Experiments with rare isotopes The limits of experiments at the limits of stability Thomas Glasmacher Michigan State University The 2nd LACM-EFES-JUSTIPEN.

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Presentation transcript:

Experiments with rare isotopes The limits of experiments at the limits of stability Thomas Glasmacher Michigan State University The 2nd LACM-EFES-JUSTIPEN Workshop Joint Institute for Heavy Ion Research, Oak Ridge, Tennessee, USA Oak Ridge National Laboratory January 23-25, 2008

Progress Our shared goal: To develop a predictive theory of atomic nuclei and their reactions Calculated observable Measured observable NatureInsight Optimize progress by investing resources wisely: Measure observables that can (in principle) be calculated Calculate observables that (in principle) can be checked in experiments

Rare isotopes are a wise investment and Tasks for experimenters Stable nuclei are well-described with closed-shell nuclei as key benchmarks Rare isotopes show evidence for – disappearance of canonical shell gaps, – appearance of new shell gaps, – reduction of spin-orbit force, – influence of continuum states Experimental task: Quantify changes encountered in rare isotopes and measure with defined certainty observables that are calculable and can be used to discriminate between theories

Facts of life for experimentalists N obs /   N R  N T × N B ×  beamtarget reacted beam N obs observed reactions  detection efficiency N R reaction rate N T atomic density of target N B beam rate  cross section

Facts of life for experimentalists N obs /   N R  N T × N B ×  beamtarget reacted beam N obs observed reactions  detection efficiency N R reaction rate N T atomic density of target N B beam rate  cross section Build more efficient detectors Use targets with more scattering centers Make more beam Given by nature

Experimental observables in experiments with in-flight produced rare isotope beams Stopped beam experiments Possible experiments and quality of observables depend on number of beam particles Possible experiments and quality of observables depend on number of beam particles Discovery (few particles total) Half live (few ten particles) Mass (few hundred particles) Fast beam experiments Possible experiments and quality of observables depend on luminosity Possible experiments and quality of observables depend on luminosity Interaction radii (few particles per hour) g-factors (hundreds of particles per second) Fast beam experiments (cont’d) Excited state energies, transition matrix elements – Elastic and inelastic scattering (ten particles per second) Electromagnetic Hadronic – Lifetimes from  -ray line shapes (hundreds of particles per second) Occupation numbers – Nucleon removal Single nucleon (particles per second) Two-nucleon (hundreds of particles per second) Multi-nucleon (hundreds of particles per second) – Nucleon addition (hundreds of particles per second)

Stopped beam experiment: Discovery of new isotopes near the n-dripline: 40 Mg, 42 Al, 43 Al, 44 Si S800 analysis line 4 x Ca beam particles Two-stage separator (one-stage did not provide sufficient clean-up) First observation of 40 Mg (3 events), 42 Al, 43 Al :GANIL Guillemaud-Mueller et al., Z. Phys. A 332, :GANIL Tarasov et al., Phys. Lett. B 409, :RIKEN Sakurai et al., Phys. Lett. B 448, :RIKEN Notani et al., Phys. Lett. B 542, 49 GANIL Lukyanov et al., J. Phys. G 28, L : NSCL Tarasov et al, Phys. Rev. C 75 (2007) ; Baumann et al, Nature 449 (2007) 1022

Stopped beam experiment: Mass measurement Stop fast exotic beams in gas cell, extract, and use in experiments 38 Ca: T 1/2 = 440 ms, 0 +  0 +  + -emitter –new candidate for the test of the conserved vector current (CVC) hypothesis ME LEBIT = (28) keV  m = 280 eV,  m/m=8·10 -9 –AME 03:  m = 5 keV Penning trap mass measurements of rare isotopes produced in-flight: Since Summer 2005: 33 Si, 29 P, 34 P 37 Ca, 38 Ca 40 S, 41 S, 42 S, 43 S, 44 S 63 Ga, 64 Ga 64 Ge, 65 Ge, 66 Ge 66 As, 67 As, 68 As, 80 As 68 Se, 69 Se, 70 Se, 81 Se, 81m Se 70m Br, 71 Br 66 As: T 1/2 = 96 ms LEBIT:  m  20 keV,  m/m  3x10 -7 –20-fold improved masses in region critical to rp process G. Bollen et al. Phys. Rev. Lett. 96 (2006)

