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Coulomb Excitation Studies of Radioactive 20,21 Na

TRIUMF/ISAC2. Coulomb Excitation Studies of Radioactive 20,21 Na. Douglas Cline for the TIGRESS Collaboration CAP Congress; Saskatoon, June 18, 2007. Bambino. SCIENTIFIC GOALS: Recommendations of the 2007 NSAC Long-Range Plan.

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Coulomb Excitation Studies of Radioactive 20,21 Na

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  1. TRIUMF/ISAC2 Coulomb Excitation Studies of Radioactive 20,21Na Douglas Cline for the TIGRESS Collaboration CAP Congress; Saskatoon, June 18, 2007 Bambino

  2. SCIENTIFIC GOALS: Recommendations of the2007 NSAC Long-Range Plan Reaffirmed construction of a next-generation radioactive beam facility which is central to nuclear science. It will allow study of nuclei far from stability and address the following fundamental questions: • What is the nature of the nuclear force binding stable and exotic nuclei? • What is the origin of simple patterns in complex nuclei? • What is the nature of neutron stars and dense nuclear matter? • What is the origin of the elements in the cosmos? • What are the nuclear reactions that drive stars and stellar explosions? CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  3. How does structure evolve at extremely large neutron number? CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  4. Supernova E0102-72.3 n-Star KS 1731-260 Impact of Nuclear Structure on nucleosynthesis X-ray burst p process s-process 4U1728-34 331 330 Frequency (Hz) r process 329 328 327 10 15 20 Time (s) rp process Nova Crust processes T Pyxidis stellar burning protons Thanks to Witek Nazarewicz, U. Tennessee neutrons

  5. THE SCIENCE • Probe collective and single-particle properties of exotic nuclei • Eλ and M1 matrix elements are sensitive probes of both collective and single-particle degrees of freedom in exotic nuclei. • Fast recoiling exotic nuclei, produced by projectile fragmentation, have been used in pioneering measurements of “B(E2:2+→0+) “ values in nuclei far from stability via unsafe Coulomb excitation. • Current goal is to Coulomb excite exotic beams at safe bombarding energies where the reaction mechanism is fully known allowing accurate determination of Eλ and M1 transition strengths plus static E2 and M1 matrix elements of excited states. CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  6. COULOMB EXCITATION • Coulomb excitation is the preeminent probe of collective shape degrees of freedom: • Selectively populates collective states in the yrast domain • Reaction mechanism fully understood if below the Coulomb barrier • The cross sections are directly and unambiguously related to the Eλ matrix elements • The Eλ matrix elements are the most direct measure of λ-pole collectivity CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  7. Major advances in the Coulomb Excitation Technique • Availability of prolific source of ~ 4.5 MeV/A variable energy exotic heavy-ion beams; TRIUMF/ISAC2 • 2. Development of powerful γ-raydetector and heavy-ion systems for high-resolution γ-ray spectroscopy: TIGRESS, Bambino • Development of the Coulomb excitation least-squares search code GOSIA* • *[Czosnyka, Cline, Wu, 1980] CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  8. Coulomb Excitation Technique • Experimental Method: • Use thin targets so that excited nuclei recoil in vacuum • Measure scattering angles and velocities of recoiling ions over a wide range of scattering angles • Detect deexcitation γ-rays in coincidence with the scattered ions. • Normalize projectile excitation to target excitation using an accurately known B(E2) • Deduce: • Masses and velocity vectors of recoiling ions, reaction Q-value • Correct for Doppler shift of de-excitation γ-rays on an event-by-event basis • Identify which γ-raysare emitted by each recoiling ion • Determine Coulomb excitation cross sections to excited states as function of impact parameter. • Use GOSIA2 to extract individual electromagnetic matrix elements from measured yields for both target and projectile excitation. CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  9. Coulomb excitation observables • Determine B(E2), B(E3), and B(M1) values • Determine sign and magnitude of static E2 moments of excited states • Determine signs and magnitudes of observable products of Eλ matrix elements • May extract M1 moments of excited states from the measured attenuation of the γ-ray angular correlations for ions recoiling in vacuum CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  10. High b SCRF Med b SCRF Low b SCRF DTL2 TIGRESS @ ISAC-II ISAC TIGRESS @ ISAC-I SC LINAC 0.15 – 5.0 MeV/A Accelerated Beam 0.15 – 1.7 MeV/A DTL1 Thick/Hot Target high-energy proton beam Ion Source RFQ Production Accelerator TRIUMF 500 MeV Cyclotron 100 mA 8p Spectrometer Ion Beam 60 keV Isotope Separator

