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Proposal for a high-intensity, light and heavy ion facility in Europe ECOS-LINCE: European LINAC CENTER Prepared by Ismael Martel (Huelva University)

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Presentation on theme: "Proposal for a high-intensity, light and heavy ion facility in Europe ECOS-LINCE: European LINAC CENTER Prepared by Ismael Martel (Huelva University)"— Presentation transcript:

1 Proposal for a high-intensity, light and heavy ion facility in Europe ECOS-LINCE: European LINAC CENTER Prepared by Ismael Martel (Huelva University)

2 This document was prepared by the ECOS (European COllaboration on Stable ion beams) working group, in order to describe the research perspectives with high intensity stable ion beams, to help categorize existing facilities and to identify the opportunities for a dedicated new facility in EUROPE ECOS Working group: Faiçal Azaiez (Chair) (IPNO Orsay) Giacomo de Angelis (LNL Legnaro) Rolf-Dietmar Herzberg (Liverpool) Sigurd Hofmann (GSI Darmstadt) Rauno Julin (Jyväskylä) Marek Lewitowicz (GANIL Caen) Marie-Helene Moscatello (GANIL Caen) Anna Maria Porcellano (LNL Legnaro) Ulrich Ratzinger (Frankfurt) HIGH INTENSITY STABLE ION BEAMS IN EUROPE

3 …“The long-term goal for a new dedicated high intensity stable ion beam facility in Europe, with energies at and above the Coulomb barrier, is considered to be one of the important issues to be discussed in the next Long Range Plan of the nuclear physics community.”… IV: Concluding remarks and recommendations ECOS working group conclusions

4 LINCE; high-intensity superconducting LINAC - Wide range of ions, from protons to Uranium - Wide range of energies, up to 10 A MeV for 238U - High Intensity accelerator (1 mA light ions  10 p  A heavy ions) LINCE: energy booster using heavy-ion synchrotron: - 50 MeV/u for light ion species MeV for deuterons. PROGRAM: - Basic and Fundamental problems in nuclear physics - Applications of nuclear physics - Interaction with Industry ECOS facility: a FIRST CLASS High intensity heavy-ion accelerator for stable ions, with energies at and above the Coulomb barrier. LINCE proposal

5 The totality of the ECOS physics case - Nuclear structure, low, medium and high spin - Reaction mechanisms - Charge-exchange reactions - Isomers - Ground-state properties - Astrophysics - Superheavies - Nuclear equation of state (EOS) - Fundamental physics: neutrinoless double-beta decay …Studies where one can benefit from high intensity stable beams Basic Nuclear Physics

6 DEVELOPMENTS - High resolution spectrometers and recoil separators with high rejection power (MAGNEX, VAMOS, PRISMA,…) - High power targets - New generation of gamma & particle detectors (FAZIA, AGATA,…) with new generation electronics and data correlation systems. Separator + Long and dedicated beam time!! Spectrometer Gamma-particle Typical experimental setup

7 Material research for energy production Fusion energy research: aiming at qualifying advanced materials resistant to extreme conditions, specific to fusion reactors like ITER. Intense ion beams of moderate energy are needed to simulate fusion reactor conditions. (CIEMAT) IFMIF project: a 40 MeV, 125 mA deuteron + lithium target  neutrons to test materials for first generation of fusion reactors  the DEMO reactor Cocktail beams à la JANNUS Double, triple charged ions Condition: Same A/q EX: 56 Fe (14+) + 4 He(1+) Fusion energy research

8 What LINACs can do better (than cyclotrons) ECOS-LINCE 2013, Ulli Coester, Grenoble Modern radioisotopes are currently investigated/used to treat in a more efficient way the different tumours and cancer disease of our society. Radioisotope production

9 Highly demanded ions & energies ~10 MeV/u Typical figures from RADEF, Finland High intensity ion beams are used in aerospace programs for radiation resistant electronics and in nuclear energy applications. Quality tests are required in order to accomplish with UE safety regulations for energy control and aerospace on-board electronics. Research can be centred on the impact of radiation on the response of new device technologies and single-event effects in new technologies and ultra-small devices. Aerospace electronics

10 For the program on basic nuclear physics and applications it is proposed the following parameters: Protons to Uranium: 1 mA max intensity  eg., 48 Ca (8+) > 10 p  A LINAC: E from 40 keV/u to (8.5 – 45) MeV/u depending on A/q SYNCHROTON: 50 MeV/u for light ion species & 200 MeV for deuterons. Full-SC ECR ion source GHz RFQ for 1 ≤ A/q ≤ 7 Superconducting cavities Energies reachable with 4 Cryo-modules: COMPACT linac hours of availability, with 5000 hours for ECOS science and 2000 hours for Applications LINCE-main parameters

11 Choice of 1 st harmonic (fundamental)  defined minimum time of flight: 50 ns Fundamental frequency: MHz (54.98 ns) from RF amplifier market  HI- buncher For protons and alphas: F = MHz  need double buncher (space charge issues) Frequency of RFQ, F = MHz (4 th harm.) ◦ E in/out = 0.04A MeV / 0.5A MeV Frequency of SC cavities : MHz (4 th harm.) and MHz (6 th harm.) Multi-Harmonic Buncher is MANDATORY A/QE/AExampleCharge state Intensity: < 1mA 142H1+ 225D O S Ca Ca U34+ Partially funded by R&D projects at University of Huelva, Spain Pre-design studies

