CRYRING@ESR: A study group report Darmstadt, July 26, 2012 Michael Lestinsky1 , Norbert Angert1 , Ralph Bär1 , Ralph Becker1 , Mario Bevcic1 , Udo Blell1 , Walter Bock1 , Angela Bräuning-Demian1 , Håkan Danared2 , Oleksiy Dolinskyy1 , Wolfgang Enders1 , Mats Engström3 , Achim Fischer1 , Bernhard Franzke1 , Georg Gruber1 , Peter Hülsmann1 , Anders Källberg3 , Oliver Kester1,4 , Carl-Michael Kleffner1 , Yuri A. Litvinov1 , Carsten Mühle1 , Bernhard Müller1 , Ina Pschorn1 , Torsten Radon1 , Heinz Ramakers1 , Hartmut Reich-Sprenger1 , Dag Reistad3 , Galina Riefert1 , Marcus Schwickert1 , Ansgar Simonsson3 , Jan Sjöholm3 , Örjan Skeppstedt3 , Markus Steck1 , Thomas Stöhlker1,5 , Wolfgang Vinzenz1 , and Horst Welker1 1 GSI Helmholtzzentrum für Schwerionenforschung, 64291 Darmstadt, Germany European Spallation Source ESS, SE-221 00 Lund, Sweden 3 Fysikum, Stockholm University, SE-106 91 Stockholm, Sweden 4 Institut für Angewandte Physik, Goethe-Universität Frankfurt, 60438 Frankfurt a. M., Germany 5 Helmholtz-Institut Jena, 07743 Jena, Germany 2 Contents Subject of this Study 5 1 Introduction 7 2 Scientific Motivation 9 3 CRYRING@ESR: Location in the Target Hall at GSI 11 4 CRYRING@ESR: List of Parameters 13 5 CRYRING as Test Bench for FAIR 5.1 Stand-Alone Operation of CRYRING . . . . . . . . . . . . . . . . 5.2 Accelerator Controls . . . . . . . . . . . . . . . . . . . . . . . . . 5.3 Beam Diagnostics . . . . . . . . . . . . . . . . . . . . . . . . . . . 5.4 UHV Control and Interlock System . . . . . . . . . . . . . . . . . 5.5 Radiation Safety and Access Control System . . . . . . . . . . . 5.6 Controls for Technical Infrastructure . . . . . . . . . . . . . . . . 5.7 Preparation for FAIR Commissioning . . . . . . . . . . . . . . . . 5.7.1 Development and Test of Special Commissioning Software 5.7.2 Training of Operating Staff . . . . . . . . . . . . . . . . . . . . . . . . . . 15 15 15 17 18 18 18 18 18 19 . . . . . . . . . . . . . . . . . . 21 21 22 23 23 23 23 24 24 24 25 25 26 26 26 27 27 28 28 6 Proposed Construction Cycle 6.1 Conditions for the Project Start . . . . . . . . . . . . . . . . . 6.2 CRYRING Disassembly and Transport . . . . . . . . . . . . . 6.3 Preparation of the CRYRING Cave at GSI . . . . . . . . . . 6.4 Preparation of the Technical Infrastructure . . . . . . . . . . 6.4.1 Access Control . . . . . . . . . . . . . . . . . . . . . . 6.4.2 Cooling Water . . . . . . . . . . . . . . . . . . . . . . 6.4.3 Electricity . . . . . . . . . . . . . . . . . . . . . . . . . 6.4.4 Others . . . . . . . . . . . . . . . . . . . . . . . . . . . 6.5 Fast ESR Beam Ejection and Transport to CRYRING . . . . 6.6 Completion of the CRYRING Components . . . . . . . . . . 6.6.1 Magnets . . . . . . . . . . . . . . . . . . . . . . . . . . 6.6.2 Power Converters . . . . . . . . . . . . . . . . . . . . . 6.6.3 Beam Diagnostics . . . . . . . . . . . . . . . . . . . . 6.6.4 Radio-Frequency Components . . . . . . . . . . . . . . 6.6.5 UHV . . . . . . . . . . . . . . . . . . . . . . . . . . . . 6.6.6 CRYRING Control System . . . . . . . . . . . . . . . 6.7 Assembly of CRYRING and Injection Beam Lines . . . . . . 6.7.1 Preparation of Magnetic Components: Fiducialization 3 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4 CONTENTS 6.7.2 6.7.3 Procurement of Mechanical Parts . . . . . . . . . . . . . . . . . . . . . . . Assembly . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7 Project Steering 7.1 Time Schedule . . . . . . . . . . . . . . . . . . . . . . . . . . 7.2 Cost and Manpower Requirements . . . . . . . . . . . . . . . 7.3 Project Structure: Installation and Operation . . . . . . . . . 7.4 Possible Sources of Funding . . . . . . . . . . . . . . . . . . . 7.5 Swedish contributions to the installation of CRYRING@ESR 7.6 Swedish Participation in Experiments at FAIR . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 28 28 31 31 32 32 33 33 34 Bibliography 35 A Letters of Support 37 Subject of this study The Swedish in-kind contribution for FAIR includes the storage ring CRYRING, built by the Manne Siegbahn Laboratory in Stockholm. The international FAIR project has decided to accept this Swedish proposal as the central storage ring for the FLAIR facility for experiments with slow and even trapped anti-protons and exotic ions. Recently, in the context of the preparation of CRYRING for the transport to Darmstadt, which is expected to happen still within 2012, the idea was born to ask GSI to check for the option to install the CRYRING in the vicinity of the ESR storage ring inside the Target Hall. Such a project would closely be related to an early realization of the FLAIR facility not included into the Modularized Start Version of the FAIR project. The research with exotic ions as proposed for the FLAIR facility could already now being pursuit with this installation and at a later stage the extension to experiments with slow anti-protons would be possible on the basis of only moderate investments. Following the advice of the GSI scientific council and of the executive board of GSI, the atomic physics department of GSI has been assigned to form a working group∗ in order to come up with a proposal for installing CRYRING within the current Target Hall at GSI and provide a reliable estimate of the required resources to install CRYRING at ESR. The results obtained by this study group for both the resources needed as well as the possible location of CRYRING at GSI are described within the current document. In addition, a comprehensive overview of the physics opportunities which can be addressed by the combination of CRYRING and ESR will be given. Detailed description of physics cases is the subject of a dedicated “Physics Book: CRYRING@ESR”, the actual version of which is attached to this document. Since we still expect a considerable amount of additional contributions from various collaborations interested in the realization of CRYRING@ESR, the physics book is being continuously updated. Once completed, it is planned to publish “Physics Book: CRYRING@ESR” as a regular article in a peer-reviewed scientific journal. Moreover, we added a dedicated chapter “CRYRING as a Test Bench for FAIR” to emphasize the important and possibly even indispensable role of CRYRING as a test bench for many FAIR relevant accelerator related developments. There, emphasis is given to the operation of CRYRING as a stand-alone facility equipped with its own ion source and injector. The CRYRING@ESR is supported by various physics communities as well as by all FAIR storage ring collaborations which is reflected by dedicated support letters. The latter are attached to the Appendix of the current document. ∗ N. Angert, A. Bräuning-Demian, H. Danared, W. Enders, M. Engström, B. Franzke, A. Källberg, O. Kester, M. Lestinsky, Yu. A. Litvinov, D. Reistad, A. Simonsson, J. Sjöholm, M. Steck, and Th. Stöhlker 5 6 CONTENTS Chapter 1 Introduction Storage ring experiments in the realm of atomic and nuclear physics with heavy ions and exotic nuclei contribute substantially to the success of the present GSI SIS18/ESR facility and form one of the essential cornerstones of the future facility for antiproton and ion research FAIR. The corresponding experiments at FAIR are being prepared by the following international collaborations SPARC (Stored Particles Atomic Physics Research Collaboration), FLAIR (Facility for Low-Energy Antiproton and Ion Research), ILIMA (Isomeric beams, LIfetimes, and MAsses), ELISE (ELectron-Ion Scattering Experiment), and EXL (EXotic nuclei studied in Light-ion induced reactions). The contributions by the Swedish and German partners in these collaborations are significant and indispensable. In the case of Sweden, the strong engagement is manifested by the provision of the Stockholm CRYRING facility as a Swedish in kind contribution for FAIR, where it will serve as the central storage ring installation within the FLAIR building. For this purpose substantial resources have already been invested to adapt CRYRING to its future role at FAIR. The delivery of CRYRING is expected to begin at the end of 2012. Because the new storage rings facilities are not part of the modularized start version (MSV) of the international FAIR project (because of the high civil construction cost for the storage ring complex NESR and FLAIR), it has been decided to maintain the operation of ESR — as documented by the Green Paper: The Modularized Start Version ∗ — in order to assure a persisting expertise in storage ring operation and physics and to allow substantial R&D work related to FAIR and in particular to FLAIR. Since CRYRING will be delivered to FAIR by the end of this year, the question needs to be answered is to what extent can CRYRING already be installed at the existing GSI Target Hall or, alternatively, whether it should be stored in containers for the next decade or longer. In view of FAIR, the operation of CRYRING at the existing ESR facility would exhibit various important advantages: • CRYRING as a FAIR test facility could be essential for FAIR relevant R&D projects, in particular with respect to accelerator related developments of instrumentation and controls: beam diagnostics, detector development, synchronization, efficient coupling of accelerators and storage rings, software development etc. Keeping in mind that there will be a break of at least 1.5 years in SIS18 operation, CRYRING would play a very important role by using it as a stand-alone facility. • CRYRING will help secure expertise of the personnel by providing otherwise not available training opportunities. • CRYRING would open novel and unique physics opportunities with large discovery potential and it would allow the existing storage ring collaborations connected to FAIR to continue. 