  11. TRIUMF • ISAC • Gamma • Ray • Escape • Suppressed • Spectrometer A Next-Generation Gamma-Ray Spectrometer for ISAC-II CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  12. TIGRESS Twelve 32-fold segmented Clover Detectors Four 40% HPGe crystals per clover. Maximum Efficiency Optimal Suppression rGe = 11.0 cm eg = 17% @ 1 MeV rGe = 14.5 cm rBGO = 11.0cm

  13. Bambino Si CD Heavy-ion detector (LLNL; Rochester) • Forward and backward annular Si CD heavy-ion detectors • Angular coverage: • 20o < θ < 50o, 130o < θ < 160o • 00 < φ < 315o • Angular resolution; • Δθ = 1.22o, Δφ = 22.5o CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  14. First TIGRESS Experiment: Coulomb excitation of 20,21Na, 21Ne • Technical Goal: • Commission TIGRESS, Bambino, Digital signal-processing data acquisition system • Evaluate optimal geometry, technique, and backgrounds. • Scientific goal: • Study 5p-0h T = ½ configurations to constrain calculations of the 5p-2h 3/2+ resonance at 4.033 MeV in 19Ne. This resonance could provide a gateway from the hot-CNO cycle to the rp-process in nova, x-ray bursts. • NB: • Accurate lifetime measurements of the first excited 5/2+ states are available • Neither 21Na and 21Ne have been Coulomb excited previously. • Inaccurate E2/M1 mixing ratios poorly determine the B(E2) transition strengths. • For 21Na the B(E2:5/2→3/2)* = 48 ± 41 e2fm4 * R.B. Firestone, Nuclear Data Sheets 103 (2004)269 plus NNDC 10/10/2006 erratum CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  15. First TIGRESS Experiment: Coulomb excitation of 20,21Na, 21Ne • Performed August 2006 using ISAC1, ran one week each for 21Na and 20Na • 1.700 MeV/A beams, incident upon a 520μg/cm2NatTi self-supporting target • 108 ions/second of 21Na was available. Electronics limited beam to 5 x 106 ions/second • 2 x 106 ions/second of 20Na delivered on target • Used two TIGRESS modules at θ = ±900 plus Bambino at 20o < θHI <50o CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  16. First TIGRESS Experiment: Coulomb Excitation of 20-21Na,21Ne, Aug 2006 1x10cm collimator Bambino Θ = 20-50o plastic scintillator Pb shielding

  17. Digital Data Acquisition Fully Implemented: 160 Channels of custom 14 bit, 100 MHz digitizers 2 HPGe clovers + BGO suppressors Silicon CD-S2, 4 TIG-10 cards 2 collector cards + master TIG-C