Exploring the boundaries of Island of Inversion C. Thibault et al: PRC 12 (1975) ,32 Na, local increase of S 2n  N=20 shell gap decreased X. Campi et al: NPA 251(1975) 193 explained by deformation via filling of (f 7/2 ) C. Detraz et al: PRC19 (1979) Na  32 Mg  decay, low 2 + in 32 Mg E. Warburton et al: PRC 41 (1990) 1147 Z=10-12 and N=20-22 have ground state wavefunctions dominated by (sd) -2 (fp) +2 configurations T. Motobayashi et al: PLB 346 (1995) 9 large B(E2;0 +  2 + ) in 32 Mg See also 29 Na V. Tripathi et al. Phys. Rev. Lett. 94 (2005) (2005) 31 Mg G. Neyens et al. Phys. Rev. Lett. 94 (2005) (2005) 27 Ne A. Obertelli et al., Phys. Lett B 633 (2006) Ne H. Iwasaki et al., Phys.Lett. B 620 (2005) Al P. Himpe, G. Neyens et al. Phys.Lett. B 658 (2008) 203 Single-neutron removal to look for negative parity states, indicating the presence of f 7/2 intruder configurations in the ground state of the parent: ( 30 Mg, 29 Mg+  ) ( 26 Ne, 25 Ne+  ) ( 28 Ne, 27 Ne+  ) ( 38 Si, 36 Mg+  ) two-proton removal

Single-neutron removal from 26,28 Ne and 30 Mg 25 Ne level structure known A.T. Reed et al., PRC 60 (1999) S. Padgett et al., PRC 72 (2005) Ne is well-described in sd shell with no evidence for intruder states below 3 MeV → No evidence for intruder configurations in the ground state wave function of 26 Ne J.R. Terry et al., Phys. Lett. B 640 (2006) Na 32 Na 33 Na 34 Mg 32 Ne 31 Ne 30 Ne 32 Mg 33 Mg 29 Ne 28 Ne 27 Ne 26 Ne 25 Ne - 1n N=20

Single-neutron removal from 26,28 Ne and 30 Mg allows for intruder configurations sd shell only 31 Na 32 Na 33 Na 32 Ne 31 Ne 30 Ne 32 Mg 33 Mg 29 Ne 28 Ne 27 Ne 26 Ne 25 Ne -1n 34 Mg

Single-neutron removal from 26,28 Ne and 30 Mg J.R. Terry et al., Phys. Lett. B 640 (2006) 86 → Ground states for 28 Ne, 30 Mg have significant 2h  f 7/2 intruder configurations See also 31 Mg G. Neyens et al. Phys. Rev. Lett. 94 (2005) (2005) 27 Ne A. Obertelli et al., Phys. Lett B 633 (2006) = 0,1 excited states

36 Mg g.s. dominated by 2h  configurations 38 Si pnpnpn + Monte-Carlo Shell Model (MCSM) calculations: SDPF-M interaction of Y. Utsuno, T. Otsuka et al. 38 Si: no significant intruder configurations in g.s. 36 Mg: MCSM predicts strong intruder admixtures for the low-lying states 2p knockout from 38 Si reaches only 0h  components in 36 Mg Comparison of measured cross sections and those calculated assuming the population of 0h  components of the final states by the direct 2p knockout reaction: Only 32(8)% and 38(8)% of the w.f. of the g.s. and 2 + state, respectively, are 0h  components, the rest is proposed to be of intruder character Intruder domination places 36 Mg inside the “Island of Inversion” A Gade et al., Phys. Rev. Lett. 99, (2007) Reaction theory: J.A. Tostevin and B.A. Brown, PRC 74, (2006), N=20

Proton scattering in inverse kinematics Many experiments at GANIL (MUST detector) Some experiments at MSU Thin target to avoid angular and energy straggeling of low-energy protons p( 56 Ni,p’) at GSI G. Kraus et al., PRL 73 (1994) 1773 Normal kinematics Inverse kinematics F. Maréchal et al., PRC 60 (1999)