7 8 Chapter 1. Introduction Moreover, the mid and long term physics perspectives of CRYRING@ESR are exciting. Once the MSV of FAIR is accomplished, a transfer beamline for anti-protons and exotic nuclei from the CR to the ESR-CRYRING storage ring complex can be considered. In this way two fully commissioned storage rings, ESR and CRYRING, would be available at a very early stage for experiments using slow anti-protons at FAIR. Additionally, the experiments in the research areas of nuclear- (EXL, ELISe, ILIMA) and hadron physics will profit from this scenario using rare isotope beams from the FRS/ESR facility and later on from the FAIR accelerator chain. Therefore, in view of both the MSV as well as the full version of the FAIR project, installing CRYRING at ESR already now has the potential to save considerable resources. It will provide a platform for prototyping FAIR technologies which is inevitably required and will consequently minimize the amount of time typically needed for the commissioning of these complex storagering facilities. ∗ Green paper [1]: “All these developments are also of particular relevance for future prospects of the SPARC physics programme which concentrates on storage rings and traps, and will become possible with Module 4. For the realization of this programme the ESR storage ring and the HITRAP facility need to be maintained in operation at GSI until they shall be surpassed by Module 4.” Chapter 2 Scientific Motivation In the following we concentrate on the ion part of the physics program to be addressed at CRYRING@ESR. It will cover to a large extent the research with ions as proposed for the FLAIR facility (module 4 of the MSV). Note, at a later stage only a moderate investment for a transfer beam line would be required to transport anti-protons to CRYRING via the ESR and to perform the anticipated FLAIR experiments with slow or even trapped anti-protons. The exploration of the unique properties of stored and cooled beams as provided by heavy ion storage rings has opened novel and fascinating research opportunities in the realm of atomic and nuclear physics research. For the particular case of the ESR storage ring, this has been demonstrated in experiments addressing e.g. the 1s Lamb shift in heavy ions, the hyperfine splitting in hydrogen-like heavy atoms, the investigation of dielectronic recombination in heavy, few-electron ions, direct mass measurements of short-lived radionuclides or by studying rare nuclear decay modes such as the bound-state β-decay or the orbital electron capture decay [2–7]. World-wide, ESR is the only storage ring that provides access to all naturally occurring elements up to the most extreme case of fully stripped uranium. Charge states and energies (4 MeV/u to 500 MeV/u) can be tailored according to the requirements of the experiment [8]. Moreover, intense beams of highly charged in-flight synthesized radioisotopes are at the experimentalist’s disposition. Likewise, CRYRING was operated at the Manne-Siegbahn Laboratory (MSL) in Stockholm with great success [9–15] however with much lighter ions or heavy ions of lower charge state. CRYRING is optimized for operation in an ion energy range of ∼ 14 MeV/u down to 300 keV/u or lower. Both rings, ESR and CRYRING operate in complementary ion energy ranges, and CRYRING thus bridges the gap between the lowest stable operation of ESR (∼ 4 MeV/u) and the HITRAP facility [16] with highly charged ions close to or even at rest whereby preserving the high luminosity, characteristic for stored ion beams. Moreover, for the low energy regime below 10 MeV/u, the properties of CRYRING along with its instrumentation have several advantages compared to ESR such as its compactness and the excellent UHV vacuum conditions of < 10−11 mbar. By combining ESR and CRYRING, the entire energy range from 500 MeV/u almost down to rest will be available for experiments dealing with intense beams of highly charged ions and exotic nuclei. CRYRING@ESR will be the only facility world-wide that provides low-energy highly charged stable beams and beams of rare isotopes with a free choice of the charge state, including bare ions. Radioisotopes synthesized in a target after SIS18 can be purified from unwanted contaminants either with the present fragment separator FRS or alternatively directly in the ESR by employing its high resolving power [16, 17]. Of particular scientific interest are stable ions and artificially synthesized nuclides dressed with few electrons or fully stripped. In such elementary ionic systems the physics topic under investigation is not masked or hampered by many-body effects 9 10 Chapter 2. Scientific Motivation or unwanted spectator electrons. The interpretation of the experiments is thus straightforward and without ambiguity. In addition, the inverse processes of many fundamental atomic and nuclear reaction and decay mechanisms only become experimentally accessible if corresponding vacancies in the atomic shell are available. Examples of these inverse effects include radiative recombination (inverse of photoeffect), dielectronic capture (inverse of autoionization), bound state beta decay (inverse of nuclear electron capture, EC) or nuclear excitation by electron capture (inverse of internal conversion). Low-energy phase space of cooled ions provide extremely well-defined experimental conditions for precision spectroscopy experiments (electrons, ions, and photons). At the same time, compared to ions at rest, orders of magnitude higher luminosity in collision experiments using low-energy ions in a storage ring is achieved due to the repeated interaction of the stored ion beam with a target (gas, free electrons, laser). These luminosities may be comparable to or even exceed those obtainable in single-pass fixed-target experiments while the dilute targets induce only a minimum amount of angular and energy straggling which can be compensated by beam cooling and guarantee for single collision conditions. For atomic collision studies, another appealing aspect is the very strong perturbation to the target atoms due to the impact of the slow highly charged ions with conditions far from equilibrium. CRYRING operates in a particular interesting energy range for nuclear reactions, that is at the Coulomb barrier and in the astrophysically relevant Gamow window of p- and rpprocesses of nucleosynthesis. The swift low-energy beam also makes the detection and monitoring of primary and secondary ions either in a destructive manner with particle detectors or in a non-destructive manner down to the level of single particles by means of Schottky techniques experimentally much easier. Hereby, the storage ring itself serves as a high-resolution magnetic heavy ion spectrometer. The dynamic range that is covered with the various experimental techniques covers the span from single stored ions, detected by means of Schottky noise analysis up to beams at the space charge limit. As stated in a previous section, the capabilities for future research on atomic, nuclear, and astrophysics with a combined CRYRING and ESR facility will be outlined in a dedicated “Physics book: CRYRING@ESR” which is in preparation. The current draft of the physics book is appended to this document. Moreover, since by the installation of CRYRING@ESR a substantial part of the heavy ion program as foreseen at FAIR for NESR and FLAIR can already be addressed, we also like to refer to the already positively evaluated physics programs as described in the FAIR documents of the contributing collaborations (SPARC [18], FLAIR [19], EXL [20], ILIMA [21], and ELISe [22]). Chapter 3 CRYRING@ESR: Location in the Target Hall at GSI For a cost efficient solution of CRYRING@ESR, utilizing existing space, technical installation, and ion beamlines is mandatory. A suitable location for setting up CRYRING at GSI can be found at Cave B, which is almost ideal. We illustrate the envisaged realization of CRYRING@ESR in Figure 3.1. Cave B is located downstream of ESR and a transport beam line for ions is presently available. Further, the cave is of the required size which means required construction changes could be performed without interfering with other experimental installations. Modifications to the cave construction can be done at moderate cost, as this essentially requires only moving available concrete blocks. However, the technical infrastructure and facilities, such as cooling water, electricity, or air conditioning, have to be adapted to the requirements of CRYRING along with its beamlines. 11 12 Chapter 3. CRYRING@ESR: Location in the Target Hall at GSI Figure 3.1. The proposed topology for CRYRING@ESR in the Target Hall of GSI. Several options for a reassembly of CRYRING have been investigated. We propose locating the setup in Cave B as the least invasive and most cost efficient solution. The modified CRYRING with injection beam lines is shown with blue lines. See also Figure 6.1 for a detailed view of the modified Cave B. Chapter 4 CRYRING@ESR: List of Parameters A detailed description of CRYRING (LSR) foreseen for the operation with antiprotons as planned for the envisioned program of the FLAIR collaboration has been given within the TDR “LSR - Low-energy Storage Ring” [23]. In the following we summarize the CRYRING parameters as they are relevant for the operation with heavy ions at the current SIS/ESR facility (Table 4.1). In addition, the most important in-ring installations as they are required for experiments are given below: • Electron cooler • Internal jet target • Transversal electron target • Collinear laser setups • Schottky pickups • Particle counters • Recoil ion, electron, and photon spectrometers Table 4.1. CRYRING parameters as they are relevant for the operation with heavy ions at the current SIS/ESR facility. Circumference 51.63 m Rigidity at injection for ions (antiprotons, protons) 1.44 Tm (0.80 Tm) Highest possible injection energy for p̄, p 30 MeV — for 12 C6+ — for 238 U92+ 24.7 MeV/u (238 U89+ ) 14.8 MeV/u (13.9 MeV/u) Lowest rigidity 0.054 Tm Lowest energy charge exchange limited Magnet ramping (deceleration and acceleration) 7 T/s, 4 T/s, or 1 T/s Vacuum pressure (N2 equiv.) 10−11 –10−12 mbar Beam injection multi-turn and fast Beam extraction slow and fast Ion sources for stand-alone operation yes (300 keV/u, q/A > 0.25) 13 14 Chapter 4. CRYRING@ESR: List of Parameters Chapter 5 CRYRING as Test Bench for FAIR 5.1 Stand-Alone Operation of CRYRING As described in Chapter 3 the installation of CRYRING in the Target Hall in combination with the fragment separator (FRS) and the Experimental Storage Ring (ESR) would represent an attractive, novel facility for atomic and nuclear physics experiments. But CRYRING would also offer an ideal opportunity for testing important technical developments for FAIR under operating conditions. These tests could be performed even during longer shut down periods of SIS18, i.e. without beam from ESR. This is because CRYRING has its own injector and, therefore, can be operated as a stand-alone system. The low energy RFQ injector delivers ions with charge-to-mass ratio q/A ≥ 0.25 at a fixed specific energy of 0.3 MeV/u. The ion beam can be pulsed with repetition frequencies up to 5 Hz and pulse lengths smaller or equal 0.5 ms. Similar to SIS18, multiturn injection is applied to attain higher circulating beam currents. The stand-alone operation would preferably be applied for the commissioning of CRYRING after the completion of the ring assembly and the successful commissioning of all ring systems without ESR beam. For the test of FAIR technologies and components the use of the RFQ-injector seems to be the most suitable mode of operation. Test times would be available without any interference with the time-limited operation of the existing accelerators. Therefore, CRYRING could operate during the long shutdown period of about 18 months expected around the year 2015 and required for • linking the proton linac building to the injection channel TK of SIS18, • modification of the extraction channel of SIS18, • installation of the first part of the beam transport from SIS18 to SIS100, and • major upgrade work on the main control room. According to these considerations CRYRING would be an excellent, if not indispensable test bench for many important developments and technologies for FAIR. Its relevance for the success of the FAIR project with respect to time schedule and quality of operation is briefly discussed in the following. 