Maria J. G. Borge ISOLDE-PH, CERN (Isotope Separator On-Line) IEM-CSIC, Madrid Maria J. G. Borge , CERN,HIE-ISOLDE PH-Dept ISOLDE – High-lights and Hot Topics in Nuclear Physics Physics at the Femtometer scale 2 Open Questions in Nuclear Physics How are complex nuclei built from their basic constituents? strong interaction in nuclear medium • How to explain collective properties from individual nucleon behavior? collective versus individual LRP2010 • How do regular and simple patterns emerge in the structure of complex nuclei? Observables: symmetries Ground-state properties: mass, radius, J, μ, Q moments Half-lives and decay modes Transition probabilities Cross sections Main models: Shell model (magic numbers) Mean-field models (deformations) Ab-initio approaches (light nuclei) 3 Production of Radiactive Beams @ ISOL Facilities 4 ISOLDE Facility ISOLDE is the CERN radioactive beam facility Nuclei produced via reactions of high intensity high energy proton beam with thick and heavy targets Provides low energy or post-accelerated exotic beams PSB upgrade (2018) intensity (2uA -> 6uA ) energy (1.4 -> 2GeV) 5 ISOLDE at CERN LHC 6 Produced Nuclei: ISOLDE 45 y Experience Over 20 target materials and ionizers, depending on beam of interest operated at high temperature U, Ta, Zr, Y, Ti, Si, … 3 types of Ion-sources: Surface, Plasma, Laser > 700 nuclides of over 70 chemical elements produced Target ISOLDE today offers the largest range of available isotopes of any ISOL facility worldwide. 7 ISOLDE Physics Topics Many beams Good beam purity and quality Best in the World! High intensity Nuclear Physics Applied Physics Condensed matter physics and Life sciences Tailored Isotopes for Diagnosis and Therapy MEDICIS Project Nuclear Decay Spectroscopy and Reactions Structure of Nuclei Exotic Decay Modes Fundamental Physics Direct Mass Measurements, Dedicated Decay Studies - WI CKM unitarity tests, search for b-n correlations, right-handed currents Atomic Physics Laser Spectroscopy and Direct Mass Measurements Radii, Moments, Nuclear Binding Energies f(N,Z) Nuclear Astrophysics Dedicated Nuclear Decay/Reaction Studies Element Synthesis, Solar Processes 8 Determination of the atomic properties of Astatine Determination of ionising potential Identification of new atomic transitions Comparison with atomic theory Scan of ionizing laser: converging Rydberg levels allow precise determination of the IP ISOLDE collaborates with the Short-Lived Nuclei Laboratory which is based on the ISOL facility IRIS at PNPI since 1999. ion curre nt (p A) 30 M. Seliverstov, V. Fedoseev team IP(At) = 9.31751(8) eV Nature Com. 14May2013 36 10 20 10 0 16150 9 16 200 16250 16 300 -1 wa venu mber (cm ) 16350 Experimental hall Beams of 30-60 keV Beams of 3 MeV/u Decay spectroscopy Coulomb excitation Transfer reactions Laser spectroscopy Beta-NMR Penning traps Applications: Solide state Life Science Target stations HRS & GPS PS-Booster 1.4 GeV protons Mass-sep. HRS WITCH REX-ISOLDE 3×1013 ppp ISCOOL RILIS Travelling setups NICOLE Post-accelerated beams Collection points MINIBALL and T-REX Travelling setups COLLAPS CRIS ISOLTRAP TAS COLLAPS – Ne charge radii Laser spectroscopy & Massses Intrinsic density distributions of dominant proton FMD configurations Geithner et al, PRL 101, 252502 (‘08) Marinova et al, PRC84, 034313 (‘11) 11 ISOLTRAP: High-precision mass of 82Zn Combined ISOLDE technical know-how: neutron-converter, quartz