1 / 10

SuperCHICO; a 4 π heavy-ion detector

SuperCHICO; a 4 π heavy-ion detector. C.Y. Wu and D. Cline An arsenal of auxiliary charged-particle detectors must be an integral component of GRETA in order to achieve and exploit the ultimate in sensitivity and selectivity for nuclear science

jonny
Download Presentation

SuperCHICO; a 4 π heavy-ion detector

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. SuperCHICO; a 4π heavy-ion detector • C.Y. Wu and D. Cline • An arsenal of auxiliary charged-particle detectors must be an integral component of GRETA in order to achieve and exploit the ultimate in sensitivity and selectivity for nuclear science • The 4π heavy-ion detector, SuperCHICO, is designed to exploit γ-ray tracking arrays for study of quasi-binary reactions at both stable and exotic beam facilities, that is: • Coulomb excitation • Single and multi-nucleon transfer reactions • Deep inelastic reactions • Fission • SuperCHICO is based on the successful CHICO detector.

  2. CHICO Ge detector CHICO* M.W.Simon, D. Cline, C.Y. Wu R.W. Gray, R. Teng. C. Long Nucl. Inst. Meth. A452 (2000) 205 *Work supported by the NSF Scattering angle: 12 85 (Front Part) 95 168 (Back Part) Azimuthal angle total: 280 of 360 Position resolution:  1 in  and 9.3 in  Solid angle: 69% of 4π Time resolution:  500 ps Mass resolution Δm/m = 5% Q-value resolution: ≤ 20 MeV

  3. Doppler-corrected γ-ray spectra 1358 MeV 238U on 170Er C.Y. Wu, D. Cline, et al, Phys. Rev. C61 (2000) 21305(R) CHICO/Gammasphere Raw data Correction for U-like recoils Correction for Er-like recoils

  4. CHICO-GS Operation 1996-2006 • CHICO-Gammasphere ideal for quasi-binary type reactions: Coulomb excitation transfer reactions deep-inelastic reactions fusion-fission reactions • 24 experiments performed by 58 researchers from 17 institutions • 48 publications, including 2 Phys. Rev. Lett. and 2 in Phys. Lett. • 5 Ph.D. theses completed

  5. SuperCHICO performance • Angular coverage: 20o ≤ θ ≤ 85o, 95o ≤ θ ≤ 160o; 280o in φ • Angular resolution:Δθ = 1o, Δφ = 1.4o • Solid angle: 66% of 4π • Time resolution:Δt = 500ps • Mass resolution for kinematic coincidence:Δm/m = 5% • Q-value resolution: ≤ 20 MeV • GRETA Doppler-corrected γ-ray resolution: ~ 0.3%

  6. Advantages of SuperCHICO • Large solid angle: Study weak exotic beams or low cross-section processes • Large angular coverage:High kinematic coincidence efficiency Large range of impact parameters • Angular and time resolution:Mass, Q-value resolution; high selectivity • Achieve maximum Doppler-corrected γ-ray resolution for GRETA: • Identify γ-rays from each fragment • Very high count-rate capability:> 100kHz • Hardness to radiation damage: • High background suppression:PPAC blind to light ions, Kinematic coincidence requirement • Minimal mass:Minimal γ-ray absorption and Compton scattering • Low initial and operational costs:only 80 channels of electronics for 26,000 pixels

  7. Cost details: LLNL estimate • Assume most engineering carried out at LLNL • Mechanical • Design: 22 weeks, $100k • Fabrication: $100k • Electronics • Amplifier • Replace CHICO hybrid circuit design • Design: 6-8 weeks, $80k • Fabrication: $80k • Downstream • Recycled from CHICO • Replaced by FADC and computer-controlled gas-handling system at some future date • Total cost: $360k excluding scientific manpower at LLNL and Rochester. St. Louis Workshop

  8. Future Opportunities • SuperCHICO plus GRETA will be a powerful facility for nuclear spectroscopy using either stable or exotic beams • Stable beams: a) Probe quadrupole, octupole, or pairing collective modes of motion in nuclei. b) Extend studies of transuranic nuclei to higher spin, ≥40ħ c)Probe collective bands built on unusual isomeric states and determine the Eλand Mλ matrix elements involved to probe both collective and shell structure. • Exotic neutron-rich beams: a) Explore the evolution of collectivity and shell structure with isospin. b) Deep inelastic and transfer reactions will extend range of neutron-rich nuclei. c) Pair transfer to probe neutron pairing correlations in neutron-rich nuclei d) Exploit isomeric beams to probe unusual configurations in nuclear structure

More Related