5.2 Accelerator Controls Though CRYRING is not part of the FAIR modularized start version an installation at ESR would provide excellent possibilities for the controls and other technical departments to implement, test, deploy and evaluate the operational experience for improvements of the technical systems for FAIR. While it was always foreseen to implement FAIR control system solutions with the existing GSI machines (SIS18, ESR), CRYRING would provide even better conditions 15 16 Chapter 5. CRYRING as Test Bench for FAIR for following reasons: • A new stack of control system solutions for FAIR can be implemented and tested without ensuring full compatibility and coherency with the existing control system at any time during development. Some of the new control system design principles for FAIR are fundamentally different from the present GSI system (e.g. new beam and cycle concept, replacement of the Virtual Accelerator concept by a more general and flexible one). With CRYRING, these new solutions can be tested in an almost isolated environment in a system comprising almost all kinds of accelerator systems (ion source, linear accelerator, beam lines, synchrotron and storage ring) and without the constraints and having to reimplement specific GSI functionality of the existing system (e.g. therapy mode, equipment status concept, etc.). • CRYRING as a stand-alone machine can provide more machine development time for control system and equipment tests with much less organizational overhead than at UNILAC, SIS, and ESR. • The present GSI accelerator chain will experience a strongly reduced operation time in the coming years (e.g. 3–4 months of operation per year only) and machine time for control system tests will be quite limited. Machine operation times will be highly dedicated to machine development (MD) activities as well as detector tests for FAIR. Since beam time will be rare, a very stable and reliable control system is essential. This situation would be in contradiction with the strategy to implement novel solutions and evaluate them during longer runs. New solutions cannot provide the same level of robustness and availability from the beginning on. It is to be expected that failures will occur. The opportunity of dedicated MD runs at an independent ion beam facility will allow to solve and fix these rollout problems with a minimal disruption of the precious beam time operation of the GSI accelerators. Practically, the strategy of the controls department would be as follows: Many of the control system solutions needed for CRYRING modification are necessary for FAIR anyway. These are presently already under development or will be developed in the course of the FAIR project. These include front-end software equipment classes, generic operator applications, timing system, setting generation software, etc. It is expected that these solutions can be adapted to CRYRING with only moderate effort. As soon as these solutions are available, they can be implemented in CRYRING for tests. First activities would be to implement the new control system environment designed for FAIR in parallel to the CRYRING installation. This environment will be the base for all control system components including those of the beam diagnostics and available for component and integration tests. Deeper understanding and more investigation of the present CRYRING control system is needed to determine which subsystems can be replaced by corresponding FAIR developments. The following list indicates some examples: Equipment control for power converters with DC, pulsed and ramped operation. The FAIR Standard Control Unit SCU with respective Front End Standard Architecture FESA equipment class developments is the adequate solution. Controller prototypes and engineering samples under development for FAIR can be used. Timing system would be replaced by the facility-wide new General Machine Timing system. Modifications to the timing system are needed anyway for beam transfer from ESR. Bunch to bucket transfer can be implemented and studied for the bunch transfer from SIS18 to 5.3. Beam Diagnostics 17 SIS100 as well as from SIS100 to CR and from CR to HESR for both the proton/antiproton and the radioactive ion beams. Setting generation system can be implemented based on the LHC Standard Architecture LSA framework as an example for a storage ring machine. Tests of the overall storage ring functionality are possible. Feedback from the users would be highly valuable. Generic operator control applications under development for FAIR can be reused for FAIR and valuable operator feedback can be collected and used for improvements. Functions of remote monitoring and manage control authority domains (main control room, local control room) can be tested. Using CRYRING for FAIR development tests will result in reduced commissioning effort and time for the control system once the FAIR machines need to be commissioned. Moreover, early testing allows for better and more stable solutions and well tested operator application programs. In spite of all these benefits with respect to time and money savings, the control system solutions for FAIR cannot be implemented and tested in CRYRING without any additional financial effort and manpower. Technical coordination and necessary software adaptations will require one fulltime position being assigned to the controls department as early as possible after a positive management decision to implement CRYRING@ESR. A potential candidate has already been identified by the Atomic Physics department. For necessary electronic hardware adaptations, the vocational trainee group (Ausbildungsgruppe) in the controls department as well as the young technicians having completed their traineeship would be highly interested to get involved and contribute as well. Without further investigations and decisions about which subsystems to be replaced by FAIR solutions, only some rough cost estimates are given in Section 7.2. However, it can be assumed that for most dedicated hardware components of the control system prototypes and engineering samples of the FAIR developments could be used at no additional costs. 5.3 Beam Diagnostics A great part of the work necessary for the CRYRING beam diagnostics could be eased by applying soft- and hardware techniques foreseen for the FAIR project. All data acquisition (DAQ) systems, i.e. analog and digital electronics, controllers, digitizers, infrastructure systems etc., as well as the required software, should unconditionally apply FAIR standards, like FESA (Front-End Software Architecture) compatibility. Important: DAQ for beam diagnostics is part of the German in-kind contribution (EoI 13i) for FAIR. The GSI beam diagnostics department will deliver the complete set of DAQ systems for FAIR and has strong interest in using CRYRING as a test bench for ongoing hardware and software development projects. This strategy has the advantages of using CRYRING as a test bench for FAIR and the reusability of work load. The results obtained during CRYRING commissioning and test runs will confirm the development concepts and, in this way, improve the preparations for FAIR. The required manpower and budget for the FAIR-type realization of the CRYRING beam diagnostics will certainly entail additional expenses over a minimum cost/equipment solution (see Section 7.2) but these can be justified in view of the opportunity for testing new FAIR equipment under ‘live’ conditions. 18 5.4 Chapter 5. CRYRING as Test Bench for FAIR UHV Control and Interlock System The vacuum controls shall be realized as an industrial control system based on Siemens SIMATIC PLC and a commercial SCADA (Supervisory Control and Data Acquisition) product in connection with the UNICOS (UNified Industrial COntrol System) framework introduced at CERN for the control of the LHC cryogenics. All devices are connected directly to the PLC and thus render a very robust solution. It is being developed and delivered as in-kind contribution by the FAIR member state Slovenia. It would be favorable to implement and operate a vacuum control installation early before implementing it in FAIR machines. Evaluation of the complete system and training of the vacuum group staff would be possible this way. CRYRING provides all necessary vacuum control aspects, including a bakeout system. The additional cost for the FAIR vacuum controls is included in Section 7.2. 5.5 Radiation Safety and Access Control System The CRYRING Cave-B could be removed from existing ZKS system and replaced by an early installation of the FAIR PSS (personnel safety system). New access gate infrastructure technology and procedures could be tested and optimized in order to implement a well-tested system later with the FAIR buildings. 5.6 Controls for Technical Infrastructure The development of instrumentation and control technology will be necessary in order to control and optimize the supply of various FAIR facilities with electricity, cooling and other auxiliary media. For instance, the flow reduction of cooling water or cooling air for facilities standing idle would considerably reduce the required load on the cooling systems. A similar consideration would probably offer a chance for minimizing the capacity of the electricity installations. The new control systems could be tested also at the CRYRING at a time when no other accelerators and experiments are in operation. 5.7 Preparation for FAIR Commissioning Practical experience from earlier accelerator projects shows that, as far as possible, it must be avoided to finally test and commission accelerator components and control system at the same time as the commissioning with ion beams takes place. Precious beam time would be lost for time consuming trouble shouting especially of controls software and hardware components. It is without any controversy that, compared to the regular operation, the commissioning of accelerators usually causes considerably higher demands on both the control system and the operating staff. 