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<strong>CRYRING@ESR</strong>:<br />

A study group report<br />

Darmstadt, July 26, 2012<br />

Michael Lestinsky 1 , Norbert Angert 1 , Ralph Bär 1 , Ralph Becker 1 , Mario Bevcic 1 , Udo Blell 1 ,<br />

Walter Bock 1 , Angela Bräuning-Demian 1 , Håkan Danared 2 , Oleksiy Dolinskyy 1 ,<br />

Wolfgang Enders 1 , Mats Engström 3 , Achim Fischer 1 , Bernhard Franzke 1 , Georg Gruber 1 ,<br />

Peter Hülsmann 1 , Anders Källberg 3 , Oliver Kester 1,4 , Carl-Michael Kleffner 1 ,<br />

Yuri A. Litvinov 1 , Carsten Mühle 1 , Bernhard Müller 1 , Ina Pschorn 1 , Torsten Radon 1 ,<br />

Heinz Ramakers 1 , Hartmut Reich-Sprenger 1 , Dag Reistad 3 , Galina Riefert 1 ,<br />

Marcus Schwickert 1 , Ansgar Simonsson 3 , Jan Sjöholm 3 , Örjan Skeppstedt 3 , Markus Steck 1 ,<br />

Thomas Stöhlker 1,5 , Wolfgang Vinzenz 1 , <strong>and</strong> Horst Welker 1<br />

1 GSI Helmholtzzentrum für Schwerionen<strong>for</strong>schung, 64291 Darmstadt, Germany<br />

2 European Spallation Source ESS, SE-221 00 Lund, Sweden<br />

3 Fysikum, Stockholm University, SE-106 91 Stockholm, Sweden<br />

4 Institut für Angew<strong>and</strong>te Physik, Goethe-Universität Frankfurt, 60438 Frankfurt a. M., Germany<br />

5 Helmholtz-Institut Jena, 07743 Jena, Germany


Contents<br />

Subject of this Study 5<br />

1 Introduction 7<br />

2 Scientific Motivation 9<br />

3 <strong>CRYRING@ESR</strong>: Location in the Target Hall at GSI 11<br />

4 <strong>CRYRING@ESR</strong>: List of Parameters 13<br />

5 CRYRING as Test Bench <strong>for</strong> FAIR 15<br />

5.1 St<strong>and</strong>-Alone Operation of CRYRING . . . . . . . . . . . . . . . . . . . . . . . . . 15<br />

5.2 Accelerator Controls . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15<br />

5.3 Beam Diagnostics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 17<br />

5.4 UHV Control <strong>and</strong> Interlock System . . . . . . . . . . . . . . . . . . . . . . . . . . 18<br />

5.5 Radiation Safety <strong>and</strong> Access Control System . . . . . . . . . . . . . . . . . . . . 18<br />

5.6 Controls <strong>for</strong> Technical Infrastructure . . . . . . . . . . . . . . . . . . . . . . . . . 18<br />

5.7 Preparation <strong>for</strong> FAIR Commissioning . . . . . . . . . . . . . . . . . . . . . . . . . 18<br />

5.7.1 Development <strong>and</strong> Test of Special Commissioning Software . . . . . . . . . 18<br />

5.7.2 Training of Operating Staff . . . . . . . . . . . . . . . . . . . . . . . . . . 19<br />

6 Proposed Construction Cycle 21<br />

6.1 Conditions <strong>for</strong> the Project Start . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21<br />

6.2 CRYRING Disassembly <strong>and</strong> Transport . . . . . . . . . . . . . . . . . . . . . . . . 22<br />

6.3 Preparation of the CRYRING Cave at GSI . . . . . . . . . . . . . . . . . . . . . 23<br />

6.4 Preparation of the Technical Infrastructure . . . . . . . . . . . . . . . . . . . . . 23<br />

6.4.1 Access Control . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 23<br />

6.4.2 Cooling Water . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 23<br />

6.4.3 Electricity . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 24<br />

6.4.4 Others . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 24<br />

6.5 Fast ESR Beam Ejection <strong>and</strong> Transport to CRYRING . . . . . . . . . . . . . . . 24<br />

6.6 Completion of the CRYRING Components . . . . . . . . . . . . . . . . . . . . . 25<br />

6.6.1 Magnets . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 25<br />

6.6.2 Power Converters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 26<br />

6.6.3 Beam Diagnostics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 26<br />

6.6.4 Radio-Frequency Components . . . . . . . . . . . . . . . . . . . . . . . . . 26<br />

6.6.5 UHV . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 27<br />

6.6.6 CRYRING Control System . . . . . . . . . . . . . . . . . . . . . . . . . . 27<br />

6.7 Assembly of CRYRING <strong>and</strong> Injection Beam Lines . . . . . . . . . . . . . . . . . 28<br />

6.7.1 Preparation of Magnetic Components: Fiducialization . . . . . . . . . . . 28<br />

3


4 CONTENTS<br />

6.7.2 Procurement of Mechanical Parts . . . . . . . . . . . . . . . . . . . . . . . 28<br />

6.7.3 Assembly . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 28<br />

7 Project Steering 31<br />

7.1 Time Schedule . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 31<br />

7.2 Cost <strong>and</strong> Manpower Requirements . . . . . . . . . . . . . . . . . . . . . . . . . . 32<br />

7.3 Project Structure: Installation <strong>and</strong> Operation . . . . . . . . . . . . . . . . . . . . 32<br />

7.4 Possible Sources of Funding . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 33<br />

7.5 Swedish contributions to the installation of <strong>CRYRING@ESR</strong> . . . . . . . . . . . 33<br />

7.6 Swedish Participation in Experiments at FAIR . . . . . . . . . . . . . . . . . . . 34<br />

Bibliography 35<br />

A Letters of Support 37


Subject of this study<br />

The Swedish in-kind contribution <strong>for</strong> FAIR includes the storage ring CRYRING, built by the<br />

Manne Siegbahn Laboratory in Stockholm. The international FAIR project has decided to accept<br />

this Swedish proposal as the central storage ring <strong>for</strong> the FLAIR facility <strong>for</strong> experiments with<br />

slow <strong>and</strong> even trapped anti-protons <strong>and</strong> exotic ions. Recently, in the context of the preparation<br />

of CRYRING <strong>for</strong> the transport to Darmstadt, which is expected to happen still within 2012,<br />

the idea was born to ask GSI to check <strong>for</strong> the option to install the CRYRING in the vicinity<br />

of the ESR storage ring inside the Target Hall. Such a project would closely be related to an<br />

early realization of the FLAIR facility not included into the Modularized Start Version of the<br />

FAIR project. The research with exotic ions as proposed <strong>for</strong> the FLAIR facility could already<br />

now being pursuit with this installation <strong>and</strong> at a later stage the extension to experiments with<br />

slow anti-protons would be possible on the basis of only moderate investments.<br />

Following the advice of the GSI scientific council <strong>and</strong> of the executive board of GSI, the<br />

atomic physics department of GSI has been assigned to <strong>for</strong>m a working group ∗ in order to come<br />

up with a proposal <strong>for</strong> installing CRYRING within the current Target Hall at GSI <strong>and</strong> provide<br />

a reliable estimate of the required resources to install CRYRING at ESR. The results obtained<br />

by this study group <strong>for</strong> both the resources needed as well as the possible location of CRYRING<br />

at GSI are described within the current document. In addition, a comprehensive overview of<br />

the physics opportunities which can be addressed by the combination of CRYRING <strong>and</strong> ESR<br />

will be given. Detailed description of physics cases is the subject of a dedicated “Physics Book:<br />

<strong>CRYRING@ESR</strong>”, the actual version of which is attached to this document. Since we still<br />

expect a considerable amount of additional contributions from various collaborations interested<br />

in the realization of <strong>CRYRING@ESR</strong>, the physics book is being continuously updated. Once<br />

completed, it is planned to publish “Physics Book: <strong>CRYRING@ESR</strong>” as a regular article in a<br />

peer-reviewed scientific journal. Moreover, we added a dedicated chapter “CRYRING as a Test<br />

Bench <strong>for</strong> FAIR” to emphasize the important <strong>and</strong> possibly even indispensable role of CRYRING<br />

as a test bench <strong>for</strong> many FAIR relevant accelerator related developments. There, emphasis is<br />

given to the operation of CRYRING as a st<strong>and</strong>-alone facility equipped with its own ion source<br />

<strong>and</strong> injector. The <strong>CRYRING@ESR</strong> is supported by various physics communities as well as by<br />

all FAIR storage ring collaborations which is reflected by dedicated support letters. The latter<br />

are attached to the Appendix of the current document.<br />

∗<br />

N. Angert, A. Bräuning-Demian, H. Danared, W. Enders, M. Engström,<br />

B. Franzke, A. Källberg, O. Kester, M. Lestinsky, Yu. A. Litvinov, D. Reistad,<br />

A. Simonsson, J. Sjöholm, M. Steck, <strong>and</strong> Th. Stöhlker<br />

5


6 CONTENTS


Chapter 1<br />

Introduction<br />

Storage ring experiments in the realm of atomic <strong>and</strong> nuclear physics with heavy ions <strong>and</strong> exotic<br />

nuclei contribute substantially to the success of the present GSI SIS18/ESR facility <strong>and</strong> <strong>for</strong>m<br />

one of the essential cornerstones of the future facility <strong>for</strong> antiproton <strong>and</strong> ion research FAIR. The<br />

corresponding experiments at FAIR are being prepared by the following international collaborations<br />

SPARC (Stored Particles Atomic Physics <strong>Research</strong> Collaboration), FLAIR (<strong>Facility</strong> <strong>for</strong><br />

Low-Energy <strong>Antiproton</strong> <strong>and</strong> <strong>Ion</strong> <strong>Research</strong>), ILIMA (Isomeric beams, LIfetimes, <strong>and</strong> MAsses),<br />

ELISE (ELectron-<strong>Ion</strong> Scattering Experiment), <strong>and</strong> EXL (EXotic nuclei studied in Light-ion induced<br />

reactions). The contributions by the Swedish <strong>and</strong> German partners in these collaborations<br />

are significant <strong>and</strong> indispensable. In the case of Sweden, the strong engagement is manifested by<br />

the provision of the Stockholm CRYRING facility as a Swedish in kind contribution <strong>for</strong> FAIR,<br />

where it will serve as the central storage ring installation within the FLAIR building. For this<br />

purpose substantial resources have already been invested to adapt CRYRING to its future role<br />

at FAIR. The delivery of CRYRING is expected to begin at the end of 2012.<br />

Because the new storage rings facilities are not part of the modularized start version (MSV)<br />

of the international FAIR project (because of the high civil construction cost <strong>for</strong> the storage<br />

ring complex NESR <strong>and</strong> FLAIR), it has been decided to maintain the operation of ESR —<br />

as documented by the Green Paper: The Modularized Start Version ∗ — in order to assure a<br />

persisting expertise in storage ring operation <strong>and</strong> physics <strong>and</strong> to allow substantial R&D work<br />

related to FAIR <strong>and</strong> in particular to FLAIR. Since CRYRING will be delivered to FAIR by the<br />

end of this year, the question needs to be answered is to what extent can CRYRING already<br />

be installed at the existing GSI Target Hall or, alternatively, whether it should be stored in<br />

containers <strong>for</strong> the next decade or longer.<br />

In view of FAIR, the operation of CRYRING at the existing ESR facility would exhibit<br />

various important advantages:<br />

• CRYRING as a FAIR test facility could be essential <strong>for</strong> FAIR relevant R&D projects, in<br />

particular with respect to accelerator related developments of instrumentation <strong>and</strong> controls:<br />

beam diagnostics, detector development, synchronization, efficient coupling of accelerators<br />

<strong>and</strong> storage rings, software development etc. Keeping in mind that there will be<br />

a break of at least 1.5 years in SIS18 operation, CRYRING would play a very important<br />

role by using it as a st<strong>and</strong>-alone facility.<br />

• CRYRING will help secure expertise of the personnel by providing otherwise not available<br />

training opportunities.<br />

• CRYRING would open novel <strong>and</strong> unique physics opportunities with large discovery potential<br />

<strong>and</strong> it would allow the existing storage ring collaborations connected to FAIR to<br />

continue.<br />

7


8 Chapter 1. Introduction<br />

Moreover, the mid <strong>and</strong> long term physics perspectives of <strong>CRYRING@ESR</strong> are exciting.<br />

Once the MSV of FAIR is accomplished, a transfer beamline <strong>for</strong> anti-protons <strong>and</strong> exotic nuclei<br />

from the CR to the ESR-CRYRING storage ring complex can be considered. In this way two<br />

fully commissioned storage rings, ESR <strong>and</strong> CRYRING, would be available at a very early stage<br />

<strong>for</strong> experiments using slow anti-protons at FAIR. Additionally, the experiments in the research<br />

areas of nuclear- (EXL, ELISe, ILIMA) <strong>and</strong> hadron physics will profit from this scenario using<br />

rare isotope beams from the FRS/ESR facility <strong>and</strong> later on from the FAIR accelerator chain.<br />

There<strong>for</strong>e, in view of both the MSV as well as the full version of the FAIR project, installing<br />

CRYRING at ESR already now has the potential to save considerable resources. It will provide<br />

a plat<strong>for</strong>m <strong>for</strong> prototyping FAIR technologies which is inevitably required <strong>and</strong> will consequently<br />

minimize the amount of time typically needed <strong>for</strong> the commissioning of these complex storagering<br />

facilities.<br />

∗<br />

Green paper [1]: “All these developments are also of particular relevance <strong>for</strong> future<br />

prospects of the SPARC physics programme which concentrates on storage rings <strong>and</strong><br />

traps, <strong>and</strong> will become possible with Module 4. For the realization of this programme<br />

the ESR storage ring <strong>and</strong> the HITRAP facility need to be maintained in operation<br />

at GSI until they shall be surpassed by Module 4.”


