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2 Euroschool on Exotic Beams: 20 th anniversary! paying back tuition loans after 20 years 2
3 Production of Exotic Euroschools In-Flight Separation of Projectile Fragments by David J. Morrissey and Brad M. Sherrill Lect. Notes Phys. 651, (2004) Isotope Separation On Line and Post Acceleration by Piet Van Duppen Lect. Notes Phys. 700, (2006) Production and acceleration of rare-isotope beams by Giovanni Bisoffi Euroschool 2012, Athens, Greece ISOL & In-flight methods, ion sources, accelerators et al. 3
4 Preparing the technical part of experimental proposal What is approach to the Production of exotic beams lectures at 2013? After discussions with some outstanding theorists, professors, who have brilliant ideas for physical motivation of an experiment, it seems to me, that the good direction of this year lectures is to create a manual how to prepare a technical part of the proposal for the in-flight production and selection experiment. Step by step from the beginning with the use of examples prepared with the LISE ++ code. 4
5 Production of.?? Production of Exotic Beams Stable 12 C is one of most exotic nuclei?! Stable 40 Ca : $.32/oz, whereas stable 48 Ca : $7M/oz 48 Ca is exotic or rare? triple α process Production of Radioactive Ion Beams Do not speak in public a word radioactivity that scares our neighbors. They already have problems with the radon in their basements according to EPA (Environmental Protection Agency). We are not guilty for that! Production and acceleration of rare-isotope beams (Euroschool 2012) That is really rare for the In-flight method, mostly is unachievable for the ISOL method 5
6 Production of Fast Rare Ion Beams So Fast Rare Ion Beams Please, do not mix with the Facility for Rare Isotope Beams! Important step forward for FRIB A note from Thomas Glasmacher On August 1, 2013, the Department of Energy s Office of Science (DOE-SC) approved Critical Decision-2 (CD-2), Approve Performance Baseline, and Critical Decision-3a (CD- 3a), Approve Start of Civil Construction and Long Lead Procurements, for the Facility for Rare Isotope Beams (FRIB) project. CD-2 formally establishes the cost and schedule for the FRIB project. The Total Project Cost for FRIB is $730M, of which $635.5M will be provided by DOE and $94.5M will be shared by the community. FRIB will be completed by June 2022 and the project is managing to an early completion in December
7 Why LISE ++? What is it? Step by step from the beginning with the use of examples prepared with the LISE ++ code The code operates under MS Windows environment and provides a highly user-friendly interface. It can be freely downloaded from the following internet addresses: The program LISE ++ is designed to predict the intensity and purity of radioactive ion beams (RIB) produced by In-flight separators. The LISE ++ name (2002) is borrowed from the well known evolution of the C programming language, and is meant to indicate that the program is no longer limited to a fixed configuration like it was in the original LISE program, but can be configured to match any type of device or add to an existing device using the concept of modular blocks. The LISE code (1985) was named after the fragment separator LISE. The main functions of the program: predict the fragment separator settings necessary to obtain a specific RIB; predict the intensity and purity of the chosen RIB; simulate identification plots for on-line comparison; provide a highly user-friendly graphical environment; allow configuration for different fragment separators. The program is constantly expanding and evolving from the feedback of its users around the world. The LISE ++ package includes configuration files for most of the existing fragment and recoil separators found in the world. Many satellite tools have been incorporated into the LISE ++ framework (will be discussed in Friday) Reference: Radioactive beam production with in-flight separators", O.T. and D.Bazin, NIM B (2008)
8 Why LISE ++? Where is it used? (1) how to prepare a technical part of the proposal? RIBF So, for the in-flight RIB facilities with the PAC system for proposals LISE ++ configurations files have been developed by local fragment separator groups. NSCL 8
9 Why LISE ++? Where is it used? (2) So, for the in-flight RIB facilities with the PAC system for proposals LISE ++ configurations files have been developed by local fragment separator groups GANIL GSI How to set up the FRS From SIS extraction of primary beam to isotope identification 9
10 Why LISE ++? Where is it used? (3) in-flight RIB facilities without the PAC system for proposals ACCULINNA & FLNR TAMU FSU 10
11 The Content of the Lectures Production of radioactive ion beams, I (27 August 14:30-16:00) 1. Introduction to RIB production 2. Production Area 3. Separation Production of radioactive ion beams, II (28 August 09:30-11:00) 4. Identification 5. Production of new isotopes Recap-session LISE++ (30 August 11:30-13:00) 6. LISE ++ : Utilities 7. Radioactive beam physicist task 11
12 Acknowledgements (as Copyright issue) Would like to thank MSU colleagues D. Bazin, T. Baumann, D.J. Morrissey, A. Stolz, T. Kubo (RIKEN), H.Weick (GSI) and especially FRIB Chief Scientist B.M. Sherrill for providing materials to prepare these lectures Discussions with B.M.Sherrill (MSU), D.J. Morrissey (MSU) and A.Gade (MSU) are very appreciated 12
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