Inelastic scattering to measure transition rates: Thick-target  -tagged inelastic proton scattering Pioneering experiment at RIKEN p( 30 Ne, 30 Ne  ) Y. Yanagisawa et al. PLB 566 (2003) 84  Hydrogen has the most scattering centers per energy loss  Inelastic p scattering using two cocktail beam settings to study chains of isotopes accessible in a consistent approach  Determine excited state energies and collectivity towards N=28  Univ. Tokyo, RIKEN, Rikkyo Univ., Michigan State Univ. collaboration 40 Si N Z 36 Si Sulfur Silicon RIKEN/Kyushu/Rikkyo LH 2 target: H. Ryuto et al., NIM A 555 (2005) 1 30 mm diameter 9 mm thick, nominal Negligible contaminant reactions

Evolution of 2 + energies towards N=28 Above Z=20 Ti, Cr and Fe Below Z=20 Si, S and Ar 40 Si 986(6) keV 1.5 million 40 Si beam particles  p,p’ = 20(3) mb ~30 counts in the photopeak Low energy indicative of neutron collectivity in 42 Si C.M. Campbell et al., PRL 97 (2006) Discovery of low-lying 2 + state in 42 Si at GANIL B. Bastin, S. Gr é vy et al. PRL 99, (2007)

Higher excited states in 40 Si Two additional  -rays in fragmentation channel 42P-p-n – States at 1.62(1) MeV and 1.82(1) MeV? Not enough statistics to test if the two transitions are in coincidence Independent of the sequence, the second excited state is low in energy In the shell model second excited state is ph-excitation across N=28 Low energy supports narrowing of the N=28 gap in 40 Si C.M. Campbell et al., PRL 97 (2006)

Evolution and character of collectivity Prior data from F. Maréchal et al, PRC 60, (1999) P.D. Cottle et al., PRL 88, (2002) N N Rotational limit Vibrational limit Sulfur Silicon Enhanced collectivity towards N=28 in silicon Sulfur transitions from vibrational mid-shell to rotational towards N=28 Silicon vibrational mid-shell C.M. Campbell Ph.D. PLB 652 (2007) 169

Nucleon addition complements knockout Traditionally performed in normal kinematics at lower beam energies, e.g. (d,n), ( 3 He,d), ( ,t), … At higher energies momentum less well matched Trick: Pickup of a strongly-bound nucleon S. Shimoura et al., JPG 31, S1759 Pioneering inverse kinematics experiment at RIKEN, ( ,t) reaction at 60 MeV/nucleon S. Michimasa et al., PLB 638, 146 (2006) Few mb cross sections observed at intermediate energies NSCL: Pickup of a well-bound proton from 9 Be [S p ( 9 Be) = 16.9 MeV] First test case: 9 Be( 20 Ne, 21 Na  )X Inverse-kinematics proton-adding direct reactions with fast beams 9 Be( 20 Ne, 21 Na+  )X 63.4 MeV/nucleon A.M. Mukhamedzhanov et al. PRC 73 (2006) Population pattern broadly consistent with low-energy transfer reactions (and shell model) Total  =1.2 mb A. Gade et al., PRC 76 (2007) (R)

Summary and Outlook Measurements and interpretation go hand-in-hand to advance knowledge For experiments with rare isotopes, beam rates limit which observables can be measured, even after we – Build more efficient detectors – Use targets with more scattering centers – Make more beam Beam rate is the “Limit of experiments at the limits of stability” New robust experimental techniques have been developed that allow sensitive experiments with much decreased beam rates required New theoretical approaches are enabled by compute power and ingenuity New facilities are operational, under construction, and envisioned  A dawn for discovery in science of atomic nuclei