Chapter 2<br />

Scientific Motivation<br />

In the following we concentrate on the ion part of the physics program to be addressed at<br />

<strong>CRYRING@ESR</strong>. It will cover to a large extent the research with ions as proposed <strong>for</strong> the<br />

FLAIR facility (module 4 of the MSV). Note, at a later stage only a moderate investment <strong>for</strong> a<br />

transfer beam line would be required to transport anti-protons to CRYRING via the ESR <strong>and</strong><br />

to per<strong>for</strong>m the anticipated FLAIR experiments with slow or even trapped anti-protons.<br />

The exploration of the unique properties of stored <strong>and</strong> cooled beams as provided by heavy<br />

ion storage rings has opened novel <strong>and</strong> fascinating research opportunities in the realm of atomic<br />

<strong>and</strong> nuclear physics research. For the particular case of the ESR storage ring, this has been<br />

demonstrated in experiments addressing e.g. the 1s Lamb shift in heavy ions, the hyperfine<br />

splitting in hydrogen-like heavy atoms, the investigation of dielectronic recombination in heavy,<br />

few-electron ions, direct mass measurements of short-lived radionuclides or by studying rare<br />

nuclear decay modes such as the bound-state β-decay or the orbital electron capture decay [2–7].<br />

World-wide, ESR is the only storage ring that provides access to all naturally occurring elements<br />

up to the most extreme case of fully stripped uranium. Charge states <strong>and</strong> energies (4 MeV/u<br />

to 500 MeV/u) can be tailored according to the requirements of the experiment [8]. Moreover,<br />

intense beams of highly charged in-flight synthesized radioisotopes are at the experimentalist’s<br />

disposition. Likewise, CRYRING was operated at the Manne-Siegbahn Laboratory (MSL) in<br />

Stockholm with great success [9–15] however with much lighter ions or heavy ions of lower charge<br />

state.<br />

CRYRING is optimized <strong>for</strong> operation in an ion energy range of ∼ 14 MeV/u down to<br />

300 keV/u or lower. Both rings, ESR <strong>and</strong> CRYRING operate in complementary ion energy<br />

ranges, <strong>and</strong> CRYRING thus bridges the gap between the lowest stable operation of ESR (∼<br />

4 MeV/u) <strong>and</strong> the HITRAP facility [16] with highly charged ions close to or even at rest whereby<br />

preserving the high luminosity, characteristic <strong>for</strong> stored ion beams. Moreover, <strong>for</strong> the low energy<br />

regime below 10 MeV/u, the properties of CRYRING along with its instrumentation have<br />

several advantages compared to ESR such as its compactness <strong>and</strong> the excellent UHV vacuum<br />

conditions of < 10 −11 mbar. By combining ESR <strong>and</strong> CRYRING, the entire energy range from<br />

500 MeV/u almost down to rest will be available <strong>for</strong> experiments dealing with intense beams of<br />

highly charged ions <strong>and</strong> exotic nuclei.<br />

<strong>CRYRING@ESR</strong> will be the only facility world-wide that provides low-energy highly charged<br />

stable beams <strong>and</strong> beams of rare isotopes with a free choice of the charge state, including bare ions.<br />

Radioisotopes synthesized in a target after SIS18 can be purified from unwanted contaminants<br />

either with the present fragment separator FRS or alternatively directly in the ESR by employing<br />

its high resolving power [16, 17]. Of particular scientific interest are stable ions <strong>and</strong> artificially<br />

synthesized nuclides dressed with few electrons or fully stripped. In such elementary ionic<br />

systems the physics topic under investigation is not masked or hampered by many-body effects<br />

9


10 Chapter 2. Scientific Motivation<br />

or unwanted spectator electrons. The interpretation of the experiments is thus straight<strong>for</strong>ward<br />

<strong>and</strong> without ambiguity. In addition, the inverse processes of many fundamental atomic <strong>and</strong><br />

nuclear reaction <strong>and</strong> decay mechanisms only become experimentally accessible if corresponding<br />

vacancies in the atomic shell are available. Examples of these inverse effects include radiative<br />

recombination (inverse of photoeffect), dielectronic capture (inverse of autoionization), bound<br />

state beta decay (inverse of nuclear electron capture, EC) or nuclear excitation by electron<br />

capture (inverse of internal conversion).<br />

Low-energy phase space of cooled ions provide extremely well-defined experimental conditions<br />

<strong>for</strong> precision spectroscopy experiments (electrons, ions, <strong>and</strong> photons). At the same time,<br />

compared to ions at rest, orders of magnitude higher luminosity in collision experiments using<br />

low-energy ions in a storage ring is achieved due to the repeated interaction of the stored ion<br />

beam with a target (gas, free electrons, laser). These luminosities may be comparable to or even<br />

exceed those obtainable in single-pass fixed-target experiments while the dilute targets induce<br />

only a minimum amount of angular <strong>and</strong> energy straggling which can be compensated by beam<br />

cooling <strong>and</strong> guarantee <strong>for</strong> single collision conditions.<br />

For atomic collision studies, another appealing aspect is the very strong perturbation to<br />

the target atoms due to the impact of the slow highly charged ions with conditions far from<br />

equilibrium. CRYRING operates in a particular interesting energy range <strong>for</strong> nuclear reactions,<br />

that is at the Coulomb barrier <strong>and</strong> in the astrophysically relevant Gamow window of p- <strong>and</strong> rpprocesses<br />

of nucleosynthesis. The swift low-energy beam also makes the detection <strong>and</strong> monitoring<br />

of primary <strong>and</strong> secondary ions either in a destructive manner with particle detectors or in a<br />

non-destructive manner down to the level of single particles by means of Schottky techniques<br />

experimentally much easier. Hereby, the storage ring itself serves as a high-resolution magnetic<br />

heavy ion spectrometer. The dynamic range that is covered with the various experimental<br />

techniques covers the span from single stored ions, detected by means of Schottky noise analysis<br />

up to beams at the space charge limit.<br />

As stated in a previous section, the capabilities <strong>for</strong> future research on atomic, nuclear,<br />

<strong>and</strong> astrophysics with a combined CRYRING <strong>and</strong> ESR facility will be outlined in a dedicated<br />

“Physics book: <strong>CRYRING@ESR</strong>” which is in preparation. The current draft of the physics<br />

book is appended to this document. Moreover, since by the installation of <strong>CRYRING@ESR</strong><br />

a substantial part of the heavy ion program as <strong>for</strong>eseen at FAIR <strong>for</strong> NESR <strong>and</strong> FLAIR can<br />

already be addressed, we also like to refer to the already positively evaluated physics programs<br />

as described in the FAIR documents of the contributing collaborations (SPARC [18], FLAIR<br />

[19], EXL [20], ILIMA [21], <strong>and</strong> ELISe [22]).


Chapter 3<br />

<strong>CRYRING@ESR</strong>: Location in the Target<br />

Hall at GSI<br />

For a cost efficient solution of <strong>CRYRING@ESR</strong>, utilizing existing space, technical installation,<br />

<strong>and</strong> ion beamlines is m<strong>and</strong>atory. A suitable location <strong>for</strong> setting up CRYRING at GSI can<br />

be found at Cave B, which is almost ideal. We illustrate the envisaged realization of CRY-<br />

RING@ESR in Figure 3.1. Cave B is located downstream of ESR <strong>and</strong> a transport beam line <strong>for</strong><br />

ions is presently available. Further, the cave is of the required size which means required construction<br />

changes could be per<strong>for</strong>med without interfering with other experimental installations.<br />

Modifications to the cave construction can be done at moderate cost, as this essentially requires<br />

only moving available concrete blocks. However, the technical infrastructure <strong>and</strong> facilities, such<br />

as cooling water, electricity, or air conditioning, have to be adapted to the requirements of<br />

CRYRING along with its beamlines.<br />

11


12 Chapter 3. <strong>CRYRING@ESR</strong>: Location in the Target Hall at GSI<br />

Figure 3.1. The proposed topology <strong>for</strong> <strong>CRYRING@ESR</strong> in the Target Hall of GSI. Several options<br />

<strong>for</strong> a reassembly of CRYRING have been investigated. We propose locating the setup in Cave B<br />

as the least invasive <strong>and</strong> most cost efficient solution. The modified CRYRING with injection beam<br />

lines is shown with blue lines. See also Figure 6.1 <strong>for</strong> a detailed view of the modified Cave B.


Chapter 4<br />

<strong>CRYRING@ESR</strong>: List of Parameters<br />

A detailed description of CRYRING (LSR) <strong>for</strong>eseen <strong>for</strong> the operation with antiprotons as<br />

planned <strong>for</strong> the envisioned program of the FLAIR collaboration has been given within the<br />

TDR “LSR - Low-energy Storage Ring” [23]. In the following we summarize the CRYRING<br />

parameters as they are relevant <strong>for</strong> the operation with heavy ions at the current SIS/ESR facility<br />

(Table 4.1). In addition, the most important in-ring installations as they are required <strong>for</strong><br />

experiments are given below:<br />

• Electron cooler<br />

• Internal jet target<br />

• Transversal electron target<br />

• Collinear laser setups<br />

• Schottky pickups<br />

• Particle counters<br />

• Recoil ion, electron, <strong>and</strong> photon spectrometers<br />

Table 4.1. CRYRING parameters as they are relevant <strong>for</strong> the operation with heavy ions at the<br />

current SIS/ESR facility.<br />

Circumference<br />

51.63 m<br />

Rigidity at injection <strong>for</strong> ions (antiprotons, protons) 1.44 Tm (0.80 Tm)<br />

Highest possible injection energy <strong>for</strong> ¯p, p<br />

30 MeV<br />

— <strong>for</strong> 12 C 6+ 24.7 MeV/u<br />

— <strong>for</strong> 238 U 92+ ( 238 U 89+ ) 14.8 MeV/u (13.9 MeV/u)<br />

Lowest rigidity<br />

0.054 Tm<br />

Lowest energy<br />

charge exchange limited<br />

Magnet ramping (deceleration <strong>and</strong> acceleration) 7 T/s, 4 T/s, or 1 T/s<br />

Vacuum pressure (N 2 equiv.)<br />

10 −11 –10 −12 mbar<br />

Beam injection<br />

multi-turn <strong>and</strong> fast<br />

Beam extraction<br />

slow <strong>and</strong> fast<br />

<strong>Ion</strong> sources <strong>for</strong> st<strong>and</strong>-alone operation yes (300 keV/u, q/A > 0.25)<br />

13


14 Chapter 4. <strong>CRYRING@ESR</strong>: List of Parameters


Chapter 5<br />

CRYRING as Test Bench <strong>for</strong> FAIR<br />

5.1 St<strong>and</strong>-Alone Operation of CRYRING<br />

As described in Chapter 3 the installation of CRYRING in the Target Hall in combination with<br />

the fragment separator (FRS) <strong>and</strong> the Experimental Storage Ring (ESR) would represent an<br />

attractive, novel facility <strong>for</strong> atomic <strong>and</strong> nuclear physics experiments. But CRYRING would<br />

also offer an ideal opportunity <strong>for</strong> testing important technical developments <strong>for</strong> FAIR under<br />

operating conditions. These tests could be per<strong>for</strong>med even during longer shut down periods<br />

of SIS18, i.e. without beam from ESR. This is because CRYRING has its own injector <strong>and</strong>,<br />

there<strong>for</strong>e, can be operated as a st<strong>and</strong>-alone system. The low energy RFQ injector delivers ions<br />

with charge-to-mass ratio q/A ≥ 0.25 at a fixed specific energy of 0.3 MeV/u. The ion beam<br />

can be pulsed with repetition frequencies up to 5 Hz <strong>and</strong> pulse lengths smaller or equal 0.5 ms.<br />

Similar to SIS18, multiturn injection is applied to attain higher circulating beam currents.<br />

