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The DESIR physics workshop (Leuven 26 th – 28 th May) Paul Campbell Present status… Community interests… The future experiments…

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Presentation on theme: "The DESIR physics workshop (Leuven 26 th – 28 th May) Paul Campbell Present status… Community interests… The future experiments…"— Presentation transcript:

1 The DESIR physics workshop (Leuven 26 th – 28 th May) Paul Campbell Present status… Community interests… The future experiments…

2 The DESIR physics workshop 73 delegates 23 institutions 12 countries ½ + 1 + ½ days, 4 sessions – the facilities, BESTIOL, LUMIERE, traps OUTCOMES: reported today and, http://www.cenbg.in2p3.fr/desir/spip.php?rubrique82 http://www.cenbg.in2p3.fr/desir/spip.php?rubrique82

3 APPENDIX III: DESIR collaboration agreement After the construction of the DESIR infrastructure (RFQ cooler SHIRaC, high-resolution separator HRS, beams lines from S1, S2, and S3 to DESIR), the DESIR collaboration proposes the installation of a certain number of general equipment (stable ion sources, identification station, general-purpose ion buncher GPIB) which will be available to all experiments. This equipment will be provided by the collaboration as a whole or by different groups and financed by different means (ANR, regional grants etc.). Part of the equipment necessary to perform experiments in DESIR exists already or is presently built and commissioned. Other parts will be constructed in the next few years. This equipment is financed by different parts of the DESIR collaboration and will be installed permanently or for longer periods in the DESIR hall. Details of this process will be fixed in a Memorandum of Understanding which is presently being elaborated.

4 The DESIR physics workshop Introduction... Present experiments and equipment... The future experiments and interest...

5 A/q=6 Injector option DESIR Facility low energy RIB DESIR Facility low energy RIB HRS+RFQ Cooler RIB Production Cave Up to 10 14 fiss./sec. RIB Production Cave Up to 10 14 fiss./sec. A/q=3 HI source Up to 1mA A/q=3 HI source Up to 1mA A/q=2 source p, d, 3,4 He 5mA A/q=2 source p, d, 3,4 He 5mA LINAC: 33MeV p 40 MeV d 14.5 AMeV HI LINAC: 33MeV p 40 MeV d 14.5 AMeV HI SP2 Beam time: 44 weeks/y GANIL Beam time: 35 weeks/y ISOL RIB Beams: 28-33 weeks/y GANIL+SP 2 Users: 700-800/y SP2 Beam time: 44 weeks/y GANIL Beam time: 35 weeks/y ISOL RIB Beams: 28-33 weeks/y GANIL+SP 2 Users: 700-800/y GANIL/SPIRAL1/SPIRAL2 facility GANIL/SPIRAL 1 today GANIL/SPIRAL 1 today CIME cyclotron RIB at 1-20 AMeV (up to 9 AMeV for fiss. fragments) S3 separator- spectrometer Neutrons For Science SPIRAL2 is one of the ESFRI list projects (40 most important EU research infrastructure projects) Cost: 200M€ Funded Cost: 200M€ Funded

6 DESIR (typical example) 29 weeks of RIB/year: 10 weeks of ISOL RIB from SPIRAL2, 4 weeks from S3, 15 weeks from SPIRAL1 DESIR (typical example) 29 weeks of RIB/year: 10 weeks of ISOL RIB from SPIRAL2, 4 weeks from S3, 15 weeks from SPIRAL1 Beamtime…

7 The DESIR physics workshop Introduction... Present experiments and equipment... The future experiments and interest...

8 New experimental setup for  2p emission : The Silicon Cube I. Matea et al, Nucl. Instr. and Meth. A 607 (2009) 576  High granularity with 1536 pixels  Angular coverage  54% for one proton detection  29% for two-proton detection  6 DSSSD with 16x16 strips  6 silicon detector behind  192 electronics channels  3 EXOGAM clovers P. Ascher