  18. 21Ne, 21Na Heavy-ion gated γ-ray Spectra • Clean γ-ray spectra with negligible influence of 511 keV due to intense beam β+ activity • For Ti Doppler correction shows both 46Ti and 48Ti 2+ decay transitions CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  19. Analysis of Yields with GOSIA • γ ray yields were measured in coincidence with θ and φ gates on the recoiling ions. • Matrix elements were fit to the measured yields using the GOSIA search code assuming the following level scheme. R.B. Firestone, Nuclear Data Sheets 103 (2004) 269. CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  20. Comparison of data with GOSIA for 48TiAnalyzed assumingB(E2;2+ → 0+) = 144 (8) e2fm4 21Ne Beam 21Na Beam ← vs q → 2+ 984 keV 0+ 48Ti GOSIA GOSIA ← vs f → CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  21. 21Ne Coulomb Excitation Preliminary B(E2)↓for 5/2+ → 3/2+g.s. (e2fm4) Present Measurement 80 ± 6 Previously Accepted 83 ±10 351 keV GOSIA CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  22. 21Na Coulomb Excitation Preliminary B(E2)↓for 5/2+ → 3/2+g.s. (e2fm4) Present Measurement 124 ± 9 Previous 48 ±41 332 keV GOSIA CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  23. Comparison of Results with Prior Work [1] R.B. Firestone, Nuclear Data Sheets 103 (2004) 269 with NNDC 10/10/2006 erratum CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  24. Interpretation of E2 Collectivity in 20 < A < 24 nuclei Weisskopf E2 single-particle estimate: • Observations: • Strong E2 enhancement ranging from 9.8 to 36 • A major fraction of nuclear charge involved in collective motion • Can these data be correlated assuming quadrupole collective deformation ? CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  25. Macroscopic quadrupole rotor model interpretation: E2 K = 3/2+ K = 0+ • Observations: • Data correlated well by the simple macroscopic prolate quadrupole rotor model. • For each nucleus the β2 values agree within the errors • The β2 values depend smoothly with a maximum for T = 0 CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  26. Macroscopic quadrupole rotor model interpretation: M1 • Observation: • Collective model correlates the M1 data moderately well. CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  27. Microscopic shell model interpretation Shell model predictions in the complete 2s-1d shell were made using OXBASH plus the USD residual interaction. Effective charges of en = 0.5e and ep = 1.5e were used to account for core polarization. [C. Barbieri, Private communication] • Observations: • Observe BE2 in 21Na is stronger than in 21Ne as is predicted. • Shell model B(E2) values require a slightly larger polarization charge • Shell model B(M1) values require to be slightly quenched. CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  28. Science implications for 21Ne and 21Na • The measured B(E2;5/2+→3/2+) values in 21Na and 21Ne are strongly enhanced. • The implied very large prolate quadrupole deformation leads to the E2 properties that are correlated well by the naïve quadrupole collective rotor model. • The large effective deformations derived assuming the naïve quadrupole rotor model are consistent with values in nearby even-even mass nuclei 20, 22Ne and 24Mg • The M1 properties also can be understood by the collective model. • Microscopic shell model calculations in the 2s-1d valence space are able to predict the strong quadrupole collectivity if a large polarization charge is assumed. CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  29. Coulomb Excitation at the Proton-Dripline: 20Na Involved in the CNO breakout via: 15O(a,γ)19Ne(p,γ)20Na Spectroscopy performed using GS+FMA; D. Seweryniak et al., PLB 590, 170 (2004) No transition matrix elements are known Gated p-γ TIGRESS spectrum 199 799 799 4+ 600 600 3+