The st<strong>and</strong>-alone operation would preferably be applied <strong>for</strong> the commissioning of CRYRING<br />

after the completion of the ring assembly <strong>and</strong> the successful commissioning of all ring systems<br />

without ESR beam.<br />

For the test of FAIR technologies <strong>and</strong> components the use of the RFQ-injector seems to be<br />

the most suitable mode of operation. Test times would be available without any interference<br />

with the time-limited operation of the existing accelerators. There<strong>for</strong>e, CRYRING could operate<br />

during the long shutdown period of about 18 months expected around the year 2015 <strong>and</strong> required<br />

<strong>for</strong><br />

• linking the proton linac building to the injection channel TK of SIS18,<br />

• modification of the extraction channel of SIS18,<br />

• installation of the first part of the beam transport from SIS18 to SIS100, <strong>and</strong><br />

• major upgrade work on the main control room.<br />

According to these considerations CRYRING would be an excellent, if not indispensable test<br />

bench <strong>for</strong> many important developments <strong>and</strong> technologies <strong>for</strong> FAIR. Its relevance <strong>for</strong> the success<br />

of the FAIR project with respect to time schedule <strong>and</strong> quality of operation is briefly discussed<br />

in the following.<br />

5.2 Accelerator Controls<br />

Though CRYRING is not part of the FAIR modularized start version an installation at ESR<br />

would provide excellent possibilities <strong>for</strong> the controls <strong>and</strong> other technical departments to implement,<br />

test, deploy <strong>and</strong> evaluate the operational experience <strong>for</strong> improvements of the technical<br />

systems <strong>for</strong> FAIR. While it was always <strong>for</strong>eseen to implement FAIR control system solutions<br />

with the existing GSI machines (SIS18, ESR), CRYRING would provide even better conditions<br />

15


16 Chapter 5. CRYRING as Test Bench <strong>for</strong> FAIR<br />

<strong>for</strong> following reasons:<br />

• A new stack of control system solutions <strong>for</strong> FAIR can be implemented <strong>and</strong> tested without<br />

ensuring full compatibility <strong>and</strong> coherency with the existing control system at any time<br />

during development. Some of the new control system design principles <strong>for</strong> FAIR are<br />

fundamentally different from the present GSI system (e.g. new beam <strong>and</strong> cycle concept,<br />

replacement of the Virtual Accelerator concept by a more general <strong>and</strong> flexible one). With<br />

CRYRING, these new solutions can be tested in an almost isolated environment in a system<br />

comprising almost all kinds of accelerator systems (ion source, linear accelerator, beam<br />

lines, synchrotron <strong>and</strong> storage ring) <strong>and</strong> without the constraints <strong>and</strong> having to reimplement<br />

specific GSI functionality of the existing system (e.g. therapy mode, equipment status<br />

concept, etc.).<br />

• CRYRING as a st<strong>and</strong>-alone machine can provide more machine development time <strong>for</strong> control<br />

system <strong>and</strong> equipment tests with much less organizational overhead than at UNILAC,<br />

SIS, <strong>and</strong> ESR.<br />

• The present GSI accelerator chain will experience a strongly reduced operation time in the<br />

coming years (e.g. 3–4 months of operation per year only) <strong>and</strong> machine time <strong>for</strong> control<br />

system tests will be quite limited. Machine operation times will be highly dedicated to<br />

machine development (MD) activities as well as detector tests <strong>for</strong> FAIR. Since beam time<br />

will be rare, a very stable <strong>and</strong> reliable control system is essential. This situation would be<br />

in contradiction with the strategy to implement novel solutions <strong>and</strong> evaluate them during<br />

longer runs. New solutions cannot provide the same level of robustness <strong>and</strong> availability<br />

from the beginning on. It is to be expected that failures will occur. The opportunity of<br />

dedicated MD runs at an independent ion beam facility will allow to solve <strong>and</strong> fix these<br />

rollout problems with a minimal disruption of the precious beam time operation of the<br />

GSI accelerators.<br />

Practically, the strategy of the controls department would be as follows: Many of the control<br />

system solutions needed <strong>for</strong> CRYRING modification are necessary <strong>for</strong> FAIR anyway. These are<br />

presently already under development or will be developed in the course of the FAIR project.<br />

These include front-end software equipment classes, generic operator applications, timing system,<br />

setting generation software, etc. It is expected that these solutions can be adapted to<br />

CRYRING with only moderate ef<strong>for</strong>t. As soon as these solutions are available, they can be<br />

implemented in CRYRING <strong>for</strong> tests. First activities would be to implement the new control<br />

system environment designed <strong>for</strong> FAIR in parallel to the CRYRING installation. This environment<br />

will be the base <strong>for</strong> all control system components including those of the beam diagnostics<br />

<strong>and</strong> available <strong>for</strong> component <strong>and</strong> integration tests.<br />

Deeper underst<strong>and</strong>ing <strong>and</strong> more investigation of the present CRYRING control system is<br />

needed to determine which subsystems can be replaced by corresponding FAIR developments.<br />

The following list indicates some examples:<br />

Equipment control <strong>for</strong> power converters with DC, pulsed <strong>and</strong> ramped operation. The<br />

FAIR St<strong>and</strong>ard Control Unit SCU with respective Front End St<strong>and</strong>ard Architecture FESA<br />

equipment class developments is the adequate solution. Controller prototypes <strong>and</strong> engineering<br />

samples under development <strong>for</strong> FAIR can be used.<br />

Timing system would be replaced by the facility-wide new General Machine Timing system.<br />

Modifications to the timing system are needed anyway <strong>for</strong> beam transfer from ESR. Bunch<br />

to bucket transfer can be implemented <strong>and</strong> studied <strong>for</strong> the bunch transfer from SIS18 to


5.3. Beam Diagnostics 17<br />

SIS100 as well as from SIS100 to CR <strong>and</strong> from CR to HESR <strong>for</strong> both the proton/antiproton<br />

<strong>and</strong> the radioactive ion beams.<br />

Setting generation system can be implemented based on the LHC St<strong>and</strong>ard Architecture<br />

LSA framework as an example <strong>for</strong> a storage ring machine. Tests of the overall storage ring<br />

functionality are possible. Feedback from the users would be highly valuable.<br />

Generic operator control applications under development <strong>for</strong> FAIR can be reused <strong>for</strong> FAIR<br />

<strong>and</strong> valuable operator feedback can be collected <strong>and</strong> used <strong>for</strong> improvements. Functions<br />

of remote monitoring <strong>and</strong> manage control authority domains (main control room, local<br />

control room) can be tested.<br />

Using CRYRING <strong>for</strong> FAIR development tests will result in reduced commissioning ef<strong>for</strong>t<br />

<strong>and</strong> time <strong>for</strong> the control system once the FAIR machines need to be commissioned. Moreover,<br />

early testing allows <strong>for</strong> better <strong>and</strong> more stable solutions <strong>and</strong> well tested operator application<br />

programs.<br />

In spite of all these benefits with respect to time <strong>and</strong> money savings, the control system<br />

solutions <strong>for</strong> FAIR cannot be implemented <strong>and</strong> tested in CRYRING without any additional<br />

financial ef<strong>for</strong>t <strong>and</strong> manpower. Technical coordination <strong>and</strong> necessary software adaptations will<br />

require one fulltime position being assigned to the controls department as early as possible<br />

after a positive management decision to implement <strong>CRYRING@ESR</strong>. A potential c<strong>and</strong>idate has<br />

already been identified by the Atomic Physics department. For necessary electronic hardware<br />

adaptations, the vocational trainee group (Ausbildungsgruppe) in the controls department as<br />

well as the young technicians having completed their traineeship would be highly interested to<br />

get involved <strong>and</strong> contribute as well.<br />

Without further investigations <strong>and</strong> decisions about which subsystems to be replaced by FAIR<br />

solutions, only some rough cost estimates are given in Section 7.2. However, it can be assumed<br />

that <strong>for</strong> most dedicated hardware components of the control system prototypes <strong>and</strong> engineering<br />

samples of the FAIR developments could be used at no additional costs.<br />

5.3 Beam Diagnostics<br />

A great part of the work necessary <strong>for</strong> the CRYRING beam diagnostics could be eased by<br />

applying soft- <strong>and</strong> hardware techniques <strong>for</strong>eseen <strong>for</strong> the FAIR project. All data acquisition<br />

(DAQ) systems, i.e. analog <strong>and</strong> digital electronics, controllers, digitizers, infrastructure systems<br />

etc., as well as the required software, should unconditionally apply FAIR st<strong>and</strong>ards, like FESA<br />

(Front-End Software Architecture) compatibility. Important: DAQ <strong>for</strong> beam diagnostics is part<br />

of the German in-kind contribution (EoI 13i) <strong>for</strong> FAIR. The GSI beam diagnostics department<br />

will deliver the complete set of DAQ systems <strong>for</strong> FAIR <strong>and</strong> has strong interest in using CRYRING<br />

as a test bench <strong>for</strong> ongoing hardware <strong>and</strong> software development projects.<br />

This strategy has the advantages of using CRYRING as a test bench <strong>for</strong> FAIR <strong>and</strong> the<br />

reusability of work load. The results obtained during CRYRING commissioning <strong>and</strong> test runs<br />

will confirm the development concepts <strong>and</strong>, in this way, improve the preparations <strong>for</strong> FAIR.<br />

The required manpower <strong>and</strong> budget <strong>for</strong> the FAIR-type realization of the CRYRING beam diagnostics<br />

will certainly entail additional expenses over a minimum cost/equipment solution (see<br />

Section 7.2) but these can be justified in view of the opportunity <strong>for</strong> testing new FAIR equipment<br />

under ‘live’ conditions.


18 Chapter 5. CRYRING as Test Bench <strong>for</strong> FAIR<br />

5.4 UHV Control <strong>and</strong> Interlock System<br />

The vacuum controls shall be realized as an industrial control system based on Siemens SIMATIC<br />

PLC <strong>and</strong> a commercial SCADA (Supervisory Control <strong>and</strong> Data Acquisition) product in connection<br />

with the UNICOS (UNified Industrial COntrol System) framework introduced at CERN<br />

<strong>for</strong> the control of the LHC cryogenics. All devices are connected directly to the PLC <strong>and</strong> thus<br />

render a very robust solution. It is being developed <strong>and</strong> delivered as in-kind contribution by the<br />

FAIR member state Slovenia.<br />

It would be favorable to implement <strong>and</strong> operate a vacuum control installation early be<strong>for</strong>e<br />

implementing it in FAIR machines. Evaluation of the complete system <strong>and</strong> training of the<br />

vacuum group staff would be possible this way. CRYRING provides all necessary vacuum<br />

control aspects, including a bakeout system. The additional cost <strong>for</strong> the FAIR vacuum controls<br />

is included in Section 7.2.<br />

5.5 Radiation Safety <strong>and</strong> Access Control System<br />

The CRYRING Cave-B could be removed from existing ZKS system <strong>and</strong> replaced by an early<br />

installation of the FAIR PSS (personnel safety system). New access gate infrastructure technology<br />

<strong>and</strong> procedures could be tested <strong>and</strong> optimized in order to implement a well-tested system<br />

later with the FAIR buildings.<br />

5.6 Controls <strong>for</strong> Technical Infrastructure<br />

The development of instrumentation <strong>and</strong> control technology will be necessary in order to control<br />

<strong>and</strong> optimize the supply of various FAIR facilities with electricity, cooling <strong>and</strong> other auxiliary<br />

media. For instance, the flow reduction of cooling water or cooling air <strong>for</strong> facilities st<strong>and</strong>ing idle<br />

would considerably reduce the required load on the cooling systems. A similar consideration<br />

would probably offer a chance <strong>for</strong> minimizing the capacity of the electricity installations.<br />

The new control systems could be tested also at the CRYRING at a time when no other<br />

accelerators <strong>and</strong> experiments are in operation.<br />

5.7 Preparation <strong>for</strong> FAIR Commissioning<br />

Practical experience from earlier accelerator projects shows that, as far as possible, it must<br />

be avoided to finally test <strong>and</strong> commission accelerator components <strong>and</strong> control system at the<br />

same time as the commissioning with ion beams takes place. Precious beam time would be lost<br />

<strong>for</strong> time consuming trouble shouting especially of controls software <strong>and</strong> hardware components.<br />

It is without any controversy that, compared to the regular operation, the commissioning of<br />

accelerators usually causes considerably higher dem<strong>and</strong>s on both the control system <strong>and</strong> the<br />

operating staff.<br />

5.7.1 Development <strong>and</strong> Test of Special Commissioning Software<br />

The presently practiced commissioning concept at the existing accelerator system at GSI requires<br />

to a large extend the intervention of experienced accelerator physicists <strong>and</strong> engineers. The<br />

approach to optimal machine settings is done by many steps of human interpretation of beam<br />

diagnostic measurements <strong>and</strong> subsequent comm<strong>and</strong>s to the controls software to suitably change<br />

settings. Not only the extremely tight time schedule <strong>for</strong> the commissioning of the new FAIR<br />

facilities but also the requirements of a highly efficient operation with time sharing between