transfer line, laser ionisation Nuclear structure: N=50 shell closure nc Astrophysics: r-process path Astrophysics: neutron star structure 1 q B 2 m Its determination is important for modelling of the crust of neutron stars , PRL110 (2013) 04110 CERN Courier, 53, n 3, 2013 12 D. Rodriguez, U. Granada The Magic Number N=32 Nature 498 (2013) 346 13 WITCH Weak Interaction Trap for Charged particles -> fundamental studies Goal: determine bn correlation for 35Ar with (a/a)stat 0.5 % Energy spectrum of recoiling ions with a retardation spectrometer Use a Penning trap to create a small, cold ion bunch June 2011 data M. Beck et al., Eur. Phys. J. A47 (2011) 45 M. Tandecki et al., NIM A629 (2011) 396 14 Gorp et al., NIM A638 (2011) 192 S. Van REX-ISOLDE Total efficiency : 1 -10 % 1+ to A/Q = 3 – 4.5 Tested A/q = 2 15 Halo Nuclei & Reactions 7Be 8Be 9Be10Be11Be12Be 6Li 7Li 8Li 9Li 10Li 11Li 3He 4He 1H 2H n 14Be 6He Common “Structural” properties Rather inert core plus one or two barely unbound extra neutrons Extended neutron distribution, large “radius”. “halo” Very few excited states –if any. Reaction properties at near-barrier energies: Is the Optical Model able to describe the scattering of the halo systems ? r2 11 r2 9 Li Li = 3.71 fm = 2.44 fm Dobrovolsky et al, NPA766 (2006) 1 Strong absorption in elastic channel Large cross section for fragmentation They are easily polarizable. Reaction mechanisms and Nuclear effects of halo nuclei need to be understood Elastic scattering of halo nuclei near the Coulomb barrier 10,11Be+64Zn 10Be+64Zn 11Be+64Zn Di Pietro et al. Phys. Rev. Lett. 105,022701(2010) Catania, IEM-CSIC, Huleva, Sevilla Collaboration CDCC calculations Experimental elastic cross section. reproduced only taking into account coupling to continuum via the Coulomb and nuclear interactions 17 Scattering of 11,9Li on 208Pb around the Coulomb Barrier Elastic Scattering ECM = 23.1 MeV below Coulomb Barrier 9Li Competing process with Elastic Scattering for loosely bound systems Direct Breakup 11Li 2n-Transfer ECM = 28.3 MeV @ the Coulomb Barrier 9Li Scattering process dominated by: - Dipole couplings (coulomb + nuclear) - Coupling to continuum - Good description in a 4-body model 11Li Cubero et al, PRL109 (2012) 262701 IEM-CSIC, Huelva, Seville Collaboration 18 18 Why to study the N=Z 72Kr Nucleus? Nuclear structure: o Shape coexistence in the mass region was first proposed for 72Se [Ham74]. o 72Kr ground state is predicted to be oblate [Dic72] and [Naz85]. o First excited 0+ state in 72Kr found to be a shape isomer [Bou03]. o Possibility of study np-pairing effects as 72Kr belongs to N=Z line. [Ham74] J.H. Hamilton et al., Phys. Rev. Lett. 32, 239 (1974) [Dic72] F. Dickmann et al., Phys.Lett. 38B, 207 (1972) [Naz85] W. Nazarewicz et al., Nucl. Phys. A435, 397 (1985) [Bou03] E. Bouchez et al., Phys. Rev. Lett. 90, 082502 (2003) Nuclear astrophysics: o 72Kr rp-process in N=Z nuclei & A=70-80 region “waiting point" in rp process. 73Rb is unbound o β decay competes with 2p capture. 