Collaborators P. Adrich a), N. Aoi c), D. Bazin a), M. D. Bowen a,b), B. A. Brown a,b), C. Campbell a,b), J. M. Cook a,b), D.-C. Dinca a,b), A. Gade a,b), M. Horoi d), S. Kanno e), K. Kemper k), T. Motobayashi c), A. Obertelli a), T. Otsuka a,c,h), L. A. Riley f), H. Sagawa g), H. Sakurai c), K. Starosta a,b), H. Suzuki h), S. Takeuchi c), J. R. Terry a,b), J. Tostevin i), Y. Utsunoi j), D. Weisshaar a), K. Yoneda c), H. Zwahlen a,b) a) National Superconducting Cyclotron Laboratory, Michigan State University b) Department of Physics and Astronomy, Michigan State University c) RIKEN Nishina Center for Accelerator-Based Science d) Physics Department, Central Michigan University e) Department of Physics, Rikkyo University f) Department of Physics and Astronomy, Ursinus College g) Center for Mathematical Sciences, University of Aizu h) Department of Physics, University of Tokyo i) Department of Physics, University of Surrey j) Japan Atomic Energy Research Institute k) Physics Department, Florida State University

Intermediate-energy Coulomb excitation of 32 Mg Large transition matrix element indicates breakdown of the N=20 shell gap Experiment: Max.  determines min. impact param. Impact parameter Scattering angle   Coul = 87 mb  B(E2 ↑ ) = 454(78) e 2 fm 4 =   2 | = 0.49(4) Shell model Valence nucleon model T. Motobayashi, R. Casten et al., Phys. Lett. B 346 (1995) 9 T.G. Ann. Rev. Nucl. Part. Sci. 48 (1998) 1

E2 transition strengths in 32,34 Mg 34 Mg Rate 10 atoms/s, run time 96 hrs, APEX detector 32 Mg B(E2  ) in agreement with RIKEN, MSU results 26 Mg B(E2  ) in agreement with adopted value 34 Mg E(2 + ) and B(E2  )=541(102) e 2 fm 4 in agreement with RIKEN result J. Church et al., Phys. Rev. C 72 (2005)

Intermediate-energy Coulomb excitation An accurate technique that allows for absolute B(E2) measurements J. Cook et al., Phys. Rev. C 73 (2006) Scheit, Gade, Glasmacher, Motobayashi, Phys. Lett. B 659 (2008) 515 Active programs at GANIL, GSI, MSU and RIKEN One-step process Sensitive to E1, E2, E3 excitations Adopted and measured B(E2  ) values for stable nuclei B(E2  ) values from different methods for 26 Mg

Structure of 23 F: Multiple reactions in one experiment ~35 MeV/nucl,100 mg/cm 2 liquid helium target at RIKEN A. Michimasa et al. Phys. Lett. B 638 (2006) He( 22 O, 23 F  ) 2000/s Proton addition 4 He( 23 F, 23 F  ) 550/s Inelastic scattering 4 He( 24 F, 23 F  ) 470/s neutron-knockout 4 He( 25 Ne, 23 F  ) 1200/s One-proton one-neutron knockout

Single-proton addition Traditionally performed in normal kinematics at lower beam energies, e.g. (d,n), ( 3 He,d), ( ,t), … Few mb cross sections observed at intermediate energies Proton well-bound in 9 Be S p ( 9 Be) = 16.9 MeV 8 Li has only one bound excited state Beam identificationReaction product identification

Measure coincident  -rays and particle momenta

Approaching the “Island”: 9 Be( 30 Mg, 29 Mg)X Level scheme of 29 Mg is known  decay and  -n decay: P. Baumann et al., PRC 36, 765 (1987) PRC 39, 626 (1989) 30 Si( 13 C, 14 O) 29 Mg and 28 Si( 13 C, 14 O) 27 Mg: C.L. Woods et al., NPA 476, 392 (1988) Levels at and MeV are assigned as 7/2- and 3/2-. Our experiment: Momentum distributions are consistent with these previous assignments and the states are directly populated in the knockout. Spectroscopic factors extracted from our data quantify intruder content in the gs of 30 Mg = 1,0 = 3,2 C 2 S extracted from experiment J. Russ Terry et al., PRC, in press p || (GeV/c)

The structure of 36 Mg via 38 Si → 36 Mg+  Beam rate too low for 36 Mg inelastic scattering and  -decay impossible ( 36 Na n-unbound) 48 Ca primary beam, Si per second secondary projectile beam (purity exceeded 95%) cross section:  =0.10(1)mb (~1 out of 400, Si) 42(6)% of the cross section to 2 +, 58(6)% to the ground state A. Gade et al., Phys. Rev. Lett. 99, (2007)