5.7. Preparation <strong>for</strong> FAIR Commissioning 19<br />

different ion species <strong>and</strong> energies <strong>for</strong> several beam users necessitate the development of a novel<br />

commissioning concept. The required new software should assume the interpretation of beam<br />

diagnostics as well as many of the human interventions. By this way, the commissioning time<br />

would be reduced considerably. For the necessary extensive tests of the new commissioning<br />

concept the st<strong>and</strong>-alone operation of CRYRING offers ideal conditions, independent of shutdown<br />

times <strong>for</strong> the existing machines.<br />

5.7.2 Training of Operating Staff<br />

At least of comparable importance as development <strong>and</strong> test of operating software is the extensive<br />

training of the operating staff with respect to the commissioning phase of FAIR. The st<strong>and</strong>alone<br />

operation of CRYRING covers nearly all relevant aspects of an accelerator facility: ion<br />

source, beam transport, linear accelerator, bunch-to-bucket transfer or multiturn injection to a<br />

synchrotron/storage ring, beam acceleration or deceleration in the ring, beam cooling <strong>and</strong> finally<br />

slow <strong>and</strong> fast beam extraction. Insofar, CRYRING must be considered an necessary complement<br />

of the FAIR project


20 Chapter 5. CRYRING as Test Bench <strong>for</strong> FAIR


Chapter 6<br />

Proposed Construction Cycle<br />

6.1 Conditions <strong>for</strong> the Project Start<br />

For the installation of CRYRING on the GSI site the following conditions must be met:<br />

Formal Agreement upon CRYRING installation at GSI: The construction cycle described<br />

in the following presumes that a decision on the installation of CRYRING at GSI will<br />

be available by the end of July 2012.<br />

CRYRING disassembly by end of 2012: The CRYRING has to be disassembled <strong>and</strong> the<br />

components have to be moved out of the building presently occupied by the Manne-<br />

Siegbahn Laboratory of the Stockholm University (MSL/SU) by the end of 2012. As<br />

the reinstallation of the ring in the planned FLAIR facility has been defined as a part of<br />

the Swedish in-kind contribution to the FAIR project with a validation of 2 Million Euro,<br />

it has to be decided very speedily, how to proceed with the ring components. Since FLAIR<br />

is not a part of the Modularized Start Version (MSV) of FAIR, a storage concept worked<br />

out by the MSL <strong>for</strong>esees the storage of the CRYRING components over a period of 10<br />

years in 12 dehumidified containers on a site defined by the FAIR GmbH.<br />

An alternative solution is presented here. It considers the prompt reinstallation <strong>and</strong> operation<br />

of CRYRING at GSI as the experimental device <strong>and</strong> test facility behind the Experimental<br />

Storage Ring ESR. This will allow to realize the science options of FAIR <strong>and</strong><br />

FLAIR at a much earlier stage as compared to the realization of the modules 4 <strong>and</strong> 5 of<br />

the MSV.<br />

Support by MSL/SU: There is strong interest on the Swedish side, i.e. by the present<br />

MSL/SU staff <strong>and</strong> by atomic <strong>and</strong> nuclear physics groups, to built up <strong>and</strong> operate the<br />

CRYRING facility as modified <strong>for</strong> FAIR <strong>and</strong> FLAIR physics experiments in the near<br />

future instead. Its long term storage in containers <strong>for</strong> more then ten years is not recommended.<br />

The MSL/SU experts expressed their intent to support the reinstallation as well<br />

as the commissioning of CRYRING at GSI. However, this support will be available only<br />

if the reinstallation <strong>and</strong> the commissioning could take place within the next two or three<br />

years.<br />

Weak interference with FAIR: The envisaged period <strong>for</strong> the reinstallation <strong>and</strong> commissioning<br />

of CRYRING at GSI in the years 2013–2014 does not interfere with the necessary work<br />

<strong>for</strong> FAIR. There is a marginal involvement of the design <strong>and</strong> planning capacities. For the<br />

installation of the necessary technical systems <strong>and</strong> the reassembly of the CRYRING the<br />

human resources seem to be available until the first components <strong>for</strong> FAIR will be delivered<br />

21


22 Chapter 6. Proposed Construction Cycle<br />

in the 2nd half of 2014 <strong>and</strong> many acceptance tests have to be prepared <strong>and</strong> per<strong>for</strong>med. At<br />

this time the commissioning of the <strong>CRYRING@ESR</strong> facility should already be finished <strong>and</strong><br />

first experiments could be accomplished by operating the facility under the responsibility<br />

of the Atomic Physics (AP) department.<br />

6.2 CRYRING Disassembly <strong>and</strong> Transport<br />

According to the LSR-TDR (Danared et al. [23]), the MSL/SU will deliver the following items:<br />

For the Low energy injection beam line<br />

• An ion source plat<strong>for</strong>m <strong>for</strong> singly charged ions, with all power supplies including a 90 ◦<br />

analysing magnet without power supply.<br />

• Electrostatic quadrupole doublets <strong>and</strong> triplets with HV-supplies.<br />

• An RFQ accelerator with 108.48 MHz rf-generator including a 108.48 MHz debuncher<br />

cavity without rf-generator.<br />

• Two dipole <strong>and</strong> nine quadrupole magnets without power supplies.<br />

• All necessary beam diagnostics (Faraday cups <strong>and</strong> luminescent screens).<br />

• All vacuum chambers <strong>and</strong> pumps.<br />

• All mechanical supports.<br />

For CRYRING as modified <strong>for</strong> FAIR <strong>and</strong> FLAIR<br />

• Ring magnets: dipole, quadrupole, sextupole, correction magnets with all power converters<br />

• Fast <strong>and</strong> slow beam injection <strong>and</strong> extraction systems consisting of two septum magnets,<br />

two fast kicker magnets, a fourfold electrostatic bumper system <strong>for</strong> multiturn injection,<br />

<strong>and</strong> an electrostatic septum <strong>for</strong> slow extraction together with all necessary power supplies<br />

except that <strong>for</strong> the injection septum magnet. The latter must be equipped with a pulsed<br />

current supply, if the magnetic rigidity of the injected ion beam is increased from 0.8 Tm<br />

to 1.4 Tm, as desirable <strong>for</strong> the injection of the ESR beam.<br />

• Acceleration system: drift tube <strong>and</strong> wide b<strong>and</strong> rf-generator <strong>for</strong> a ramp rate of 1 T/s.<br />

• Electron cooler with all power supplies.<br />

• UHV components: vacuum chambers, valves, NEG <strong>and</strong> ion pumps, baking jackets, including<br />

replacement of old ones using ceramic paper. <strong>Ion</strong> pumps need to be equipped with<br />

new power supplies.<br />

• Beam diagnostics (faraday cups, fluorescent screens, electrostatic pick-ups, Schottky pickup,<br />

ac <strong>and</strong> dc beam current trans<strong>for</strong>mers, beam-profile monitors).<br />

• Cables as far as dismantling <strong>and</strong> transport are economically favorable.<br />

• All mechanical supports.<br />

MSL/SU has incurred also the liability <strong>for</strong> organizing <strong>and</strong> financing the disassembly <strong>and</strong><br />

appropriate transport of all equipment to GSI. However, the participation by GSI staff members<br />

allocated <strong>for</strong> the later reinstallation seems to be reasonable. They could help to conserve UHV<br />

cleanliness during disassembly, to suitably mark items <strong>for</strong> later identification, <strong>and</strong> to protect<br />

sensitive parts from damage during transport.<br />

The CRYRING shall not be decomposed into small single components. Complete subsections<br />

(straight sections between bending magnets) of the ring could be transported after removal of<br />

cables <strong>and</strong> pipes. In this way, considerable re-assembly work time cost would be saved. In<br />

addition, in order to minimize the reinstallation cost, the technical infrastructure might be<br />

reused to a large extent. Cables between power converters <strong>and</strong> magnets, distribution lines <strong>and</strong><br />

local connections <strong>for</strong> cooling water <strong>and</strong> pressurized air, shall be disassembled <strong>and</strong> transported<br />

in an appropriate way.


6.3. Preparation of the CRYRING Cave at GSI 23<br />

6.3 Preparation of the CRYRING Cave at GSI<br />

The reinstallation of CRYRING is proposed behind the ESR with regard to the least possible<br />

interference with presently operating beam lines <strong>and</strong> experiments. In addition, the most southern<br />

part of the Target Hall will be the ideal location <strong>for</strong> the ring, when SIS18 <strong>and</strong> beam lines are<br />

shut down <strong>for</strong> a longer period in 2015 (at least <strong>for</strong> 1.5 years) in order to improve the extraction<br />

channel of SIS18 <strong>and</strong> construct the first part of the beam line to SIS100.<br />

Be<strong>for</strong>e modifying Cave B <strong>for</strong> the installation of CRYRING, the FOPI detector <strong>and</strong> the<br />

last part of the beam line have to be disassembled <strong>and</strong> cabling <strong>and</strong> piping <strong>for</strong> FOPI must be<br />

removed. For the heavy FOPI solenoid a suitable storage position must be found until its<br />

future employment is decided. Six air conditioned containers, in which detector electronics <strong>and</strong><br />

experiment control of FOPI are installed, have to be removed to make room <strong>for</strong> the extended<br />

area of the nearly square CRYRING cave.<br />

Though the CRYRING will be operated with low intensity beams <strong>and</strong> generally at low, subthreshold<br />

ion energies, radiation shielding by means of concrete walls <strong>and</strong> covers is necessary.<br />

Regarding the maximum magnetic rigidity of 1.44 Tm, the energies <strong>for</strong> protons <strong>and</strong> light ions<br />

would be high enough <strong>for</strong> nuclear reactions with the implication of neutron production. For<br />

the sufficient concrete shield thickness of 0.8 m the extended CRYRING cave can be completely<br />

built by using supernumerous concrete wall <strong>and</strong> cover modules of Cave B, where the walls had<br />

to have a thickness of 2.4 m <strong>and</strong> the covers a thickness of 1.6 m, both consisting of 0.8 m thick<br />

modules.<br />

The ground floor of the extended CRYRING cave is shown in Figure 6.1 together with<br />

CRYRING <strong>and</strong> injection beam lines. It can be seen that the injection beam line from the ESR<br />

requires a new breakthrough in the northern concrete wall. The cave offers enough space to<br />

install the shortened low energy injector beam line completely inside the cave.<br />

The maximum permitted surface load of 500 kg/m 2 of the 0.8 m thick concrete cover allows<br />

<strong>for</strong> arranging all necessary power supplies <strong>and</strong> electronics on the cave top. Three air conditioned<br />

containers will accommodate the sensitive accelerator <strong>and</strong> experiment electronics <strong>and</strong> a local<br />

control room (see Figure 6.2).<br />

6.4 Preparation of the Technical Infrastructure<br />

6.4.1 Access Control<br />

The controlled access to Cave B can be employed with minor modifications <strong>for</strong> the new CRY-<br />

RING cave. It is desirable if the access control could be switched to a local controlling mode<br />

when the CRYRING is operated as a st<strong>and</strong>-alone system. Maintaining the ion source <strong>and</strong> in-ring<br />

experiments would be much easier <strong>and</strong> less time consuming.<br />

Compared to the <strong>for</strong>mer safety concept, the new cave will require an additional emergency<br />

exit on the eastern side of the cave opposite to the normal access.<br />

6.4.2 Cooling Water<br />

Fortunately the required flux of cooling water does not exceed the capacity of the existing<br />

cooling system. For the connection to the CRYRING <strong>and</strong> the water-cooled power converters<br />

<strong>and</strong> containers on the upper floor new pipes have to be installed. It may be possible to reuse<br />

the main ring pipe line <strong>and</strong> the connection to the components.