  30. CONCLUSIONS • TIGRESS commissioning experiments at ISAC-1 were a tremendous success • Intense radioactive beams of 20, 21Na produced by TRIUMF/ISAC-1 • TIGRESS and Bambino, plus the digital signal-processing system performed well. • The technique provided high-quality and significant scientific results. This bodes well for the planned exotic beam Coulomb excitation program at TIGRESS CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  31. Acknowledgements M.A. Schumaker1, A. Andreyev2, R.A.E. Austin3, G.C. Ball2, D. Bandyopadhyay1, C. Barbieri2, J.A. Becker4, A.J. Boston5, H.C. Boston5, R. Churchman2, F. Cifarelli2, D. Cline6, R.J. Cooper5, D.S. Cross7, D. Dashdorj8, G.A. Demand1, M.R. Dimmock5, T.E. Drake9, P. Finlay1, A.T. Gallant3, P.E. Garrett1,2, K.L. Green1, A.N. Grint5, G.F. Grinyer1, G. Hackman2, L.J. Harkness2,5, A.B. Hayes6, R. Kanungo2, K.G. Leach1, G. Lee2,9, R. Maharaj2, J-P. Martin10, F. Moisan11, A.C. Morton2, S. Mythili2,12, L. Nelson5, O. Newman2,13, P.J. Nolan5, E. Padilla-Rodal2, C.J. Pearson2, A.A. Phillips1, M. Porter-Peden14, J.J. Ressler7, R. Roy11, C. Ruiz2, F. Sarazin14, D.P. Scraggs5, C.E. Svensson1, J.C. Waddington15, J.M. Wan7, A. Whitbeck6, S.J. Williams2, J. Wong1, C.Y. Wu4 1Department of Physics, University of Guelph, Guelph, Ontario, N1G 2W1, Canada 2TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia, V6T 2A3, Canada 3Department of Astronomy and Physics, St. Mary's University, Halifax, NS, B3H 3C3, Canada 4Lawrence Livermore National Laboratory, Livermore, California, 94551, U.S.A. 5Department of Physics, University of Liverpool, Liverpool, L69 7ZE, U.K. 6Department of Physics and Astronomy, University of Rochester, Rochester, NY, 14627, U.S.A. 7Department of Chemistry, Simon Fraser University, Burnaby, British Columbia, V5A 1S6, Canada 8Department of Physics, North Carolina State University, Raleigh, North Carolina, 27695, U.S.A. 9Department of Physics, University of Toronto, Toronto, Ontario, M5S 1A7, Canada 10Département de Physique, Université de Laval, Québec, Québec, G1K 7P4, Canada 11Département de Physique, Université de Montréal, Montréal, Québec, H3C 3J7, Canada 12Department of Physics and Astronomy, University of British Columbia, BC, V6T 1Z1, Canada 13Department of Physics, University of Surrey, Guildford, Surrey, GU2 7XH, U.K. 14Physics Department, Colorado School of Mines, Golden, Colorado, 80401, U.S.A. 15Department of Physics, McMaster University, Hamilton, Ontario, L8S 4L8, Canada Funding provided by: Natural Sciences and Engineering Research Council of Canada U.S. Department of Energy through University of California, Lawrence Livermore National Laboratory U.S. Department of Energy U.S. National Science Foundation U.K. Engineering and Physical Sciences Research Council TRIUMF funded by the National Research Council of Canada CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  32. CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  33. TIGRESS FUTURE PLANS July-August 2007: - Coulomb excitation of 28,29Na beams from ISAC-II - 6 TIGRESS modules plus two Bambino Si CD detectors 2008 → ISAC-II: - Charge-state booster will allow A < 150 beams - Actinide target will produce higher isotopic yields TIGRESS: - 12 detector modules completed in 2009 Auxiliary detectors: - SuperCHICO (LLNL, Rochester) - DESCANT, deuterated scintillator neutron detector array (Guelph) - EMMA, a recoil mass spectrometer (TRIUMF) - Bragg detector (York) - DSSD Barrel (York, Colorado) - CsI(Tl) (St Mary’s) CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

  34. Semiclassical least-squares Coulomb excitation search code GOSIA T. Czosnyka, D. Cline, C.Y. WuUniversity of Rochester Developed in 1980 at Rochester. Codes and manual for GOSIA can be obtained from the website: http://www.pas.rochester.edu/~cline/Research/index.html Look under links > Techniques > GOSIA to obtain: • GOSIA MANUAL: Describes the June 2007 version of the complete set of GOSIA codes • GOSIA UPDATES: Lists the most recent updates to the GOSIA Manual and associated codes. • GOSIA CODES: • GOSIA is the Fortran source code for the June 2006 version of the basic code. • GOSIA2is the Fortran source code for the June 2006 version of a special version of GOSIA designed for use when analyzing simultaneous Coulomb excitation with a common normalization. This is useful for determining transition strengths in radioactive beams by normalization to a known transition strength in the target. • PAWELis the Fortran source code for the June 2006 version of a special offspring of GOSIA designed to handle cases where a fraction of the nuclei have an excited isomeric state as the initial state. • ANNL is a special version of GOSIA, developed by Rich Ibbotson, that uses simulated annealing techniques to locate minima. • SIGMA is the Fortran source code for deducing the quadrupole invariants from the E2 matrix elements determined by GOSIA. CAP Congress Saskatoon, 18 June 2007 Douglas Cline for TIGRESS Collaboration

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