19 Coulomb excitation of 72Kr Use of submicron Y203 material for target => Yield increase x 10 Coulex Spectra - number of counts in 710 keV peak depends on the shape of 72Kr Oblate 72Kr expected Doppler Corrected for 104Pd target excitation The technique Doppler Corrected for 72Kr projectile excitation: 150 counts in 710 keV line 20 TAGS @ISOLDE: The case of 72Kr o Conversion electron studies to determine the multiplicities of the low gamma transitions o B(GT) obtained by measuring the intensity of the full gamma de-excitation cascade from each fed level to the ground state. P. Sarriguren, Phys. Rev. C 79, 044315 (2009) Briz, ISOLDE Workshop 2012 IEM-CSIC, Strasbourg, Surrey, Valencia The B(GT) 21 distribution favours oblate deformation! Searching for pear-shaped nuclei at ISOLDE Quadrupole deformation Coulomb excitation to directly access E3 transition strengths λ=2 Oblate (Earth) λ=2 Prolate (Rugby ball) B(E3) ≳ 30 s.p.u. gives significant β3 Octupole correlations enhanced at numbers: Z or N=34, 56, 88, and N= 134. Observed Z≈88 & N≈134 Microscopically driven... Intruder orbitals of opposite parity and ∆J, ∆L = 3 close to the Fermi level 22 L. P. Gaffney, et al. (2013). Nature, 497(7448), 199–204. doi:10.1038/nature12073 Hangout with CERN: Going pear-shaped (http://www.youtube.com/watch?v=x8Jdu9O2RhU&feature=emuploademail) MORE than 1000 viewers 23 Physics program @ REX REX-ISOLDE started in 2001 72 different beams already used at REX- ISOLDE of 700 available! 20 40 82 50 222,224Ra; 220,222Rn 184,186,188Hg Probing Pear Shape Nature 497 (2013)199 Probing shape coexistence 82 The Limitations of REX-ISOLDE (E 3.1 MeV/u) Evolution of collectivity Extension to higher energy is difficult Xe Se, shape coexistence, Hurst PRL 2007 around Sn 110Sn; Cederkäll, PRL 2007 Very limited energy flexibility 106,108Sn, Cederkäll, PRL 2008 Operation restricted to pulsed mode 50 122,124,126Cd Bunch length is not flexible 70 138,140,142,144 96Sr, 88Kr, 92Kr 28 132 140,148,150Ba 74,76,78,80Zn Probing large scale shell model, Van der Walle, PRL2007 67,69,71,73Cu, Stefanescu et al., PRL 2008 68,70Cu, isomeric 68Cu, Stefanescu , PRL 2007 30,31,32Mg, 20 Niedermaier PRL2005, H. Scheit d(30Mg,p)31Mg, K. Wimmer, PRL 2010 Halos & clusters d(8Li,p)9Li*; d(9Li,p)10Li… 24 Near Future: HIE-ISOLDE project • • • • Energy Upgrade: The HIE-ISOLDE project construction of the SC LINAC to upgrade the energy of the postaccelerated radioactive ion beams to 5.5 MeV/u in 2015 and 10 MeV/u by 2017 25 Approved Dec 2009 Offically started Jan 2010 Yacine Kadi project Leader Budget 40 M$ Intensity Upgrade: The design study for the intensity upgrade, also part of HIE-ISOLDE, started in 2011, and addresses the technical feasibility and cost estimate for operating the facility at 10 kW once LINAC4 and PS Booster are online. Physics addressed with HIE-ISOLDE / IS564 Study of the unbound proton-rich nucleus 21Al with resonance elastic and inelastic scattering using an active target (USC, IEM, MAYA Collaboration) 26 Experiment To measure resonant elastic, 20Mg(0+), and inelastic, 20Mg(2+), scattering using MAYA to determine energy, spin and parity of the 21Al excited states. 27 Summary and outlook The future of ISOLDE is bright. It will restart in June 2014 with the low energy program. With more than 40 year of operation ISOLDE remains as the pioneer ISOL-installation both at the level of designing new devices and production of frontier Physics. Post accelerated beams up to 5.5 MeV/u for the wide range of nuclei produced at ISOLDE will be available from Autumn 2015. HIE-ISOLDE will be the only next-generation radioactive beam facility (as identified by the NuPECC LRP) available in Europe in 2015, and the most advanced ISOL facility world-wide. Welcome to propose challenging experiments! Thanks for your attention ! 28