24 Chapter 6. Proposed Construction Cycle<br />

6.4.3 Electricity<br />

The extension area of the new cave requires the installation of additional lighting. It would<br />

be worthwhile to increase the brightness in the cave by means of coating the rough concrete<br />

surface with white paint. This would also improve the cleanliness in the cave with respect to<br />

the requirements during the opening <strong>and</strong> assembly of UHV components.<br />

The mains voltage distribution <strong>and</strong> 3-phase line connectors have to be installed along ring<br />

<strong>and</strong> beam lines. The total power loss of the installed heat jackets <strong>for</strong> the UHV baking system<br />

would require 210 kW. However, baking will be done partially, i.e. sector by sector. There<strong>for</strong>e<br />

a line connection <strong>for</strong> a maximum consumption of about 100 kW in the cave will be sufficient.<br />

6.4.4 Others<br />

The technical infrastructure of Cave B can be almost unchanged from its present configuration.<br />

The walls, where air conditioning <strong>and</strong> electric lighting are mounted, will not be dismantled.<br />

The same applies <strong>for</strong> the walls bearing the runways <strong>for</strong> two cranes, which are required <strong>for</strong> the<br />

transport of heavy loads inside the cave.<br />

The connection to the pressurized air <strong>and</strong> dry nitrogen systems is already available in the<br />

existing Cave B. The distribution in the new cave is only a small fraction of installation cost<br />

<strong>and</strong> activities.<br />

The planning of a false floor <strong>for</strong> the installation of the power converters will be done as<br />

soon as a detailed arrangement of the supplies has been worked out. It has to be investigated,<br />

whether an impounding basin <strong>for</strong> the cooling water will be necessary or not. The same is the<br />

case concerning the required impounding basin <strong>for</strong> the oil-filled trans<strong>for</strong>mers. Their position,<br />

inside or outside the Target Hall, on the upper or the ground floor, will be decided after working<br />

out the arrangement of all supplies.<br />

6.5 Fast ESR Beam Ejection <strong>and</strong> Transport to CRYRING<br />

The CRYRING can be supplied with decelerated ions from the ESR. The option of decelerating<br />

ions to 4 MeV/u is routinely used in combination with the HITRAP decelerator which is designed<br />

<strong>for</strong> an injection energy of 4 MeV/u. The ESR cycle has been optimized <strong>for</strong> this extraction energy.<br />

As the operation of the ESR is flexible the beam can be decelerated to other energies as well.<br />

The beams which are available are highly charged stable ions, but also rare isotope beams<br />

from the fragment separator FRS can be injected <strong>and</strong> decelerated. An injection energy into<br />

the ESR of 400 MeV/u is favorably chosen in order to profit from the availability of stochastic<br />

cooling which is optimized <strong>for</strong> this energy. At this energy <strong>for</strong> all ions stripping to the bare<br />

charge state is achieved with high efficiency. For lower charge states the injection energy can be<br />

reduced. Cooling after injection at lower energies can be per<strong>for</strong>med by electron cooling which<br />

is slower <strong>for</strong> hot beams, but has also been used in many ESR experiments <strong>and</strong> which results in<br />

even better condition <strong>for</strong> deceleration. The injection energy of 400 MeV/u is sufficiently high<br />

<strong>for</strong> the production <strong>and</strong> storage of rare isotope beams which need an even higher primary beam<br />

energy due to the use of thick production targets <strong>and</strong> the energy loss in the target.<br />

Independent of the injection energy the st<strong>and</strong>ard ESR deceleration cycle employs electron<br />

cooling at an intermediate level of 30 MeV/u. The cooling provides best conditions <strong>for</strong> efficient<br />

deceleration <strong>and</strong> the intermediate flat top in the magnetic cycle is used <strong>for</strong> changing the rf<br />

frequency from harmonic number h = 2 to h = 4. This change is necessary due to the limited<br />

frequency tuning range of the rf system. The deceleration to 4 MeV/u is done with harmonic<br />

number h = 4. At 4 MeV/u electron cooling is applied again in order cool the beam to small<br />

emittance <strong>and</strong> momentum spread which eases the transfer to a subsequent accelerator.


6.6. Completion of the CRYRING Components 25<br />

A serious limitation <strong>for</strong> the preparations at the low energy originates from the short lifetime<br />

of highly charged ions which is caused by electron capture from the residual gas atoms. Lifetimes<br />

of a few seconds were observed <strong>for</strong> beams of highly charged ions at 4 MeV/u.<br />

The fast extraction from the ESR with a kicker magnet can be applied to a coasting or a<br />

bunched beam. The coasting beam results in losses determined by the rise time <strong>and</strong> the available<br />

flat top time of the kicker pulse. For HITRAP operation the second ESR cavity was modified<br />

so that it can be tuned to the revolution frequency of the circulating decelerated ions. Thus a<br />

single bunch is <strong>for</strong>med which can be significantly shorter than the ESR ring circumference. The<br />

bunching with h = 1 allows extraction from the ESR <strong>and</strong> injection into CRYRING with highest<br />

efficiency. The fast extraction, either of coasting or of a bunched beam, which was developed<br />

<strong>for</strong> HITRAP, would also be available <strong>for</strong> the transfer of decelerated ions to the CRYRING.<br />

The intensity of the cooled beam at low energy is limited by the space charge tune shift<br />

which is more pronounced <strong>for</strong> a bunched beam. On the other h<strong>and</strong>, as the space charge limit<br />

is virtually independent of the accelerator, it also applies to the CRYRING <strong>and</strong> there<strong>for</strong>e sets<br />

the limit <strong>for</strong> achievable beam intensities. Measurements of the coasting (unbunched) beam at<br />

4 MeV/u showed a momentum spread of ∆p/p about 10 −4 or better. Even with moderate<br />

bunching transverse emittances ɛ x,y smaller than or equal to 10 −3 mm mrad were found.<br />

If the CRYRING is ready to accept particles at higher energy, the deceleration in the ESR can<br />

end at any energy between the intermediate energy of 30 MeV/u <strong>and</strong> the energy of 4 MeV/u. This<br />

will reduce losses in the ESR <strong>and</strong> shift the lifetime problem by electron capture from the residual<br />

gas to the CRYRING which is expected to per<strong>for</strong>m even better due to its lower vacuum pressure.<br />

The transfer energy is not limited by the ESR per<strong>for</strong>mance, but by the bending power of the<br />

CRYRING magnets <strong>and</strong> the parameters of the CRYRING injection kicker. The parameters of<br />

this system are still under discussion as it is currently being manufactured. Operation with<br />

4 MeV/u beams is in full accordance with the present specification, but operation up to the<br />

maximum bending power of the CRYRING which <strong>for</strong> bare ions corresponds to roughly 14 MeV/u<br />

is expected to work with the present kicker design.<br />

The ESR has already now achieved all parameters which are required to serve as a decelerator<br />

of heavy ions <strong>for</strong> CRYRING. The only modification which is needed is the installation of an<br />

additional fast kicker system. The CRYRING installation is planned south of the ESR, there<strong>for</strong>e<br />

the beam must be extracted towards the SIS Target Hall. The existing fast kicker cannot be<br />

used <strong>for</strong> extraction towards the south. A new kicker must be installed in the northern arc of the<br />

ESR. A position close to the existing magnetic <strong>and</strong> electrostatic septum would be favorable in<br />

order to adopt the same ion optics <strong>and</strong> extraction concept which is used <strong>for</strong> the slow extraction<br />

implemented in the ESR. The electronics <strong>and</strong> the power part <strong>for</strong> this new kicker can be salvaged<br />

from a previous diagnostics kicker which was dismounted a few years ago. There<strong>for</strong>e only the<br />

kicker magnet <strong>and</strong> a new or modified vacuum chamber are needed.<br />

As the ion optical mode of the ESR would be the same as <strong>for</strong> slow extraction the matching<br />

of the beamline <strong>for</strong> the transport of the beam to CRYRING could be copied from the slow<br />

extraction mode. Slow extraction from the ESR was used down to energies of 11.9 MeV/u<br />

<strong>and</strong> the magnetic system was designed <strong>for</strong> decelerated beams. Consequently no difficulties in<br />

transporting low energy beam from the ESR to CRYRING are expected.<br />

6.6 Completion of the CRYRING Components<br />

6.6.1 Magnets<br />

The new beam line from ESR can be assembled from existing magnets available at GSI:<br />

• Two 22.5 ◦ bending magnets,


26 Chapter 6. Proposed Construction Cycle<br />

• Six quadrupole magnets (types SQ010-SQ030), <strong>and</strong><br />

• Two H/V steering magnets.<br />

All magnets are components of the beam distribution system behind the UNILAC designed <strong>for</strong><br />

a maximum magnetic rigidity of 4.4 Tm. Hence they are well suited <strong>for</strong> the maximum value of<br />

1.44 Tm rigidity of the beam from the ESR. It should be noted that the power consumption will<br />

be below 10% of the nominal values <strong>and</strong> the required amount of cooling water is correspondingly<br />

small.<br />

6.6.2 Power Converters<br />

Power converters will have to be made available <strong>for</strong> all magnets of the two injection beam lines.<br />

Fortunately all required supplies are available at GSI, except a pulsed 2940 A supply <strong>for</strong> the<br />

injection septum magnet which has to be purchased from an industrial company. It is necessary<br />

<strong>for</strong> the injection of ions from the ESR at the maximum magnetic rigidity of 1.4 Tm.<br />

The power supplies <strong>for</strong> all ring <strong>and</strong> electron cooler magnets shall be reinstalled on the concrete<br />

cover of the new cave. The peak power of about 2.6 MVA <strong>for</strong> the operation of CRYRING with a<br />

ramp rate of 7 T/s requires a corresponding intermediate 20/10.5 kV trans<strong>for</strong>mer, if the existing<br />

oil-filled 10.5 kV/880–400 V trans<strong>for</strong>mer <strong>for</strong> silicon controlled rectifiers SCR application is used.<br />

The alternative solution of a new 20 kV/880–400 V dry trans<strong>for</strong>mer <strong>for</strong> SCR will be investigated<br />

later.<br />

6.6.3 Beam Diagnostics<br />

From the discussion with MSL colleagues it is clear that the beam diagnostic equipment will<br />

not be ready <strong>for</strong> use ‘out of the box’, because of several reasons.<br />

• Data acquisition systems were in most cases purpose-built by MSL experts <strong>and</strong> GSI will<br />

not be able to service <strong>and</strong> maintain the devices.<br />

• Often the applied techniques are somewhat outdated (e.g. PC interfacing <strong>for</strong> residual gas<br />

ionization profile monitor) <strong>and</strong> will have to be renewed <strong>for</strong> future usability.<br />

• In general, the degree of control system integration is relatively low: only Faraday-cups<br />

<strong>and</strong> scintillating screens have interfaces to the control system at MSL.<br />

As a consequence, more or less the complete data acquisition part of the diagnostic systems has<br />

to be renewed, whereas the detectors <strong>and</strong> mechanics would remain unchanged wherever possible.<br />

Additionally, it is emphasized that no spare parts exist <strong>for</strong> the diagnostic components, which<br />

introduces some risk <strong>for</strong> future operation of the devices.<br />

It has to be mentioned that the replacement of the existing data acquisition (DAQ) systems<br />

with state-of-the-art techniques will consume the major part of the man power required <strong>for</strong> the<br />

commissioning of CRYRING beam diagnostics at GSI. The renewal of the DAQ is a project<br />

in its own <strong>and</strong> requires manpower <strong>for</strong> technical coordination, <strong>for</strong> adaptations of the existing<br />

hardware (digital <strong>and</strong> analog electronics), as well as <strong>for</strong> programming DAQ software.<br />

6.6.4 Radio-Frequency Components<br />

108.48 MHz RFQ <strong>and</strong> debuncher The 108.48 MHz end stage <strong>for</strong> the RFQ accelerator requires<br />

a new 2–5 kW solid state driver amplifier. The same type can be applied also to operate the<br />

debuncher cavity to reduce the momentum spread of the 300 keV/u RFQ beam from ±1% to<br />

±0.5% in order to increase the efficiency of multiturn injection to CRYRING.<br />

Wideb<strong>and</strong> drift tube The present wideb<strong>and</strong> generator <strong>for</strong> the drift tube accelerating gap of<br />

CRYRING allows a dipole ramp rate of 1 T/s <strong>for</strong> acceleration or deceleration in the frequency


6.6. Completion of the CRYRING Components 27<br />

range of 40 kHz to 2.4 MHz. With a sinusoidal wave<strong>for</strong>m the 200 W generator produces 280<br />

V p−p into 50 Ω which a balloon trans<strong>for</strong>mer multiplies by 4, giving 1 kV p−p at the drift tube<br />

gaps. For higher ramping rates (4 T/s or 7 T/s) the gap voltage has to be increased proportional<br />

to dB/dt <strong>and</strong> the required RF power proportional to the square of dB/dt.<br />

6.6.5 UHV<br />

For the remote control of vacuum sections <strong>and</strong> bakeout systems the existing MSL hardware can<br />

be adapted after some modification to the present GSI vacuum <strong>and</strong> interlock control. The cost<br />

<strong>for</strong> the control unit planned <strong>for</strong> FAIR is included in Section 7.2.<br />

CRYRING <strong>and</strong> Low-Energy Beam Line Although all vacuum chambers, beam pipes <strong>and</strong><br />

pumps will be delivered by MSL, the material <strong>for</strong> the reassembly must be purchased: CF<br />

<strong>and</strong> Helicoflex gaskets, temperature resistant bolts <strong>and</strong> nuts, new non evaporable getter (NEG)<br />

material <strong>for</strong> 40 pumping units, cables etc. In addition, the HV supplies <strong>for</strong> 6–10 Varian ion<br />

pumps have to be replaced by new units.<br />

Mechanical pumps will be installed permanently only in the LE beam line near the ion source.<br />