9 M. B. Gómez et al. UPC, Barcelona SIMULATION VALIDATION WITH 252 Cf SOURCE IN UPC LAB Wall effect 190 keV Noise Wall effect 575 keV Full energy 765 keV Exp %MCNPX %GEANT4 % Inner crown21.3 ± 3.221.3 ± 1.525.0 ± 1.6 Outer crown4.9 ± 0.76.0 ± 0.85.4 ± 0. 7 Tot26.1 ± 3.927.3 ± 1.730.4 ± 1.7 Experimental uncertainty due to source activity uncertainty (15%) 252 Cf neutron energy distribution

10 TAGS uses large 4  scintillation detectors, aiming to detect the full  -ray cascade rather than individual  -rays Deconvolution with spectrometer response to decay spectrum strength An ideal TAS would give directly the  -intensity I  Response from MC simulations and nuclear statistical model  Clean sources & minimum of statistics J.L. Tain

11 T. Cocolios

12 Pumping in the cooler: G. Neyens, K. Flanagan, B. Cheal, F. Charlwood, P. Campbell

13 1.9 m neutralizer re-ionizer unpolarized A Na +1 30 keV polarized A Na +1 B 10Gauss C.D.P. Levy et al. Nucl. Instr. and Meth. B204 (2003) 689 TRIUMF ISAC Polarized Beam Line pumping within 2.6  s beam velocity tuning polarized A Na 0 Kiefl 8 Li: longitudinal  -NMR condensed matter physics Kiefl 8 Li: transverse  -NMR condensed matter physics Shimoda A Na: transverse 11 Li: transverse decay spectroscopy two frequency laser beams T. Shimoda

14  - n,  - n-  - , coincidence Li-glass scintillator: Δ  n = 0.92% x 5,  n =2.1%@15 keV,  n = 1.3%@80 keV En ≧ 1 keV Flight Length: 130 mm Ge detector: HPGe, 50 and 60 %,  Δ     = 3.2x10 @3 MeV plastic scintillator: Δ  n = 1.8% x 6,  n = 19%@2 MeV, En ≧ 500 keV Flight Length: 1.5 m  -ray telescope: Δ   = 14.7% x 2,   = 90% -3 E n = 1 keV – 9 MeV Experiment at TRIUMF (E903) 11 Li gs 11 Be*+  10 Be* + n 10 Be gs +  30.5 keV 50% polarization  -decay asymmetry

15 Status of MLLTRAP - 7T trap magnet, identical to SHIPTRAP, JYFLTRAP Status: - operational with  m/m~5. 10 -8 (without systematic errors) - systematic effects on B field studied DESIR Workshop, Leuven, May 26-28, 2010 P. Thirolf, D. Lunney

16 12/17/2015 16 [ O. Naviliat-Cuncic & N.S., Phys. Rev. Lett. 102 (2009) 142302 reduce by new measurements of Ft values and correlation coefficients E. Lienard, N. Severijns

17 The DESIR physics workshop Introduction... Present experiments and equipment... The future experiments and interest...

18 146 Gd 100 Sn 2 nd FP 1 st FP A~74 N~Z Existing TAS measurements 132 Sn 78 Ni 100 Sn Superallowed Proposed TAS measurements Nuclear structure @ magic nuclei Astrophysics: r-process Fundamental physics Reactor decay-heat Reactor neutrino-spectrum

19 Motivation GT- resonance is close to Q β window Complementary to earlier studies using high resolution (Leuven group) ~ 78 Ni

20 Mass scan Measured TAS spectra Measurement of Nb, Mo and Tc isotopes for Reactor Decay Heat IGISOL separator + ion guide source: refractory elements JYFLTRAP Penning trap: isotopic purification TAS measurements @ Univ. Jyvaskyla Valencia, Jyvaskyla, Debrecen, Gatchina, Surrey

21 122 Pd 128 Cd 135 Sn 140 Te 146 Xe 130 Cd from Q  (ISOLDE) PRL 91(2003)162503 Penning trap data SPIRAL2 hunting for odds