5.7.1 Development and Test of Special Commissioning Software The presently practiced commissioning concept at the existing accelerator system at GSI requires to a large extend the intervention of experienced accelerator physicists and engineers. The approach to optimal machine settings is done by many steps of human interpretation of beam diagnostic measurements and subsequent commands to the controls software to suitably change settings. Not only the extremely tight time schedule for the commissioning of the new FAIR facilities but also the requirements of a highly efficient operation with time sharing between 5.7. Preparation for FAIR Commissioning 19 different ion species and energies for several beam users necessitate the development of a novel commissioning concept. The required new software should assume the interpretation of beam diagnostics as well as many of the human interventions. By this way, the commissioning time would be reduced considerably. For the necessary extensive tests of the new commissioning concept the stand-alone operation of CRYRING offers ideal conditions, independent of shutdown times for the existing machines. 5.7.2 Training of Operating Staff At least of comparable importance as development and test of operating software is the extensive training of the operating staff with respect to the commissioning phase of FAIR. The standalone operation of CRYRING covers nearly all relevant aspects of an accelerator facility: ion source, beam transport, linear accelerator, bunch-to-bucket transfer or multiturn injection to a synchrotron/storage ring, beam acceleration or deceleration in the ring, beam cooling and finally slow and fast beam extraction. Insofar, CRYRING must be considered an necessary complement of the FAIR project 20 Chapter 5. CRYRING as Test Bench for FAIR Chapter 6 Proposed Construction Cycle 6.1 Conditions for the Project Start For the installation of CRYRING on the GSI site the following conditions must be met: Formal Agreement upon CRYRING installation at GSI: The construction cycle described in the following presumes that a decision on the installation of CRYRING at GSI will be available by the end of July 2012. CRYRING disassembly by end of 2012: The CRYRING has to be disassembled and the components have to be moved out of the building presently occupied by the ManneSiegbahn Laboratory of the Stockholm University (MSL/SU) by the end of 2012. As the reinstallation of the ring in the planned FLAIR facility has been defined as a part of the Swedish in-kind contribution to the FAIR project with a validation of 2 Million Euro, it has to be decided very speedily, how to proceed with the ring components. Since FLAIR is not a part of the Modularized Start Version (MSV) of FAIR, a storage concept worked out by the MSL foresees the storage of the CRYRING components over a period of 10 years in 12 dehumidified containers on a site defined by the FAIR GmbH. An alternative solution is presented here. It considers the prompt reinstallation and operation of CRYRING at GSI as the experimental device and test facility behind the Experimental Storage Ring ESR. This will allow to realize the science options of FAIR and FLAIR at a much earlier stage as compared to the realization of the modules 4 and 5 of the MSV. Support by MSL/SU: There is strong interest on the Swedish side, i.e. by the present MSL/SU staff and by atomic and nuclear physics groups, to built up and operate the CRYRING facility as modified for FAIR and FLAIR physics experiments in the near future instead. Its long term storage in containers for more then ten years is not recommended. The MSL/SU experts expressed their intent to support the reinstallation as well as the commissioning of CRYRING at GSI. However, this support will be available only if the reinstallation and the commissioning could take place within the next two or three years. Weak interference with FAIR: The envisaged period for the reinstallation and commissioning of CRYRING at GSI in the years 2013–2014 does not interfere with the necessary work for FAIR. There is a marginal involvement of the design and planning capacities. For the installation of the necessary technical systems and the reassembly of the CRYRING the human resources seem to be available until the first components for FAIR will be delivered 21 22 Chapter 6. Proposed Construction Cycle in the 2nd half of 2014 and many acceptance tests have to be prepared and performed. At this time the commissioning of the CRYRING@ESR facility should already be finished and first experiments could be accomplished by operating the facility under the responsibility of the Atomic Physics (AP) department. 6.2 CRYRING Disassembly and Transport According to the LSR-TDR (Danared et al. [23]), the MSL/SU will deliver the following items: For the Low energy injection beam line • An ion source platform for singly charged ions, with all power supplies including a 90◦ analysing magnet without power supply. • Electrostatic quadrupole doublets and triplets with HV-supplies. • An RFQ accelerator with 108.48 MHz rf-generator including a 108.48 MHz debuncher cavity without rf-generator. • Two dipole and nine quadrupole magnets without power supplies. • All necessary beam diagnostics (Faraday cups and luminescent screens). • All vacuum chambers and pumps. • All mechanical supports. For CRYRING as modified for FAIR and FLAIR • Ring magnets: dipole, quadrupole, sextupole, correction magnets with all power converters • Fast and slow beam injection and extraction systems consisting of two septum magnets, two fast kicker magnets, a fourfold electrostatic bumper system for multiturn injection, and an electrostatic septum for slow extraction together with all necessary power supplies except that for the injection septum magnet. The latter must be equipped with a pulsed current supply, if the magnetic rigidity of the injected ion beam is increased from 0.8 Tm to 1.4 Tm, as desirable for the injection of the ESR beam. • Acceleration system: drift tube and wide band rf-generator for a ramp rate of 1 T/s. • Electron cooler with all power supplies. • UHV components: vacuum chambers, valves, NEG and ion pumps, baking jackets, including replacement of old ones using ceramic paper. Ion pumps need to be equipped with new power supplies. • Beam diagnostics (faraday cups, fluorescent screens, electrostatic pick-ups, Schottky pickup, ac and dc beam current transformers, beam-profile monitors). • Cables as far as dismantling and transport are economically favorable. • All mechanical supports. MSL/SU has incurred also the liability for organizing and financing the disassembly and appropriate transport of all equipment to GSI. However, the participation by GSI staff members allocated for the later reinstallation seems to be reasonable. They could help to conserve UHV cleanliness during disassembly, to suitably mark items for later identification, and to protect sensitive parts from damage during transport. The CRYRING shall not be decomposed into small single components. Complete subsections (straight sections between bending magnets) of the ring could be transported after removal of cables and pipes. In this way, considerable re-assembly work time cost would be saved. In addition, in order to minimize the reinstallation cost, the technical infrastructure might be reused to a large extent. Cables between power converters and magnets, distribution lines and local connections for cooling water and pressurized air, shall be disassembled and transported in an appropriate way. 6.3. Preparation of the CRYRING Cave at GSI 6.3 23 Preparation of the CRYRING Cave at GSI The reinstallation of CRYRING is proposed behind the ESR with regard to the least possible interference with presently operating beam lines and experiments. In addition, the most southern part of the Target Hall will be the ideal location for the ring, when SIS18 and beam lines are shut down for a longer period in 2015 (at least for 1.5 years) in order to improve the extraction channel of SIS18 and construct the first part of the beam line to SIS100. Before modifying Cave B for the installation of CRYRING, the FOPI detector and the last part of the beam line have to be disassembled and cabling and piping for FOPI must be removed. For the heavy FOPI solenoid a suitable storage position must be found until its future employment is decided. Six air conditioned containers, in which detector electronics and experiment control of FOPI are installed, have to be removed to make room for the extended area of the nearly square CRYRING cave. Though the CRYRING will be operated with low intensity beams and generally at low, subthreshold ion energies, radiation shielding by means of concrete walls and covers is necessary. Regarding the maximum magnetic rigidity of 1.44 Tm, the energies for protons and light ions would be high enough for nuclear reactions with the implication of neutron production. For the sufficient concrete shield thickness of 0.8 m the extended CRYRING cave can be completely built by using supernumerous concrete wall and cover modules of Cave B, where the walls had to have a thickness of 2.4 m and the covers a thickness of 1.6 m, both consisting of 0.8 m thick modules. The ground floor of the extended CRYRING cave is shown in Figure 6.1 together with CRYRING and injection beam lines. It can be seen that the injection beam line from the ESR requires a new breakthrough in the northern concrete wall. The cave offers enough space to install the shortened low energy injector beam line completely inside the cave. The maximum permitted surface load of 500 kg/m2 of the 0.8 m thick concrete cover allows for arranging all necessary power supplies and electronics on the cave top. Three air conditioned containers will accommodate the sensitive accelerator and experiment electronics and a local control room (see Figure 6.2). 6.4 6.4.1 Preparation of the Technical Infrastructure Access Control The controlled access to Cave B can be employed with minor modifications for the new CRYRING cave. It is desirable if the access control could be switched to a local controlling mode when the CRYRING is operated as a stand-alone system. Maintaining the ion source and in-ring experiments would be much easier and less time consuming. Compared to the former safety concept, the new cave will require an additional emergency exit on the eastern side of the cave opposite to the normal access. 