The CRYRING itself will be evacuated by means of mobile turbopump units. We expect that a<br />

fraction of about 10% of the baking jackets will have to be replaced because of damage during<br />

disassembly <strong>and</strong> transport.<br />

Beam Line from ESR The missing vacuum sections of the beam line from the ESR have to be<br />

purchased. Only the magnets from the GSI pool are equipped with vacuum chambers (dipole<br />

magnets) or pipes (quadrupole <strong>and</strong> steering magnets). All other parts, valves, chambers <strong>for</strong><br />

pumping <strong>and</strong> beam diagnostics, pipes with compensators, measuring systems <strong>and</strong> ion pumps<br />

have to be purchased if not available from the GSI pool.<br />

6.6.6 CRYRING Control System<br />

The present CRYRING accelerator control system is in almost all aspects very different from<br />

the existing GSI control system as well as the control system under development <strong>for</strong> FAIR. As it<br />

is, it cannot be coherently integrated in the existing GSI control system framework. Taking into<br />

account that GSI fully focuses its activities <strong>and</strong> resources on the FAIR project, a comprehensive<br />

replacement of the CRYRING control system within the proposed time schedule (setting up the<br />

machine at ESR in the course of the year 2013) is unrealistic. Moreover, no technical support<br />

<strong>and</strong> maintenance to the original CRYRING control system can be provided by the Accelerator<br />

Controls Department (BEL).<br />

Consequently, this report proposes to initially set up <strong>and</strong> recommission CRYRING at GSI<br />

with its original control system with support by CRYRING experts from Sweden. However, a<br />

partial or full replacement of the control system after initial recommissioning is possible <strong>and</strong><br />

would even provide excellent test opportunities <strong>for</strong> FAIR (see Chapter 5).<br />

Considering the installation of CRYRING at GSI, it was discussed <strong>and</strong> agreed with the<br />

technical experts, that it is not reasonable to move the present general IT infrastructure of<br />

the CRYRING control system (servers, active network equipment, <strong>and</strong> control room operator<br />

stations) to GSI. Instead, a new system environment shall be provided <strong>and</strong> installed by the GSI<br />

Controls department on which the CRYRING control system can be installed <strong>and</strong> configured<br />

by CRYRING experts from Sweden.


28 Chapter 6. Proposed Construction Cycle<br />

6.7 Assembly of CRYRING <strong>and</strong> Injection Beam Lines<br />

6.7.1 Preparation of Magnetic Components: Fiducialization<br />

As network measurements <strong>and</strong> final alignment are based on using Laser Trackers <strong>and</strong> Digital<br />

Levels about 55 magnetic components of the CRYRING <strong>and</strong> two injection beam lines have to be<br />

fiducialized be<strong>for</strong>e assembly. Fiducialization means that the magnetic axes, planes <strong>and</strong> effective<br />

centres of dipole, quadrupole or sextupole magnets have to be transferred to mechanical marks<br />

suitable <strong>for</strong> the final alignment during the assembly of beam lines <strong>and</strong> ring. As the alignment of<br />

12 quadrupole magnets in the injection beam lines will be carried out by telescope, fiducialization<br />

of these components is not necessary <strong>and</strong> a 3D-determination of the actual condition w.r.t. the<br />

global coordinate system will not be possible.<br />

6.7.2 Procurement of Mechanical Parts<br />

The procurement of about 200 additional mechanical supports is necessary <strong>for</strong> lifting the low<br />

energy injection beam line <strong>and</strong> the present beam axis of CRYRING from 1.5 m to 2.0 m which<br />

is the nominal height <strong>for</strong> ion beams in ESR <strong>and</strong> in the Target Hall.<br />

The material <strong>for</strong> the supports of the 20 m long new beam line from the high energy beam<br />

transport to the CRYRING is available from the pool of dismantled systems.<br />

6.7.3 Assembly<br />

Survey Be<strong>for</strong>e starting the mechanical assembly the positions of all bending magnets (beam<br />

lines <strong>and</strong> CRYRING) have to be surveyed precisely. Position marks on the ground floor with an<br />

accuracy of ±0.5 mm will help to achieve a rather good positioning during the assembly work<br />

without the presence of the survey people.<br />

Assembly of CRYRING The assembly of the ring will be per<strong>for</strong>med sector by sector. By<br />

this way assembled sectors can already be connected to power supplies <strong>and</strong> water cooling while<br />

others are still being mechanically assembled. Fine alignment of the ring can be done by means<br />

of laser tracking simultaneously to the mechanical assembly of the injection beam lines.<br />

Assembly of Injection Beam Lines The alignment of the beam lines will be done by applying<br />

conventional methods. There<strong>for</strong>e three pillars with bearings <strong>for</strong> telescopes have to be surveyed in<br />

advance. Targets marking the axes of quadrupoles will allow fine adjustments to about ±0.5 mm<br />

accuracy. Suitable marks on the luminescent screens, applied <strong>for</strong> the determination of the ion<br />

beam axis, can be adjusted by this method to similar accuracy.


6.7. Assembly of CRYRING <strong>and</strong> Injection Beam Lines 29<br />

Figure 6.1.<br />

RING@ESR.<br />

Detailed view of proposed modification to Cave B with the installation of CRY-


30 Chapter 6. Proposed Construction Cycle<br />

Figure 6.2. Arrangement of power supplies <strong>and</strong> other technical installations <strong>for</strong> CRYRING on top<br />

of the modified Cave B roof.


Chapter 7<br />

Project Steering<br />

7.1 Time Schedule<br />

The proposed time schedule of the <strong>CRYRING@ESR</strong> project is shown in Figure 7.1. The rather<br />

tight schedule is associated to the boundary conditions at the Manne-Siegbahn-Laboratory <strong>and</strong><br />

at GSI/FAIR described in Section 6.1 which are repeated here once more:<br />

• The disassembly <strong>and</strong> removal of CRYRING has to be finished around the end of 2012.<br />

• The absolutely necessary technical support by experienced MSL staff members during<br />

reassembly <strong>and</strong> commissioning of the modified CRYRING at GSI will be available only<br />

during the coming two or three years.<br />

• The support by GSI staff from technical divisions (BES <strong>and</strong> GA) will be disposable only<br />

until middle of 2014.<br />

<strong>CRYRING@ESR</strong> (a study goup report)<br />

GSI board (May/June)<br />

FAIR board (June)<br />

FAIR council (Dec. 2nd)<br />

Clearing of Cave B area<br />

Disassembly of CRYRING at MSL<br />

Construction of CRYRING cave<br />

Transport of CRYRING to GSI<br />

Fast beam ejection at ESR<br />

Reassembly at ESR<br />

Commissioning with RFQ injector<br />

Commissioning with ESR beam<br />

First experiments<br />

2012 2013<br />

2014<br />

5 6 7 8 9 10 11 12 1 2 3 4 5 6 7 8 9 10 11 12 1 2 3 4 5 6<br />

Figure 7.1. Proposed time schedule <strong>for</strong> <strong>CRYRING@ESR</strong> under the boundary conditions described<br />

in Section 6.1<br />

In order to meet the described conditions the project should be started without any delay<br />

within the coming 2 months. The most urgent decisions have to be made concerning both the<br />

dismantling of Cave B <strong>and</strong> the disassembly of the FOPI-detector, i.e. concerning the clearing<br />

of the Cave B area. A detailed MS project plan <strong>for</strong> disassembling CRYRING at MSL <strong>and</strong><br />

31


32 Chapter 7. Project Steering<br />

reassembling it in the Target Hall at GSI has been worked out already by the BES division,<br />

responsible <strong>for</strong> all mechanical work packages. The plan supposes that the start of the activities<br />

takes place in August 2012.<br />

7.2 Cost <strong>and</strong> Manpower Requirements<br />

The cost <strong>and</strong> man power requirements <strong>for</strong> the realization of <strong>CRYRING@ESR</strong> were analyzed<br />

in detail. We have completed our analysis <strong>for</strong> two scenarios, a minimal solution <strong>and</strong> a FAIR<br />

compatible setup. A minimal solution adapts the ring mostly as it is to the GSI infrastructure.<br />

The cost estimate <strong>for</strong> the minimal solution is 1 190 k <strong>and</strong> includes all work per<strong>for</strong>med by<br />

external companies. Moreover, 290 man weeks <strong>for</strong> the installation need to be provided by GSI,<br />

i.e. its infrastructure divisions (about 7–8 man years). It shall be noted, that this estimate<br />

does not yet include the costs <strong>for</strong> installation <strong>and</strong> commissioning of the main ring magnet power<br />

supplies; there, negotiations with external companies are still ongoing.<br />

The FAIR compatible solution will require additional expenses of 717 k <strong>and</strong> additional 197<br />

man weeks. These additional expenses should be covered by the FAIR budget (<strong>for</strong> test benches<br />

<strong>and</strong> hardware commissioning).<br />

The majority of cost estimates are based on careful calculations by experts from technical<br />

divisions. Some items are still rough estimates, some may be too high <strong>and</strong> less expensive<br />

alternatives are under investigation by the EET division.<br />

7.3 Project Structure: Installation <strong>and</strong> Operation<br />

For the installation of CRYRING at the ESR <strong>and</strong> finally <strong>for</strong> its operation, a dedicated project<br />

team is required. This team will be responsible <strong>for</strong> the organization, coordination, <strong>and</strong> physics<br />

per<strong>for</strong>mance of <strong>CRYRING@ESR</strong> (see Organization Figure 7.2). Project During Phasethe installation phase, it needs to<br />

Project Coordinator<br />

<strong>Ion</strong> Optics&<br />

Electron<br />

Cooling<br />

<strong>Ion</strong> Source &<br />

RFQ Injector<br />

Mechanics &<br />

UHV<br />

Beam<br />

Diagnostics &<br />

RF<br />

physicist** physicist engineer physicist<br />

Controls &<br />

Power<br />

Supplies<br />

physicist or<br />

engineer<br />

Cave<br />

Infrastructure<br />

& Safety<br />

physicist or<br />

engineer<br />

** also deputy project coordinator<br />

Figure 7.2. Organisation chart <strong>for</strong> the project phase of <strong>CRYRING@ESR</strong>. (** also deputy project<br />

coordinator).<br />

act in close cooperation with the teams of GSI infrastructure <strong>and</strong> will coordinate in addition<br />

the support by external groups, such as by the colleagues from Sweden. After the building up<br />

phase, the project team will change its profile <strong>and</strong> takes over the responsibility <strong>for</strong> operation<br />

(Figure 7.3). Basically, the group members will nearly remain the same but their tasks will<br />

be directed towards operation, maintenance, <strong>and</strong> the dem<strong>and</strong>s of the FAIR project (test of<br />

novel beam diagnostics, controls etc.). Members of the atomic physics division will act as the<br />

core of the project team. Most of them are already involved into the HITRAP project <strong>and</strong> its<br />

commissioning. Since from physical <strong>and</strong> technical point of view HITRAP <strong>and</strong> CRYRING are<br />

closely entangled (both HITRAP <strong>and</strong> CRYRING are the central facilities within the FLAIR<br />

building), the merging of both projects appears to be evident. The time <strong>and</strong> resource planning<br />

<strong>for</strong> HITRAP need to be adjusted accordingly. The assignment of personnel as well as the use of


7.4. Possible Sources of Funding 33<br />

Organization Commissioning & Operation<br />

Coordinator Operating &<br />

Experiments<br />

<strong>Ion</strong> Optics&<br />

Electron<br />

Cooling<br />

<strong>Ion</strong> Source &<br />

RFQ Injector<br />

Mechanics &<br />

UHV<br />

Beam<br />

Diagnostics &<br />

RF<br />

physicist** physicist engineer physicist<br />

Controls &<br />

Power<br />

Supplies<br />

physicist or<br />

engineer<br />

Cave<br />

Infrastructure<br />

& Safety<br />

physicist or<br />

engineer<br />

** also deputy project coordinator<br />

Figure 7.3. Organisation chart <strong>for</strong> commissioning <strong>and</strong> operation of <strong>CRYRING@ESR</strong>. (** also<br />

deputy operating & experiment coordinator)<br />

available financial resources has to be redistributed in order to enable HITRAP <strong>and</strong> CRYRING<br />

but with the priority to accomplish the installation of CRYRING be<strong>for</strong>e mid of 2014.<br />

7.4 Possible Sources of Funding<br />

In the following we list possible sources <strong>for</strong> funding of the <strong>CRYRING@ESR</strong> project. Once the<br />

project has been accepted, further sources of support will be investigated.<br />