12 LINCE LINAC layout Pre-design activities

13 Building integration

14 C1: β = 0.045, f = MHz C2: β = 0.077, f = MHz C3: β = 0.15, f = MHz RFQ f = 72.75MHz LINCE LINAC: “60 MV equivalent electrostatic accelerator” Proposed layout of LINCE MHB2 f = MHz MHB1 f = MHz Rebuncher

15 Experimental equipment has to be defined and built - Benefit of already detectors being build at EU 1. FAZIA 2. AGATA 3. GASPARD/HYDE - High Resolution Fragment separator: high selectivity at high intensity - High Resolution Spectrometer The experimental equipment

16 On-going actions at University of Huelva Beam dynamics, transport to exp. lines and building integration Design studies of ECR, buncher, warm magnets, RFQ, SC QWR, couplers, SC magnets, and criomodules RFQ model in Al (one full section) and in Cu (one vane) + brazing tests Ion source test bench Model of MH Buncher Machining and welding tests with Nb Parts of one QWR resonator Cryolab for cavity testing, including one multi-propose cryostat RF lab for testing resonators Specific design of selected elements Industry & Universities Technology Transfer Project funded by National Government in Spain (5 Universities, 7 large companies, 5 small companies). Pre-design studies of LINCE

17 General operation Host region can cover part of the personnel and the operation costs Participating institutes can collaborate with personnel, instruments, funds… A legal framework should be defined for the full facility (International ECOS collaboration) Estimated cost of LINAC Complete LINAC accelerator with servitudes, without building and experimental facilities : 48 M€ Estimated operation cost : 5 M€/y EU Convergence funds with help of participating Institutes Preliminary matrix cost

18 Pre- design Detailed designConstructionCommis sioning Construction decision Proposed planning

19 ECOS-LINCE: Possible European Sites

20 SPAIN

21 Punta Umbría Beach Resort, 3 Km Huelva University 3 Km PARQUE CIENTÍFICO TECNOLÓGICO DE HUELVA (PCTH, Aljaraque)

22 European LINAC CENTER ECOS-LINCE

23 Superheavies

24   picobarn!! at relevant energies < 1 MeV, few GK Extrapolation from higher energies by using the astrophysical S(E) factor: S(E) =  (E) E exp(2πη)  DIRECT & INDIRECT METHODS -Increase number of detected particles ( “brute force”:  intensity,  detector eff.) - Reduce the background - Fight with electron screening: theory does not work!! DIRECT METHODS Coulomb dissociation: Determine the absolute S(E) factor of a radiative capture reaction A+x  B+  studying the reversing photodisintegration process B+   A+x ~100 MeV/A Trojan Horse Method (THM): Determine the S(E) factor of a charged particle reaction A+x  c+C selecting the Quasi Free contribution of an appropriate A+a(x+s)  c+C+s reaction. INDIRECT METHODS Asymptotic Normalization Coefficients (ANC): Determine the S(0) factor of the radiative capture reaction, A+x  B+  studying a peripheral transfer reaction into a bound state of the B nucleus. Astropysics

25 - Pair correlations (nn,pp,np channels) in transfer reactions at sub-barrier energies - Charge exchange reactions - Multinucleon transfer reactions (neutron rich nuclei) and effects on induced fission and quasi fission processes - Hindrance phenomenon in sub-barrier fusion reactions Transfer and fusion reaction studies

26 In-flight production of exotic nuclei at reaction targets Typical beams 40 Ar ~ 14 MeV/u 86 Kr ~ 8.5 MeV/u 84 Kr ~ 10 MeV/u 136 Xe ~ 7 MeV/u Exotic isotope production: Height of the Coulomb barrier ~ 4 to 5 MeV/nucleon:  compound nucleus/fus.evap reactions, E ~ Eb  proton rich  reactions of nucleon exchange, E>> Eb  neutron rich Compound nucleus/fus. evap reactions  Basic mechanism for production of proton rich nuclei M. Veselsky, G.A. Souliotis, Nuclear Physics A 765 (2006) 252; A 781 (2007) 521. G.A.Souliotis et al., PRC 84, (2011); M. Veselsky,et al., Nucl. Phys. A 872 (2011) 1. Nuclear structure at low, medium and high spin Neutron rich: preferably ”cold“ processes with minimum neutron loss.  Reactions of heavy ions with energies around > 10 MeV/u

27 Physics beyond the Standard Model

28 Xsections: ~nanobarn!!  High intensity ion beams Nuclear matrix elements

29 Reliable beam dynamics with low beam losses Calculated full transmission for H-I > 75% TRACK 3D (P. Ostroumov, A. Villari, I. Martel) Pre-design studies

30 HEAVY-ION SYNCHROTON: - LINAC injection at 15 MeV/u - OUTPUT: 50 MeV/u for light ion species & 200 MeV for deuterons - Design study to be done LINCE “energy booster”


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