22

23 Candidate: 257 Rf DESIR Workshop, Leuven, May 26-28, 2010 SHIPTRAP: 2010 : 255 Lr 255 No, 256 Lr: ~ 100 nb

24 12/17/201524 N. Severijns, DESIR Workshop - Leuven - May 26-28, 2010 37 K – D. Melconian, J.A. Behr et al., Phys. Lett. B 649 (2007) 370 M W 2 > 180 GeV/c 2 (90 % C.L.) Example of polarized atoms in MOT: neutrino asymmetry parameter for 37 K 5 % precision very difficult to determine nuclear polarization precisely ! TRINAT MOT trap @ TRIUMF

25 The DESIR physics workshop Introduction... Present experiments and equipment... The future experiments and interest...

26 APPENDIX III: DESIR collaboration agreement After the construction of the DESIR infrastructure (RFQ cooler SHIRaC, high-resolution separator HRS, beams lines from S1, S2, and S3 to DESIR), the DESIR collaboration proposes the installation of a certain number of general equipment (stable ion sources, identification station, general-purpose ion buncher GPIB) which will be available to all experiments. This equipment will be provided by the collaboration as a whole or by different groups and financed by different means (ANR, regional grants etc.). Part of the equipment necessary to perform experiments in DESIR exists already or is presently built and commissioned. Other parts will be constructed in the next few years. This equipment is financed by different parts of the DESIR collaboration and will be installed permanently or for longer periods in the DESIR hall. Details of this process will be fixed in a Memorandum of Understanding which is presently being elaborated.

27 The major equipment consists of stable ion sources and a general purpose ion buncher (D. Lunney et al.) with a total investment cost of 250 k€ an identification station with tape drive and associated detectors (Ph. Dessagne et al.) with a total investment cost of 100 k€ a Penning trap system for mass measurement (the MLLTRAP) provided by the Ludwig- Maximilian University of Munich (P. Thirolf et al.) with a total investment cost of about 700 k€ a magneto optical trap for studies “beyond the standard model” proposed by KVI Groningen (H. Wilschut et al.) with an investment cost of 500 k€ the LPCTRAP for weak-interaction studies (G. Ban et al.) with a total investment cost of 225 k€ a Collinear Laser-Spectroscopy setup (the LUMIERE facility) provided by the University of Leuven (G. Neyens et al.), the University of Manchester (P. Campbell et al.) and the IPN Orsay (F. Le Blanc) with a total investment cost of 970 k€ a total absorption gamma spectrometer provided by CSIC Valencia (J.L. Tain et al.) with a total investment cost of 425 k€ the TETRA neutron multiplicity setup proposed by JINR Dubna (Y. Penionzhkevich et al.) with an investment cost of 200 k€ a neutron time-of-flight spectrometer provided by a CIEMAT (D. Cano Ott et al.) - LPC Caen (N. Orr et al.) collaboration with an investment cost of 445 k€ a double Penning trap system for beam purification and preparation proposed by CEN Bordeaux-Gradignan (B. Blank et al.) with a total investment cost of 750 k€ a fast-timing setup provided by a collaboration led by G. Simpson (LPSC Grenoble) with an investment cost of 50 k€ a 4p charged particle array proposed by CEN Bordeaux-Gradignan (B. Blank et al.) and CSIC Madrid (M.J.G. Borge et al.) with a total investment cost of 130 k€

28 The DESIR physics workshop The range of beam... The beamtime... The timing...

29 DESIR (typical example) 29 weeks of RIB/year: 10 weeks of ISOL RIB from SPIRAL2, 4 weeks from S3, 15 weeks from SPIRAL1 DESIR (typical example) 29 weeks of RIB/year: 10 weeks of ISOL RIB from SPIRAL2, 4 weeks from S3, 15 weeks from SPIRAL1 Beamtime…

30 Beamtime


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