aspects (CERN)
TASK 10 : Physics & Instrumentation • Robert Page, Angela Bonaccorso, Nigel Orr • Expected Deliverables • Broad scientific goals selected • Key experiments selected • Evaluation of feasibility • Conceptual design of apparatus • Costing of instrumentation • Definition of beam properties
Goals of the Workshop • Update the Physics Case : new ideas and newconcepts. • What are the key experiments which will test these concepts? • What are the requirements of the facility : species, energy, …. • How do we carry forward the involvement of theoreticians in the Design Study, and more generally in the EURISOL road map.
Combination of beta beam with low energy super beam Unique to CERN- based scenario combines CP and T violation tests e m(+) (T)me (p+) (CP) e m (-) (T)me (p-)
CERN-SPL-based Neutrino SUPERBEAM 300 MeV n m Neutrinos small contamination from ne (no K at 2 GeV!) Fréjus underground lab. A large underground water Cerenkov (400 kton) UNO/HyperK or/and a large L.Arg detector. also : proton decay search, supernovae events solar and atmospheric neutrinos. Performance similar to J-PARC II There is a window of opportunity for digging the cavern starting in 2008 (safety tunnel in Frejus or TGV test gallery)
Time scales 2005 2007 2010 2012 2016 FAIR Project definition Construction Exploitation
AGATA(Advanced GAmma Tracking Array)4πγ-array for Nuclear Physics Experiments at European accelerators providing radioactive and high-intensity stable beams Main features of AGATA Efficiency: 40% (Mγ=1) 25% (Mγ =30) today’s arrays ~10% (gain ~4) 5% (gain ~1000) Peak/Total: 55% (Mγ=1) 45% (Mγ=30) today ~55% 40% Angular Resolution: ~1º FWHM (1 MeV, v/c=50%) ~ 6 keV !!! today ~40 keV Rates: 3 MHz (Mγ=1) 300 kHz (Mγ=30) today 1 MHz 20 kHz • 180 or 120 large volume 36-fold segmented Ge crystals in 60 or 40 triple-clusters • Digital electronics and sophisticated Pulse Shape Analysis algorithms allow • Operation of Ge detectors in position sensitive mode γ-ray tracking • Demonstrator ready by 2007 • Construction of full array from 2008 ?? J. Simpson
RIA (USA) The Rare Isotope Accelerator(USA)