6.4.2 Cooling Water Fortunately the required flux of cooling water does not exceed the capacity of the existing cooling system. For the connection to the CRYRING and the water-cooled power converters and containers on the upper floor new pipes have to be installed. It may be possible to reuse the main ring pipe line and the connection to the components. 24 6.4.3 Chapter 6. Proposed Construction Cycle Electricity The extension area of the new cave requires the installation of additional lighting. It would be worthwhile to increase the brightness in the cave by means of coating the rough concrete surface with white paint. This would also improve the cleanliness in the cave with respect to the requirements during the opening and assembly of UHV components. The mains voltage distribution and 3-phase line connectors have to be installed along ring and beam lines. The total power loss of the installed heat jackets for the UHV baking system would require 210 kW. However, baking will be done partially, i.e. sector by sector. Therefore a line connection for a maximum consumption of about 100 kW in the cave will be sufficient. 6.4.4 Others The technical infrastructure of Cave B can be almost unchanged from its present configuration. The walls, where air conditioning and electric lighting are mounted, will not be dismantled. The same applies for the walls bearing the runways for two cranes, which are required for the transport of heavy loads inside the cave. The connection to the pressurized air and dry nitrogen systems is already available in the existing Cave B. The distribution in the new cave is only a small fraction of installation cost and activities. The planning of a false floor for the installation of the power converters will be done as soon as a detailed arrangement of the supplies has been worked out. It has to be investigated, whether an impounding basin for the cooling water will be necessary or not. The same is the case concerning the required impounding basin for the oil-filled transformers. Their position, inside or outside the Target Hall, on the upper or the ground floor, will be decided after working out the arrangement of all supplies. 6.5 Fast ESR Beam Ejection and Transport to CRYRING The CRYRING can be supplied with decelerated ions from the ESR. The option of decelerating ions to 4 MeV/u is routinely used in combination with the HITRAP decelerator which is designed for an injection energy of 4 MeV/u. The ESR cycle has been optimized for this extraction energy. As the operation of the ESR is flexible the beam can be decelerated to other energies as well. The beams which are available are highly charged stable ions, but also rare isotope beams from the fragment separator FRS can be injected and decelerated. An injection energy into the ESR of 400 MeV/u is favorably chosen in order to profit from the availability of stochastic cooling which is optimized for this energy. At this energy for all ions stripping to the bare charge state is achieved with high efficiency. For lower charge states the injection energy can be reduced. Cooling after injection at lower energies can be performed by electron cooling which is slower for hot beams, but has also been used in many ESR experiments and which results in even better condition for deceleration. The injection energy of 400 MeV/u is sufficiently high for the production and storage of rare isotope beams which need an even higher primary beam energy due to the use of thick production targets and the energy loss in the target. Independent of the injection energy the standard ESR deceleration cycle employs electron cooling at an intermediate level of 30 MeV/u. The cooling provides best conditions for efficient deceleration and the intermediate flat top in the magnetic cycle is used for changing the rf frequency from harmonic number h = 2 to h = 4. This change is necessary due to the limited frequency tuning range of the rf system. The deceleration to 4 MeV/u is done with harmonic number h = 4. At 4 MeV/u electron cooling is applied again in order cool the beam to small emittance and momentum spread which eases the transfer to a subsequent accelerator. 6.6. Completion of the CRYRING Components 25 A serious limitation for the preparations at the low energy originates from the short lifetime of highly charged ions which is caused by electron capture from the residual gas atoms. Lifetimes of a few seconds were observed for beams of highly charged ions at 4 MeV/u. The fast extraction from the ESR with a kicker magnet can be applied to a coasting or a bunched beam. The coasting beam results in losses determined by the rise time and the available flat top time of the kicker pulse. For HITRAP operation the second ESR cavity was modified so that it can be tuned to the revolution frequency of the circulating decelerated ions. Thus a single bunch is formed which can be significantly shorter than the ESR ring circumference. The bunching with h = 1 allows extraction from the ESR and injection into CRYRING with highest efficiency. The fast extraction, either of coasting or of a bunched beam, which was developed for HITRAP, would also be available for the transfer of decelerated ions to the CRYRING. The intensity of the cooled beam at low energy is limited by the space charge tune shift which is more pronounced for a bunched beam. On the other hand, as the space charge limit is virtually independent of the accelerator, it also applies to the CRYRING and therefore sets the limit for achievable beam intensities. Measurements of the coasting (unbunched) beam at 4 MeV/u showed a momentum spread of ∆p/p about 10−4 or better. Even with moderate bunching transverse emittances x,y smaller than or equal to 10−3 mm mrad were found. If the CRYRING is ready to accept particles at higher energy, the deceleration in the ESR can end at any energy between the intermediate energy of 30 MeV/u and the energy of 4 MeV/u. This will reduce losses in the ESR and shift the lifetime problem by electron capture from the residual gas to the CRYRING which is expected to perform even better due to its lower vacuum pressure. The transfer energy is not limited by the ESR performance, but by the bending power of the CRYRING magnets and the parameters of the CRYRING injection kicker. The parameters of this system are still under discussion as it is currently being manufactured. Operation with 4 MeV/u beams is in full accordance with the present specification, but operation up to the maximum bending power of the CRYRING which for bare ions corresponds to roughly 14 MeV/u is expected to work with the present kicker design. The ESR has already now achieved all parameters which are required to serve as a decelerator of heavy ions for CRYRING. The only modification which is needed is the installation of an additional fast kicker system. The CRYRING installation is planned south of the ESR, therefore the beam must be extracted towards the SIS Target Hall. The existing fast kicker cannot be used for extraction towards the south. A new kicker must be installed in the northern arc of the ESR. A position close to the existing magnetic and electrostatic septum would be favorable in order to adopt the same ion optics and extraction concept which is used for the slow extraction implemented in the ESR. The electronics and the power part for this new kicker can be salvaged from a previous diagnostics kicker which was dismounted a few years ago. Therefore only the kicker magnet and a new or modified vacuum chamber are needed. As the ion optical mode of the ESR would be the same as for slow extraction the matching of the beamline for the transport of the beam to CRYRING could be copied from the slow extraction mode. Slow extraction from the ESR was used down to energies of 11.9 MeV/u and the magnetic system was designed for decelerated beams. Consequently no difficulties in transporting low energy beam from the ESR to CRYRING are expected. 6.6 6.6.1 Completion of the CRYRING Components Magnets The new beam line from ESR can be assembled from existing magnets available at GSI: • Two 22.5◦ bending magnets, 26 Chapter 6. Proposed Construction Cycle • Six quadrupole magnets (types SQ010-SQ030), and • Two H/V steering magnets. All magnets are components of the beam distribution system behind the UNILAC designed for a maximum magnetic rigidity of 4.4 Tm. Hence they are well suited for the maximum value of 1.44 Tm rigidity of the beam from the ESR. It should be noted that the power consumption will be below 10% of the nominal values and the required amount of cooling water is correspondingly small. 6.6.2 Power Converters Power converters will have to be made available for all magnets of the two injection beam lines. Fortunately all required supplies are available at GSI, except a pulsed 2940 A supply for the injection septum magnet which has to be purchased from an industrial company. It is necessary for the injection of ions from the ESR at the maximum magnetic rigidity of 1.4 Tm. The power supplies for all ring and electron cooler magnets shall be reinstalled on the concrete cover of the new cave. The peak power of about 2.6 MVA for the operation of CRYRING with a ramp rate of 7 T/s requires a corresponding intermediate 20/10.5 kV transformer, if the existing oil-filled 10.5 kV/880–400 V transformer for silicon controlled rectifiers SCR application is used. The alternative solution of a new 20 kV/880–400 V dry transformer for SCR will be investigated later. 6.6.3 Beam Diagnostics From the discussion with MSL colleagues it is clear that the beam diagnostic equipment will not be ready for use ‘out of the box’, because of several reasons. • Data acquisition systems were in most cases purpose-built by MSL experts and GSI will not be able to service and maintain the devices. • Often the applied techniques are somewhat outdated (e.g. PC interfacing for residual gas ionization profile monitor) and will have to be renewed for future usability. • In general, the degree of control system integration is relatively low: only Faraday-cups and scintillating screens have interfaces to the control system at MSL. As a consequence, more or less the complete data acquisition part of the diagnostic systems has to be renewed, whereas the detectors and mechanics would remain unchanged wherever possible. Additionally, it is emphasized that no spare parts exist for the diagnostic components, which introduces some risk for future operation of the devices. It has to be mentioned that the replacement of the existing data acquisition (DAQ) systems with state-of-the-art techniques will consume the major part of the man power required for the commissioning of CRYRING beam diagnostics at GSI. The renewal of the DAQ is a project in its own and requires manpower for technical coordination, for adaptations of the existing hardware (digital and analog electronics), as well as for programming DAQ software. 