• Merging of the HITRAP <strong>and</strong> the CRYRING project: Resources <strong>for</strong> investment <strong>and</strong> consumables<br />

will be redistributed accordingly. Man power <strong>for</strong> the project team will be provided<br />

by the atomic physics division.<br />

• Collaboration agreement between KVI <strong>and</strong> GSI.<br />

• Collaboration agreement between MPIK Heidelberg <strong>and</strong> GSI.<br />

• Offer by the University of Stockholm to support the installation of CRYRING by experienced<br />

personnel (in total up to two FTEs).<br />

• Stockholm University has recently offered an advanced internal gas target system <strong>for</strong> CRY-<br />

RING experiments.<br />

• A team of Atomic Physicists from Chalmers University of Technology, Gothenburg <strong>and</strong><br />

Stockholm University, as well as Nuclear Physicists from Chalmers <strong>and</strong> Lund University<br />

<strong>and</strong> Accelerator Physicists from Stockholm University <strong>and</strong> ESS, Lund, are preparing an<br />

application to the Knut & Alice Wallenberg Foundation <strong>for</strong> travel costs <strong>and</strong> stationing of<br />

personnel <strong>for</strong> extended periods of time at GSI/FAIR.<br />

• Application sent to the Council <strong>for</strong> <strong>Research</strong> Infrastructures in April 2012 by the board of<br />

SFAIR, the “umbrella organization” of Swedish scientists aiming <strong>for</strong> using FAIR further<br />

applications such as EU synergy grants.<br />

• Support by the Helmholtz-Institute Jena can be anticipated.<br />

7.5 Swedish contributions to the installation of <strong>CRYRING@ESR</strong><br />

The Manne Siegbahn Laboratory (MSL) at the Department of Physics, Stockholm University<br />

will mutatis mut<strong>and</strong>is fulfill the commitment as described in section 2.4 of the FLAIR LSR<br />

Technical Design Report [23]. In the changed perspective of a fast installation of CRYRING<br />

at ESR this would mean that MSL is responsible <strong>for</strong> the new hardware <strong>and</strong> modifications defined<br />

in the LSR, disassembling of the CRYRING <strong>and</strong> the transportation of it to GSI/FAIR in


34 Chapter 7. Project Steering<br />

Darmstadt in the beginning of 2013. It is planned that a small group from GSI will be invited<br />

by MSL to spend some months in Stockholm during the autumn 2012 to participate in the<br />

final disassembly <strong>and</strong> packing of the CRYRING in order to gain experience about the configuration<br />

of CRYRING be<strong>for</strong>e the disassembly. This experience would help considerably <strong>for</strong> an<br />

optimal reassembly of the ring at GSI. It should be remarked that the fact that the CRYRING<br />

is available intact <strong>and</strong> properly modified according to the requirements defined by the FLAIR<br />

collaboration has been accomplished by a large grant from the Swedish <strong>Research</strong> Council <strong>and</strong> by<br />

generous support from Stockholm University, both acknowledging the high scientific potential<br />

of the future use of the CRYRING at GSI/FAIR. The leader of the MSL team is the accelerator<br />

physicist Anders Källberg, who through the years has been responsible <strong>for</strong> the operation of the<br />

CRYRING at MSL. In addition to the CRYRING hardware described in the TDR, Stockholm<br />

University has recently offered an advanced internal gas target system <strong>for</strong> CRYRING experiments<br />

to be delivered with a ring. This opens new scientific opportunities which have attracted<br />

a substantial interest from physicists planning future experiments at <strong>CRYRING@ESR</strong>. After<br />

the transportation of CRYRING to Darmstadt, there are hitherto no <strong>for</strong>mal commitments <strong>for</strong><br />

a Swedish participation in its installation at the ESR. However Stockholm University offers<br />

that two experienced accelerator physicists, a highly qualified engineer, expert on the CRY-<br />

RING Control System <strong>and</strong> a mechanical engineer will spend up to in total two person-years<br />

at GSI/FAIR. Dependent on the success of applications of further financial support from the<br />

Swedish <strong>Research</strong> Council (application sent to the Council <strong>for</strong> <strong>Research</strong> Infrastructures in April<br />

2012 by the board of SFAIR, the “umbrella organization” of Swedish scientists aiming <strong>for</strong> using<br />

FAIR) <strong>and</strong> the Knut & Alice Wallenberg Foundation (see below), Swedish presence in the<br />

installation <strong>and</strong> commissioning work might be increased.<br />

7.6 Swedish Participation in Experiments at FAIR: <strong>CRYRING@ESR</strong><br />

The new exciting scientific opportunities that can be offered soon with an early installation<br />

of the <strong>CRYRING@ESR</strong> have stimulated Swedish scientists to plan <strong>for</strong> experiments at the new<br />

facility. A team of Atomic Physicists from Chalmers University of Technology, Gothenburg <strong>and</strong><br />

Stockholm University, as well as Nuclear Physicists from Chalmers <strong>and</strong> Lund University <strong>and</strong><br />

Accelerator Physicists from Stockholm University <strong>and</strong> ESS, Lund are preparing an application<br />

to the Knut & Alice Wallenberg Foundation <strong>for</strong> travel costs <strong>and</strong> stationing of personnel <strong>for</strong><br />

extended periods of time at GSI/FAIR. Scientific issues that are planned to be addressed are<br />

within the areas: Atomic-ion collisions, <strong>Ion</strong>-photon collisions <strong>and</strong> nuclear <strong>and</strong> nuclear astrophysics<br />

experiments. An important part of the application is also positions <strong>for</strong> two postdoctoral<br />

researchers, who should work on<br />

1. starting up research development on experiments <strong>and</strong> detectors with a focus on nuclear<br />

reactions <strong>and</strong> nuclear astrophysics <strong>and</strong><br />

2. ion-optical problems, in particular optimization of the transmission of radioactive beams<br />

into the ESR.<br />

The main applicant, PI, <strong>for</strong> the application to the Knut & Alice Wallenberg Foundation is<br />

Andreas Heinz, nuclear physicist at Chalmers University of Technology.


Bibliography<br />

[1] FAIR. Green Paper: The Modularized Start Version. Tech. rep. Darmstadt: GSI, 2009.<br />

url: http : / / www . fair - center . de / fileadmin / fair / publications _ FAIR / FAIR _<br />

GreenPaper_2009.pdf.<br />

[2] B. Franzke, H. Geissel, <strong>and</strong> G. Münzenberg. In: Mass Spectrometry Reviews 27.5 (2008),<br />

pp. 428–469. issn: 1098-2787. doi: 10.1002/mas.20173.<br />

[3] A. Gumberidze, T. Stöhlker, D. Banaś, et al. In: Phys. Rev. Lett. 94 (2005), p. 223001.<br />

doi: 10.1103/PhysRevLett.94.223001.<br />

[4] I. Klaft, S. Borneis, T. Engel, et al. In: Phys. Rev. Lett. 73 (1994), pp. 2425–2427. doi:<br />

10.1103/PhysRevLett.73.2425.<br />

[5] C. Br<strong>and</strong>au, C. Kozhuharov, A. Müller, et al. In: Phys. Rev. Lett. 91.7 (2003), p. 073202.<br />

doi: 10.1103/PhysRevLett.91.073202.<br />

[6] M. Jung, F. Bosch, K. Beckert, et al. In: Phys. Rev. Lett. 69 (15 1992), pp. 2164–2167.<br />

doi: 10.1103/PhysRevLett.69.2164.<br />

[7] Y. A. Litvinov, F. Bosch, H. Geissel, et al. In: Phys. Rev. Lett. 99 (26 2007), p. 262501.<br />

doi: 10.1103/PhysRevLett.99.262501.<br />

[8] J. Eichler <strong>and</strong> T. Stöhlker. In: Phys. Reports 439 (2007), pp. 1–99. doi: 10.1016/j.<br />

physrep.2006.11.003.<br />

[9] D. Misra, H. T. Schmidt, M. Gudmundsson, et al. In: Phys. Rev. Lett. 102 (15 2009),<br />

p. 153201. doi: 10.1103/PhysRevLett.102.153201.<br />

[10] E. Vigren, M. Hamberg, V. Zhaunerchyk, et al. In: Astrophys. J. 709 (2010), pp. 1429–<br />

1434. doi: 10.1088/0004-637X/709/2/1429.<br />

[11] I. Orban, S. D. Loch, S. Böhm, <strong>and</strong> R. Schuch. In: Astrophys. J. 721 (2010), pp. 1603–<br />

1607. doi: 10.1088/0004-637X/721/2/1603.<br />

[12] E. Vigren, M. Hamberg, V. Zhaunerchyk, et al. In: Astrophys. J. 695.1 (2009), p. 317.<br />

doi: 10.1088/0004-637X/695/1/317.<br />

[13] H. T. Schmidt, D. Fischer, Z. Berenyi, et al. In: Phys. Rev. Lett. 101 (8 2008), p. 083201.<br />

doi: 10.1103/PhysRevLett.101.083201.<br />

[14] R. Schuch, E. Lindroth, S. Madzunkov, et al. In: Phys. Rev. Lett. 95 (2005), p. 183003.<br />

doi: 10.1103/PhysRevLett.95.183003.<br />

[15] H. T. Schmidt, A. Fardi, R. Schuch, et al. In: Phys. Rev. Lett. 89 (2002), p. 163201. doi:<br />

10.1103/PhysRevLett.89.163201.<br />

[16] H.-J. Kluge, T. Beier, K. Blaum, et al. In: Adv. Quant. Chem. 53 (2008), p. 83. doi:<br />

10.1016/S0065-3276(07)53007-8.<br />

[17] C. Br<strong>and</strong>au. unpublished.<br />

35


36 BIBLIOGRAPHY<br />

[18] SPARC. Stored Particles Atomic <strong>Research</strong> Collaboration. url: http://www.gsi.de/<br />

sparc.<br />

[19] FLAIR. <strong>Facility</strong> <strong>for</strong> Low-energy <strong>Antiproton</strong> <strong>and</strong> <strong>Ion</strong> <strong>Research</strong>. url: http : / / www .<br />

flairatfair.eu/.<br />

[20] EXL. EXotic nuclei studied in Light-ion induced reactions. url: http://www.rug.nl/<br />

kvi/<strong>Research</strong>/hnp/<strong>Research</strong>/EXL/index.<br />

[21] ILIMA. Isomeric beams, LIfetimes <strong>and</strong> MAsses. url: http://www.fair-center.eu/<br />

fair-users/experiments/nustar/experiments/ilima.html.<br />

[22] ELISe. ELectron-<strong>Ion</strong> Scattering Experiment. url: http://www.fair-center.eu/fairusers/experiments/nustar/experiments/elise.html.<br />

[23] H. Danared, G. Andler, M. Björkhage, et al. LSR - Low-energy Storage Ring. Technical<br />

Design Report. Version 1.3, May 6th 2011. Manne-Siegbahn Laboratory, Physics<br />

Department, Stockholm University, 2011.


Appendix A<br />

Letters of Support<br />

Letters of Support <strong>for</strong> <strong>CRYRING@ESR</strong> were kindly provided by several international research<br />

groups <strong>and</strong> all storage ring collaborations of the FAIR project <strong>and</strong> are appended in the following:<br />

• KVI Groningen (pg. 38),<br />

• Institute of Modern Physics, Chinese Academy of Sciences (pg. 39),<br />

• the community of Austrian researchers (pg. 40),<br />

• Swedish FAIR Consortium (FAIR Sweden) (pg. 43).<br />

The storage ring collaborations at FAIR:<br />

• ELectron-<strong>Ion</strong> Scattering Experiment, ELISe collaboration (pg. 45),<br />

http://www.fair-center.eu/fair-users/experiments/nustar/experiments/elise.<br />

html<br />

• EXotic nuclei studied in Light-ion induced reactions, EXL collaboration (pg. 46),<br />

http://www.rug.nl/kvi/<strong>Research</strong>/hnp/<strong>Research</strong>/EXL/index<br />

• <strong>Facility</strong> <strong>for</strong> Low-energy <strong>Antiproton</strong> <strong>and</strong> <strong>Ion</strong> <strong>Research</strong>, FLAIR collaboration (pg. 47),<br />

http://www.flairatfair.eu/<br />

• Isomeric beams, LIfetimes, <strong>and</strong> MAsses, ILIMA collaboration (pg. 48),<br />

http://www.fair-center.eu/fair-users/experiments/nustar/experiments/ilima.<br />

html<br />

• Stored Particles Atomic Physics <strong>Research</strong> Collaboration, SPARC collaboration (pg. 50).<br />

http://www.gsi.de/sparc<br />

37


Prof. Dr. Horst Stöcker<br />

GSI Helmholtzzentrum für<br />

Schwerionen<strong>for</strong>schung GmbH<br />

Planckstr. 1<br />

64291 Darmstadt<br />

Dear Prof. Stöcker, lieber Horst,<br />

we, members of the community of Austrian scientists interested<br />

in the research possible at FAIR, want to express our strong<br />

support <strong>for</strong> the recent initiative of installing the CRYRING accelerator<br />

at the ESR storage ring of GSI. This will open up the possibility<br />

to explore already now a part of the physics program of<br />

FLAIR with highly charged ions available from ESR <strong>and</strong> keep<br />