6.6.4 Radio-Frequency Components 108.48 MHz RFQ and debuncher The 108.48 MHz end stage for the RFQ accelerator requires a new 2–5 kW solid state driver amplifier. The same type can be applied also to operate the debuncher cavity to reduce the momentum spread of the 300 keV/u RFQ beam from ±1% to ±0.5% in order to increase the efficiency of multiturn injection to CRYRING. Wideband drift tube The present wideband generator for the drift tube accelerating gap of CRYRING allows a dipole ramp rate of 1 T/s for acceleration or deceleration in the frequency 6.6. Completion of the CRYRING Components 27 range of 40 kHz to 2.4 MHz. With a sinusoidal waveform the 200 W generator produces 280 Vp−p into 50 Ω which a balloon transformer multiplies by 4, giving 1 kVp−p at the drift tube gaps. For higher ramping rates (4 T/s or 7 T/s) the gap voltage has to be increased proportional to dB/dt and the required RF power proportional to the square of dB/dt. 6.6.5 UHV For the remote control of vacuum sections and bakeout systems the existing MSL hardware can be adapted after some modification to the present GSI vacuum and interlock control. The cost for the control unit planned for FAIR is included in Section 7.2. CRYRING and Low-Energy Beam Line Although all vacuum chambers, beam pipes and pumps will be delivered by MSL, the material for the reassembly must be purchased: CF and Helicoflex gaskets, temperature resistant bolts and nuts, new non evaporable getter (NEG) material for 40 pumping units, cables etc. In addition, the HV supplies for 6–10 Varian ion pumps have to be replaced by new units. Mechanical pumps will be installed permanently only in the LE beam line near the ion source. The CRYRING itself will be evacuated by means of mobile turbopump units. We expect that a fraction of about 10% of the baking jackets will have to be replaced because of damage during disassembly and transport. Beam Line from ESR The missing vacuum sections of the beam line from the ESR have to be purchased. Only the magnets from the GSI pool are equipped with vacuum chambers (dipole magnets) or pipes (quadrupole and steering magnets). All other parts, valves, chambers for pumping and beam diagnostics, pipes with compensators, measuring systems and ion pumps have to be purchased if not available from the GSI pool. 6.6.6 CRYRING Control System The present CRYRING accelerator control system is in almost all aspects very different from the existing GSI control system as well as the control system under development for FAIR. As it is, it cannot be coherently integrated in the existing GSI control system framework. Taking into account that GSI fully focuses its activities and resources on the FAIR project, a comprehensive replacement of the CRYRING control system within the proposed time schedule (setting up the machine at ESR in the course of the year 2013) is unrealistic. Moreover, no technical support and maintenance to the original CRYRING control system can be provided by the Accelerator Controls Department (BEL). Consequently, this report proposes to initially set up and recommission CRYRING at GSI with its original control system with support by CRYRING experts from Sweden. However, a partial or full replacement of the control system after initial recommissioning is possible and would even provide excellent test opportunities for FAIR (see Chapter 5). Considering the installation of CRYRING at GSI, it was discussed and agreed with the technical experts, that it is not reasonable to move the present general IT infrastructure of the CRYRING control system (servers, active network equipment, and control room operator stations) to GSI. Instead, a new system environment shall be provided and installed by the GSI Controls department on which the CRYRING control system can be installed and configured by CRYRING experts from Sweden. 28 6.7 6.7.1 Chapter 6. Proposed Construction Cycle Assembly of CRYRING and Injection Beam Lines Preparation of Magnetic Components: Fiducialization As network measurements and final alignment are based on using Laser Trackers and Digital Levels about 55 magnetic components of the CRYRING and two injection beam lines have to be fiducialized before assembly. Fiducialization means that the magnetic axes, planes and effective centres of dipole, quadrupole or sextupole magnets have to be transferred to mechanical marks suitable for the final alignment during the assembly of beam lines and ring. As the alignment of 12 quadrupole magnets in the injection beam lines will be carried out by telescope, fiducialization of these components is not necessary and a 3D-determination of the actual condition w.r.t. the global coordinate system will not be possible. 6.7.2 Procurement of Mechanical Parts The procurement of about 200 additional mechanical supports is necessary for lifting the low energy injection beam line and the present beam axis of CRYRING from 1.5 m to 2.0 m which is the nominal height for ion beams in ESR and in the Target Hall. The material for the supports of the 20 m long new beam line from the high energy beam transport to the CRYRING is available from the pool of dismantled systems. 6.7.3 Assembly Survey Before starting the mechanical assembly the positions of all bending magnets (beam lines and CRYRING) have to be surveyed precisely. Position marks on the ground floor with an accuracy of ±0.5 mm will help to achieve a rather good positioning during the assembly work without the presence of the survey people. Assembly of CRYRING The assembly of the ring will be performed sector by sector. By this way assembled sectors can already be connected to power supplies and water cooling while others are still being mechanically assembled. Fine alignment of the ring can be done by means of laser tracking simultaneously to the mechanical assembly of the injection beam lines. Assembly of Injection Beam Lines The alignment of the beam lines will be done by applying conventional methods. Therefore three pillars with bearings for telescopes have to be surveyed in advance. Targets marking the axes of quadrupoles will allow fine adjustments to about ±0.5 mm accuracy. Suitable marks on the luminescent screens, applied for the determination of the ion beam axis, can be adjusted by this method to similar accuracy. 6.7. Assembly of CRYRING and Injection Beam Lines 29 Figure 6.1. Detailed view of proposed modification to Cave B with the installation of CRYRING@ESR. 30 Chapter 6. Proposed Construction Cycle Figure 6.2. Arrangement of power supplies and other technical installations for CRYRING on top of the modified Cave B roof. Chapter 7 Project Steering 7.1 Time Schedule The proposed time schedule of the CRYRING@ESR project is shown in Figure 7.1. The rather tight schedule is associated to the boundary conditions at the Manne-Siegbahn-Laboratory and at GSI/FAIR described in Section 6.1 which are repeated here once more: • The disassembly and removal of CRYRING has to be finished around the end of 2012. • The absolutely necessary technical support by experienced MSL staff members during reassembly and commissioning of the modified CRYRING at GSI will be available only during the coming two or three years. • The support by GSI staff from technical divisions (BES and GA) will be disposable only until middle of 2014. 2012 5 6 7 8 2013 9 10 11 12 1 2 3 4 5 6 7 2014 8 9 10 11 12 1 2 3 4 5 6 CRYRING@ESR (a study goup report) GSI board (May/June) FAIR board (June) FAIR council (Dec. 2nd) Clearing of Cave B area Disassembly of CRYRING at MSL Construction of CRYRING cave Transport of CRYRING to GSI Fast beam ejection at ESR Reassembly at ESR Commissioning with RFQ injector Commissioning with ESR beam First experiments Figure 7.1. Proposed time schedule for CRYRING@ESR under the boundary conditions described in Section 6.1 In order to meet the described conditions the project should be started without any delay within the coming 2 months. The most urgent decisions have to be made concerning both the dismantling of Cave B and the disassembly of the FOPI-detector, i.e. concerning the clearing of the Cave B area. A detailed MS project plan for disassembling CRYRING at MSL and 31 32 Chapter 7. Project Steering reassembling it in the Target Hall at GSI has been worked out already by the BES division, responsible for all mechanical work packages. The plan supposes that the start of the activities takes place in August 2012. 7.2 Cost and Manpower Requirements The cost and man power requirements for the realization of CRYRING@ESR were analyzed in detail. We have completed our analysis for two scenarios, a minimal solution and a FAIR compatible setup. A minimal solution adapts the ring mostly as it is to the GSI infrastructure. The cost estimate for the minimal solution is 1 190 k¤ and includes all work performed by external companies. Moreover, 290 man weeks for the installation need to be provided by GSI, i.e. its infrastructure divisions (about 7–8 man years). It shall be noted, that this estimate does not yet include the costs for installation and commissioning of the main ring magnet power supplies; there, negotiations with external companies are still ongoing. The FAIR compatible solution will require additional expenses of 717 k¤ and additional 197 man weeks. These additional expenses should be covered by the FAIR budget (for test benches and hardware commissioning). The majority of cost estimates are based on careful calculations by experts from technical divisions. Some items are still rough estimates, some may be too high and less expensive alternatives are under investigation by the EET division. 