CRYRING in continuous operation until antiproton or higher intensity<br />

HCI beams from FAIR become available, <strong>for</strong> which<br />

CRYRING was originally <strong>for</strong>eseen. The FOPI experiment existing<br />

in the vicinity of ESR could then potentially be used to explore<br />

hadron physics with stopped antiprotons, which will be a unique<br />

feature of FLAIR.<br />

We think this current initiative will strengthen the interest <strong>and</strong><br />

support of the physics communities in FLAIR <strong>and</strong> will allow a<br />

strong physics program to be carried out until the full FLAIR facility<br />

can be realized.<br />

Wien, 23.05.2012<br />

Bearbeiter/in / Durchwahl / E-Mail<br />

Prof. Dr. Eberhard Widmann, Director<br />

Eberhard.widmann@oeaw.ac.at<br />

Expression of support <strong>for</strong><br />

<strong>CRYRING@ESR</strong><br />

Yours sincerely<br />

Prof. Eberhard Widmann<br />

Director, Stefan Meyer Institute<br />

Page 1 of 3


Univ.-Prof. Dipl.-Ing.Dr. Gerald BADUREK<br />

Dean of the Faculty of Physics<br />

Vienna University of Technology<br />

Univ.Prof. Dr. Friedrich Aumayr<br />

Institut f. Angew<strong>and</strong>te Physik<br />

Vienna University of Technology<br />

Univ.Prof. Dipl.-Ing. Dr.techn. Manfried Faber<br />

Atominstitut<br />

Vienna University of Technology<br />

Univ.Prof. Dipl.-Ing. Dr.techn. Helmut Leeb<br />

Atominstitut<br />

Vienna University of Technology<br />

Ass.Prof. Dipl.-Ing. Dr. Erwin Jericha<br />

Atominstitut<br />

Vienna University of Technology<br />

Page 2 of 3


2(2)<br />

timely implementation of major parts of the APPA-FLAIR facility, now in module 4, in<br />

a much earlier stage <strong>and</strong> could as well serve <strong>for</strong> research along the scientific lines of<br />

NUSTAR.<br />

The community represented by SFAIR is most supportive to these plans, <strong>and</strong> have or<br />

are underway to try to secure additional resources <strong>for</strong> their successful completion.<br />

Several research groups from Swedish universities have declared strong interest in using<br />

the CRYRING/ LSR set-up with beams from the ESR in the first phase <strong>for</strong> novel<br />

research program. Furthermore, key personnel from MSL will be made available from<br />

Stockholm University to support the mounting <strong>and</strong> commissioning of CRYRING/ LSR<br />

in the Target Hall at GSI.<br />

We emphasize that SFAIR sees the CRYRING/ LSR project as an important step to<br />

realize the storage ring physics program in a timely manner at FAIR.<br />

Chairperson, SFAIR<br />

c.c. T. Stöhlker, GSI<br />

B. Sharkov, FAIR<br />

G. Rosner, FAIR<br />

Organisations/VATnr:<br />

202100-2932


GSI Helmholtzzentrum für<br />

Schwerionen<strong>for</strong>schung GmbH<br />

Planckstraße 1<br />

64291 Darmstadt<br />

www.gsi.de<br />

GSI . Planckstraße 1 . 64291 Darmstadt . Deutschl<strong>and</strong><br />

Prof. Dr. Thomas Stöhlker<br />

Nuclear Reactions/<strong>Research</strong><br />

Head of Department:<br />

Prof. Dr. Thomas Aumann<br />

Deputy:<br />

Dr. Haik Simon<br />

Phone +49 6159 71-2887<br />

Fax +49 6159 71-2809<br />

Mobile +49 1743281519<br />

H.Simon@gsi.de<br />

Subject:<br />

CRYRING project:<br />

Letter of support from the ELISe collaboration<br />

May 20 th , 2012<br />

Dear Prof. Dr. Thomas Stöhlker, dear Thomas,<br />

I am writing this letter as the spokesperson of the ELISe collaboration <strong>and</strong> on behalf<br />

of the collaboration. I would like to express our full support <strong>and</strong> interest in the activities<br />

leading to the storage ring facility ESR <strong>and</strong> <strong>CRYRING@ESR</strong>, being initially<br />

coupled to the FRS <strong>and</strong> potentially later to the Super-FRS.<br />

Since ELISe is not included in the start-version of FAIR, the <strong>CRYRING@ESR</strong> facility<br />

provides excellent opportunities <strong>for</strong> test experiments <strong>and</strong> detector developments<br />

<strong>for</strong> the in-ring instrumentation of the ELISe setup.<br />

Geschäftsführung:<br />

Professor Dr. Dr. h.c. Horst Stöcker<br />

Dr. Hartmut Eickhoff<br />

Vorsitzende des Aufsichtsrates:<br />

Dr. Beatrix Vierkorn-Rudolph<br />

Stellvertreter:<br />

Ministerialdirigent Dr. Rolf Bernhardt<br />

Sitz: Darmstadt<br />

Amtsgericht Darmstadt HRB 1528<br />

VAT-ID: DE 111 671 917<br />

L<strong>and</strong>esbank Hessen/Thüringen<br />

BLZ 500 500 00 . Konto 50 01865 004<br />

IBAN DE56 5005 0000 5001 8650 04<br />

BIC HELA DE FF<br />

We are currently looking also into the opportunities <strong>for</strong> first installing the eA collider<br />

at the ESR with limited per<strong>for</strong>mance, keeping in mind that we’d be such already<br />

competitive with the upcoming SCRIT facility in Japan.<br />

In this context we welcome any activities <strong>and</strong> plans that allow <strong>for</strong> a vivid <strong>and</strong> strong<br />

nuclear physics programme at GSIs storage ring prior to the delayed realization of<br />

the NESR at FAIR. The realization of <strong>CRYRING@ESR</strong> would set an important corner<br />

stone immediately thrilling all experimental communities associated with the<br />

storage ring physics programme at FAIR.<br />

With kind regards,<br />

(Haik Simon)


Prof. Dr. Horst Stöcker<br />

GSI Helmholtzzentrum für<br />

Schwerionen<strong>for</strong>schung GmbH<br />

Planckstr. 1<br />

Gespeicherte und gekühlte <strong>Ion</strong>en<br />

Stored <strong>and</strong> Cooled <strong>Ion</strong>s<br />

Prof. Dr. Klaus Blaum<br />

Tel: 06221-516 850/1<br />

Fax: 06221-516 852<br />

sekretariat.blaum@mpi-hd.mpg.de<br />

64291 Darmstadt<br />

25. April 2012<br />

Dear Professor Stöcker, lieber Horst,<br />

On behalf of the FLAIR collaboration we would like to express our strong support <strong>for</strong> the<br />

<strong>CRYRING@ESR</strong> project, <strong>and</strong> we appreciate very much the future option of a connection to<br />

the Super-FRS.<br />

Since FLAIR is not included in the start-up version of FAIR, the <strong>CRYRING@ESR</strong> project<br />

provides excellent possibilities to pursue already some of our planned test experiments <strong>and</strong><br />

detector tests, especially in view of the delay in the construction of the New Experimental<br />

Storage Ring (NESR), which is a m<strong>and</strong>atory ring <strong>for</strong> FLAIR. <strong>CRYRING@ESR</strong> will provide<br />

low energetic highly charged heavy ion beams, one of the main experimental programs of<br />

FLAIR, see the LSR-project within FLAIR.<br />

In addition, a continuous running of CRYRING <strong>and</strong> the installation of HITRAP at its final<br />

position will allow a fast <strong>and</strong> efficient start of the physics program of FLAIR@FAIR.<br />

In summary, we see the <strong>CRYRING@ESR</strong> installation as an excellent initiative towards the<br />

low-energetic storage ring projects at FAIR.<br />

With our best regards,<br />

KLAUS BLAUM<br />

Spokesperson of the FLAIR Collaboration<br />

EBERHARD WIDMANN<br />

Co-Spokesperson of the FLAIR Collaboration


Professor H. Stöcker<br />

GSI, Darmstadt<br />

4 th May 2012<br />

Dear Professor Stöcker,<br />

On behalf of the ILIMA collaboration, I would like to express strong support <strong>for</strong> the<br />

<strong>CRYRING@ESR</strong> project, with the future option of a connection to the Super-FRS.<br />

One of the main facilities <strong>for</strong> the ILIMA experimental program is the New<br />

Experimental Storage Ring (NESR), which is however outside the start-up version of<br />

FAIR. As has often been stressed, this significantly delays the realisation of the<br />

planned storage-ring experimental programs, <strong>and</strong> it could also cause irreversible<br />

negative consequences <strong>for</strong> the associated experimental communities.<br />

A novel possibility is now under consideration. Installation of the CRYRING coupled<br />

to the present ESR will extend the physics capabilities by enabling the production, in<br />

the near future, of highly ionized heavy ions at the lowest kinetic energies. This<br />

project has very high experimental discovery potential, including <strong>for</strong> ILIMA-related<br />

experiments. For instance, searching <strong>for</strong> the Nuclear Excitation by Electron Capture<br />

(NEEC) <strong>and</strong> the Nuclear Excitation by Electron Transition (NEET) phenomena will<br />

become possible. There<strong>for</strong>e, we support an early construction of the CRYRING<br />

coupled to the ESR.<br />

It is important to emphasise that there is a future option which <strong>for</strong>esees the connection<br />

of the present ESR to the Super-FRS. This is extremely attractive <strong>for</strong> the ILIMA<br />

collaboration. It will enable the possibility of per<strong>for</strong>ming ILIMA experiments with<br />

cooled exotic ions in the ESR, with the highest secondary-beam intensities which will<br />

be available from the Super-FRS. This transitional arrangement would enable us to<br />

cover part of the ILIMA experimental program prior to the realisation of the NESR.<br />

Furthermore, the novel detector setups, which are <strong>for</strong>eseen <strong>for</strong> the NESR experiments,<br />

can be built <strong>and</strong> implemented <strong>for</strong> real physics experiments in the ESR under FAIR


conditions, which will allow us to prepare in the best way <strong>for</strong> experiments in the<br />

NESR.<br />

Overall, we see the <strong>CRYRING@ESR</strong> as a very timely <strong>and</strong> important step towards the<br />

success of the storage-ring scientific program at FAIR.<br />

Yours sincerely,<br />

Phil Walker<br />

Spokesperson <strong>for</strong> the ILIMA Collaboration


STOCKHOLM UNIVERSITY<br />

Physics Department<br />

Atomic Physics Division<br />

Prof. Dr. Reinhold Schuch<br />

May. 24. 2012<br />

Subject: <strong>CRYRING@ESR</strong>, Letter of support from the SPARC collaboration<br />

To whom it may concern!<br />

I am writing this letter as spokesperson <strong>and</strong> on behalf of the SPARC collaboration. I would like<br />

to express our full support in this new FAIR related initiative of installing the CRYRING at the<br />

ESR of GSI. This project is an important <strong>and</strong> essential step towards the realization of our<br />

challenging anticipated physics progam at FAIR which concentrates on physics with stored <strong>and</strong><br />

cooled heavy ions <strong>and</strong> rare isotopes.<br />

Although the storage ring branch of the FAIR project has an outst<strong>and</strong>ing visibility due to its<br />

expected scientific impact, its major component, the NESR, has been postponed by an<br />

undefined amount of years. The realization of CRYRING at the ESR would compensate already<br />

now to a large extend <strong>for</strong> this loss <strong>and</strong> this combination of CRYRING with the ESR would<br />

bring the storage ring physics into Modularized Start Version of FAIR. In particular SPARC but<br />

also all the other collaborations that depend on storage rings would profit tremendously from<br />

this project <strong>and</strong> will keep them actively involved into FAIR. Finally, the SPARC collaboration<br />

is convinced that the scientific success of the CRYRING project at the ESR will promote the<br />

realization of the NESR <strong>and</strong> the FLAIR facility at the earliest possible date.<br />

I want to point out also, in view of the scientific merits of this initiative, the SPARC<br />

collaboration would contribute as much as possible to realize this important project.<br />

Yours sincerely<br />

Reinhold Schuch<br />

Spokesperson of the SPARC Collaboration<br />

Division of Atomic Physics<br />

FYSIKUM<br />

Stockholm University<br />

Address: Physics Center<br />

S-106 91 Stockholm<br />

Sweden<br />

Telephone:<br />

Nat. 08-55378621<br />

Int. +46-8-55378621<br />

Secr:<br />

+46-8-55378600<br />

Fax +46-8-55378601<br />

E-mail addresses:<br />

schuch@physto.se<br />

http://physto.se

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