7.3 Project Structure: Installation and Operation For the installation of CRYRING at the ESR and finally for its operation, a dedicated project team is required. This team will be responsible for the organization, coordination, and physics performance of CRYRING@ESR (see Figure 7.2). During Organization Project Phasethe installation phase, it needs to Project Coordinator Ion Optics& Electron Cooling physicist** Ion Source & RFQ Injector Mechanics & UHV Beam Diagnostics & RF physicist engineer physicist Controls & Power Supplies physicist or engineer Cave Infrastructure & Safety physicist or engineer ** also deputy project coordinator Figure 7.2. Organisation chart for the project phase of CRYRING@ESR. (** also deputy project coordinator). act in close cooperation with the teams of GSI infrastructure and will coordinate in addition the support by external groups, such as by the colleagues from Sweden. After the building up phase, the project team will change its profile and takes over the responsibility for operation (Figure 7.3). Basically, the group members will nearly remain the same but their tasks will be directed towards operation, maintenance, and the demands of the FAIR project (test of novel beam diagnostics, controls etc.). Members of the atomic physics division will act as the core of the project team. Most of them are already involved into the HITRAP project and its commissioning. Since from physical and technical point of view HITRAP and CRYRING are closely entangled (both HITRAP and CRYRING are the central facilities within the FLAIR building), the merging of both projects appears to be evident. The time and resource planning for HITRAP need to be adjusted accordingly. The assignment of personnel as well as the use of 7.4. Possible Sources of Funding 33 Organization Commissioning & Operation Coordinator Operating & Experiments Ion Optics& Electron Cooling physicist** Ion Source & RFQ Injector Mechanics & UHV Beam Diagnostics & RF physicist engineer physicist Controls & Power Supplies physicist or engineer Cave Infrastructure & Safety physicist or engineer ** also deputy project coordinator Figure 7.3. Organisation chart for commissioning and operation of CRYRING@ESR. (** also deputy operating & experiment coordinator) available financial resources has to be redistributed in order to enable HITRAP and CRYRING but with the priority to accomplish the installation of CRYRING before mid of 2014. 7.4 Possible Sources of Funding In the following we list possible sources for funding of the CRYRING@ESR project. Once the project has been accepted, further sources of support will be investigated. • Merging of the HITRAP and the CRYRING project: Resources for investment and consumables will be redistributed accordingly. Man power for the project team will be provided by the atomic physics division. • Collaboration agreement between KVI and GSI. • Collaboration agreement between MPIK Heidelberg and GSI. • Offer by the University of Stockholm to support the installation of CRYRING by experienced personnel (in total up to two FTEs). • Stockholm University has recently offered an advanced internal gas target system for CRYRING experiments. • A team of Atomic Physicists from Chalmers University of Technology, Gothenburg and Stockholm University, as well as Nuclear Physicists from Chalmers and Lund University and Accelerator Physicists from Stockholm University and ESS, Lund, are preparing an application to the Knut & Alice Wallenberg Foundation for travel costs and stationing of personnel for extended periods of time at GSI/FAIR. • Application sent to the Council for Research Infrastructures in April 2012 by the board of SFAIR, the “umbrella organization” of Swedish scientists aiming for using FAIR further applications such as EU synergy grants. • Support by the Helmholtz-Institute Jena can be anticipated. 7.5 Swedish contributions to the installation of CRYRING@ESR The Manne Siegbahn Laboratory (MSL) at the Department of Physics, Stockholm University will mutatis mutandis fulfill the commitment as described in section 2.4 of the FLAIR LSR Technical Design Report [23]. In the changed perspective of a fast installation of CRYRING at ESR this would mean that MSL is responsible for the new hardware and modifications defined in the LSR, disassembling of the CRYRING and the transportation of it to GSI/FAIR in 34 Chapter 7. Project Steering Darmstadt in the beginning of 2013. It is planned that a small group from GSI will be invited by MSL to spend some months in Stockholm during the autumn 2012 to participate in the final disassembly and packing of the CRYRING in order to gain experience about the configuration of CRYRING before the disassembly. This experience would help considerably for an optimal reassembly of the ring at GSI. It should be remarked that the fact that the CRYRING is available intact and properly modified according to the requirements defined by the FLAIR collaboration has been accomplished by a large grant from the Swedish Research Council and by generous support from Stockholm University, both acknowledging the high scientific potential of the future use of the CRYRING at GSI/FAIR. The leader of the MSL team is the accelerator physicist Anders Källberg, who through the years has been responsible for the operation of the CRYRING at MSL. In addition to the CRYRING hardware described in the TDR, Stockholm University has recently offered an advanced internal gas target system for CRYRING experiments to be delivered with a ring. This opens new scientific opportunities which have attracted a substantial interest from physicists planning future experiments at CRYRING@ESR. After the transportation of CRYRING to Darmstadt, there are hitherto no formal commitments for a Swedish participation in its installation at the ESR. However Stockholm University offers that two experienced accelerator physicists, a highly qualified engineer, expert on the CRYRING Control System and a mechanical engineer will spend up to in total two person-years at GSI/FAIR. Dependent on the success of applications of further financial support from the Swedish Research Council (application sent to the Council for Research Infrastructures in April 2012 by the board of SFAIR, the “umbrella organization” of Swedish scientists aiming for using FAIR) and the Knut & Alice Wallenberg Foundation (see below), Swedish presence in the installation and commissioning work might be increased. 7.6 Swedish Participation in Experiments at FAIR: CRYRING@ESR The new exciting scientific opportunities that can be offered soon with an early installation of the CRYRING@ESR have stimulated Swedish scientists to plan for experiments at the new facility. A team of Atomic Physicists from Chalmers University of Technology, Gothenburg and Stockholm University, as well as Nuclear Physicists from Chalmers and Lund University and Accelerator Physicists from Stockholm University and ESS, Lund are preparing an application to the Knut & Alice Wallenberg Foundation for travel costs and stationing of personnel for extended periods of time at GSI/FAIR. Scientific issues that are planned to be addressed are within the areas: Atomic-ion collisions, Ion-photon collisions and nuclear and nuclear astrophysics experiments. An important part of the application is also positions for two postdoctoral researchers, who should work on 1. starting up research development on experiments and detectors with a focus on nuclear reactions and nuclear astrophysics and 2. ion-optical problems, in particular optimization of the transmission of radioactive beams into the ESR. The main applicant, PI, for the application to the Knut & Alice Wallenberg Foundation is Andreas Heinz, nuclear physicist at Chalmers University of Technology. Bibliography [1] FAIR. Green Paper: The Modularized Start Version. Tech. rep. Darmstadt: GSI, 2009. url: http : / / www . fair - center . de / fileadmin / fair / publications _ FAIR / FAIR _ GreenPaper_2009.pdf. [2] B. Franzke, H. Geissel, and G. Münzenberg. In: Mass Spectrometry Reviews 27.5 (2008), pp. 428–469. issn: 1098-2787. doi: 10.1002/mas.20173. [3] A. Gumberidze, T. Stöhlker, D. Banaś, et al. In: Phys. Rev. Lett. 94 (2005), p. 223001. doi: 10.1103/PhysRevLett.94.223001. [4] I. Klaft, S. Borneis, T. Engel, et al. In: Phys. Rev. Lett. 73 (1994), pp. 2425–2427. doi: 10.1103/PhysRevLett.73.2425. [5] C. Brandau, C. Kozhuharov, A. Müller, et al. In: Phys. Rev. Lett. 91.7 (2003), p. 073202. doi: 10.1103/PhysRevLett.91.073202. [6] M. Jung, F. Bosch, K. Beckert, et al. In: Phys. Rev. Lett. 69 (15 1992), pp. 2164–2167. doi: 10.1103/PhysRevLett.69.2164. [7] Y. A. Litvinov, F. Bosch, H. Geissel, et al. In: Phys. Rev. Lett. 99 (26 2007), p. 262501. doi: 10.1103/PhysRevLett.99.262501. [8] J. Eichler and T. Stöhlker. In: Phys. Reports 439 (2007), pp. 1–99. doi: 10.1016/j. physrep.2006.11.003. [9] D. Misra, H. T. Schmidt, M. Gudmundsson, et al. In: Phys. Rev. Lett. 102 (15 2009), p. 153201. doi: 10.1103/PhysRevLett.102.153201. [10] E. Vigren, M. Hamberg, V. Zhaunerchyk, et al. In: Astrophys. J. 709 (2010), pp. 1429– 1434. doi: 10.1088/0004-637X/709/2/1429. [11] I. Orban, S. D. Loch, S. Böhm, and R. Schuch. In: Astrophys. J. 721 (2010), pp. 1603– 1607. doi: 10.1088/0004-637X/721/2/1603. [12] E. Vigren, M. Hamberg, V. Zhaunerchyk, et al. In: Astrophys. J. 695.1 (2009), p. 317. doi: 10.1088/0004-637X/695/1/317. [13] H. T. Schmidt, D. Fischer, Z. Berenyi, et al. In: Phys. Rev. Lett. 101 (8 2008), p. 083201. doi: 10.1103/PhysRevLett.101.083201. [14] R. Schuch, E. Lindroth, S. Madzunkov, et al. In: Phys. Rev. Lett. 95 (2005), p. 183003. doi: 10.1103/PhysRevLett.95.183003. [15] H. T. Schmidt, A. Fardi, R. Schuch, et al. In: Phys. Rev. Lett. 89 (2002), p. 163201. doi: 10.1103/PhysRevLett.89.163201. [16] H.-J. Kluge, T. Beier, K. Blaum, et al. In: Adv. Quant. Chem. 53 (2008), p. 83. doi: 10.1016/S0065-3276(07)53007-8. [17] C. Brandau. unpublished. 35 36 BIBLIOGRAPHY [18] SPARC. Stored Particles Atomic Research Collaboration. url: http://www.gsi.de/ sparc. [19] FLAIR. Facility for Low-energy Antiproton and Ion Research. url: http : / / www . flairatfair.eu/. [20] EXL. EXotic nuclei studied in Light-ion induced reactions. url: http://www.rug.nl/ kvi/Research/hnp/Research/EXL/index. [21] ILIMA. Isomeric beams, LIfetimes and MAsses. url: http://www.fair- center.eu/ fair-users/experiments/nustar/experiments/ilima.html. [22] ELISe. ELectron-Ion Scattering Experiment. url: http://www.fair-center.eu/fairusers/experiments/nustar/experiments/elise.html. [23] H. Danared, G. Andler, M. Björkhage, et al. LSR - Low-energy Storage Ring. Technical Design Report. Version 1.3, May 6th 2011. Manne-Siegbahn Laboratory, Physics Department, Stockholm University, 2011. Appendix A Letters of Support Letters of Support for CRYRING@ESR were kindly provided by several international research groups and all storage ring collaborations of the FAIR project and are appended in the following: • KVI Groningen (pg. 38), • Institute of Modern Physics, Chinese Academy of Sciences (pg. 39), • the community of Austrian researchers (pg. 40), • Swedish FAIR Consortium (FAIR Sweden) (pg. 43). The storage ring collaborations at FAIR: • ELectron-Ion Scattering Experiment, ELISe collaboration (pg. 45), http://www.fair-center.eu/fair-users/experiments/nustar/experiments/elise. html • EXotic nuclei studied in Light-ion induced reactions, EXL collaboration (pg. 46), http://www.rug.nl/kvi/Research/hnp/Research/EXL/index • Facility for Low-energy Antiproton and Ion Research, FLAIR collaboration (pg. 47), http://www.flairatfair.eu/ • Isomeric beams, LIfetimes, and MAsses, ILIMA collaboration (pg. 48), http://www.fair-center.eu/fair-users/experiments/nustar/experiments/ilima. html • Stored Particles Atomic Physics Research Collaboration, SPARC collaboration (pg. 50). http://www.gsi.de/sparc 37 Prof. Dr. Horst Stöcker GSI Helmholtzzentrum für Schwerionenforschung GmbH Planckstr. 1 64291 Darmstadt Wien, 23.05.2012 Dear Prof. Stöcker, lieber Horst, Bearbeiter/in / Durchwahl / E-Mail we, members of the community of Austrian scientists interested in the research possible at FAIR, want to express our strong support for the recent initiative of installing the CRYRING accelerator at the ESR storage ring of GSI. This will open up the possibility to explore already now a part of the physics program of FLAIR with highly charged ions available from ESR and keep CRYRING in continuous operation until antiproton or higher intensity HCI beams from FAIR become available, for which CRYRING was originally foreseen. The FOPI experiment existing in the vicinity of ESR could then potentially be used to explore hadron physics with stopped antiprotons, which will be a unique feature of FLAIR. We think this current initiative will strengthen the interest and support of the physics communities in FLAIR and will allow a strong physics program to be carried out until the full FLAIR facility can be realized. Yours sincerely Prof. Eberhard Widmann Director, Stefan Meyer Institute Page 1 of 3 Prof. Dr. Eberhard Widmann, Director Eberhard.widmann@oeaw.ac.at Expression of support for CRYRING@ESR Univ.-Prof. Dipl.-Ing.Dr. Gerald BADUREK Dean of the Faculty of Physics Vienna University of Technology Univ.Prof. Dr. Friedrich Aumayr Institut f. Angewandte Physik Vienna University of Technology Univ.Prof. Dipl.-Ing. Dr.techn. Manfried Faber Atominstitut Vienna University of Technology Univ.Prof. Dipl.-Ing. Dr.techn. Helmut Leeb Atominstitut Vienna University of Technology Ass.Prof. Dipl.-Ing. Dr. Erwin Jericha Atominstitut Vienna University of Technology Page 2 of 3 2(2) timely implementation of major parts of the APPA-FLAIR facility, now in module 4, in a much earlier stage and could as well serve for research along the scientific lines of NUSTAR. The community represented by SFAIR is most supportive to these plans, and have or are underway to try to secure additional resources for their successful completion. Several research groups from Swedish universities have declared strong interest in using the CRYRING/ LSR set-up with beams from the ESR in the first phase for novel research program. Furthermore, key personnel from MSL will be made available from Stockholm University to support the mounting and commissioning of CRYRING/ LSR in the Target Hall at GSI. We emphasize that SFAIR sees the CRYRING/ LSR project as an important step to realize the storage ring physics program in a timely manner at FAIR. Chairperson, SFAIR c.c. T. Stöhlker, GSI B. Sharkov, FAIR G. Rosner, FAIR Organisations/VATnr: 202100-2932 GSI Helmholtzzentrum für Schwerionenforschung GmbH Planckstraße 1 64291 Darmstadt www.gsi.de GSI . Planckstraße 1 . 64291 Darmstadt . Deutschland Nuclear Reactions/Research Prof. Dr. Thomas Stöhlker Head of Department: Prof. Dr. Thomas Aumann Deputy: Dr. Haik Simon Phone +49 6159 71-2887 Fax +49 6159 71-2809 Mobile +49 1743281519 H.Simon@gsi.de Subject: CRYRING project: Letter of support from the ELISe collaboration May 20th, 2012 Dear Prof. Dr. Thomas Stöhlker, dear Thomas, I am writing this letter as the spokesperson of the ELISe collaboration and on behalf of the collaboration. I would like to express our full support and interest in the activities leading to the storage ring facility ESR and CRYRING@ESR, being initially coupled to the FRS and potentially later to the Super-FRS. Since ELISe is not included in the start-version of FAIR, the CRYRING@ESR facility provides excellent opportunities for test experiments and detector developments for the in-ring instrumentation of the ELISe setup. We are currently looking also into the opportunities for first installing the eA collider at the ESR with limited performance, keeping in mind that we’d be such already competitive with the upcoming SCRIT facility in Japan. In this context we welcome any activities and plans that allow for a vivid and strong nuclear physics programme at GSIs storage ring prior to the delayed realization of the NESR at FAIR. The realization of CRYRING@ESR would set an important corner stone immediately thrilling all experimental communities associated with the storage ring physics programme at FAIR. With kind regards, (Haik Simon) Geschäftsführung: Professor Dr. Dr. h.c. Horst Stöcker Dr. Hartmut Eickhoff Vorsitzende des Aufsichtsrates: Dr. Beatrix Vierkorn-Rudolph Stellvertreter: Ministerialdirigent Dr. Rolf Bernhardt Sitz: Darmstadt Amtsgericht Darmstadt HRB 1528 VAT-ID: DE 111 671 917 Landesbank Hessen/Thüringen BLZ 500 500 00 . Konto 50 01865 004 IBAN DE56 5005 0000 5001 8650 04 BIC HELA DE FF Prof. Dr. Horst Stöcker GSI Helmholtzzentrum für Schwerionenforschung GmbH Planckstr. 1 Gespeicherte und gekühlte Ionen Stored and Cooled Ions Prof. Dr. Klaus Blaum Tel: 06221-516 850/1 Fax: 06221-516 852 sekretariat.blaum@mpi-hd.mpg.de 64291 Darmstadt 25. April 2012 Dear Professor Stöcker, lieber Horst, On behalf of the FLAIR collaboration we would like to express our strong support for the CRYRING@ESR project, and we appreciate very much the future option of a connection to the Super-FRS. Since FLAIR is not included in the start-up version of FAIR, the CRYRING@ESR project provides excellent possibilities to pursue already some of our planned test experiments and detector tests, especially in view of the delay in the construction of the New Experimental Storage Ring (NESR), which is a mandatory ring for FLAIR. CRYRING@ESR will provide low energetic highly charged heavy ion beams, one of the main experimental programs of FLAIR, see the LSR-project within FLAIR. In addition, a continuous running of CRYRING and the installation of HITRAP at its final position will allow a fast and efficient start of the physics program of FLAIR@FAIR. In summary, we see the CRYRING@ESR installation as an excellent initiative towards the low-energetic storage ring projects at FAIR. With our best regards, KLAUS BLAUM Spokesperson of the FLAIR Collaboration EBERHARD WIDMANN Co-Spokesperson of the FLAIR Collaboration Professor H. Stöcker GSI, Darmstadt 4th May 2012 Dear Professor Stöcker, On behalf of the ILIMA collaboration, I would like to express strong support for the CRYRING@ESR project, with the future option of a connection to the Super-FRS. One of the main facilities for the ILIMA experimental program is the New Experimental Storage Ring (NESR), which is however outside the start-up version of FAIR. As has often been stressed, this significantly delays the realisation of the planned storage-ring experimental programs, and it could also cause irreversible negative consequences for the associated experimental communities. A novel possibility is now under consideration. Installation of the CRYRING coupled to the present ESR will extend the physics capabilities by enabling the production, in the near future, of highly ionized heavy ions at the lowest kinetic energies. This project has very high experimental discovery potential, including for ILIMA-related experiments. For instance, searching for the Nuclear Excitation by Electron Capture (NEEC) and the Nuclear Excitation by Electron Transition (NEET) phenomena will become possible. Therefore, we support an early construction of the CRYRING coupled to the ESR. It is important to emphasise that there is a future option which foresees the connection of the present ESR to the Super-FRS. This is extremely attractive for the ILIMA collaboration. It will enable the possibility of performing ILIMA experiments with cooled exotic ions in the ESR, with the highest secondary-beam intensities which will be available from the Super-FRS. This transitional arrangement would enable us to cover part of the ILIMA experimental program prior to the realisation of the NESR. Furthermore, the novel detector setups, which are foreseen for the NESR experiments, can be built and implemented for real physics experiments in the ESR under FAIR conditions, which will allow us to prepare in the best way for experiments in the NESR. Overall, we see the CRYRING@ESR as a very timely and important step towards the success of the storage-ring scientific program at FAIR. Yours sincerely, Phil Walker Spokesperson for the ILIMA Collaboration STOCKHOLM UNIVERSITY Physics Department Atomic Physics Division Prof. Dr. Reinhold Schuch May. 24. 2012 Subject: CRYRING@ESR, Letter of support from the SPARC collaboration To whom it may concern! I am writing this letter as spokesperson and on behalf of the SPARC collaboration. I would like to express our full support in this new FAIR related initiative of installing the CRYRING at the ESR of GSI. This project is an important and essential step towards the realization of our challenging anticipated physics progam at FAIR which concentrates on physics with stored and cooled heavy ions and rare isotopes. Although the storage ring branch of the FAIR project has an outstanding visibility due to its expected scientific impact, its major component, the NESR, has been postponed by an undefined amount of years. The realization of CRYRING at the ESR would compensate already now to a large extend for this loss and this combination of CRYRING with the ESR would bring the storage ring physics into Modularized Start Version of FAIR. In particular SPARC but also all the other collaborations that depend on storage rings would profit tremendously from this project and will keep them actively involved into FAIR. Finally, the SPARC collaboration is convinced that the scientific success of the CRYRING project at the ESR will promote the realization of the NESR and the FLAIR facility at the earliest possible date. I want to point out also, in view of the scientific merits of this initiative, the SPARC collaboration would contribute as much as possible to realize this important project. Yours sincerely Reinhold Schuch Spokesperson of the SPARC Collaboration Division of Atomic Physics Address: Physics Center FYSIKUM S-106 91 Stockholm Stockholm University Sweden Telephone: Nat. 08-55378621 Int. +46-8-55378621 Secr: E-mail addresses: +46-8-55378600 schuch@physto.se Fax +46-8-55378601 http://physto.se