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Advanced Implantation Detector Array (AIDA):

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on behalf of the DESPEC-DSSD/AIDA collaboration. Tom Davinson. School of Physics ... Digital data via fibre-optic cable to PC-based data concentrator/event builder ... – PowerPoint PPT presentation

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Title: Advanced Implantation Detector Array (AIDA):


1
Advanced Implantation Detector Array
(AIDA) Update Issues
presented by Tom Davinson on behalf of the
DESPEC-DSSD/AIDA collaboration
Tom Davinson School of Physics The University of
Edinburgh
2
DESPEC Implantation DSSD Concept
  • Super FRS Low Energy Branch (LEB)
  • Exotic nuclei energies 50-150MeV/u
  • Implanted into multi-plane, highly segmented
    DSSD array
  • Implant - decay correlations
  • Multi-GeV DSSD implantation events
  • Observe subsequent p, 2p, a, b, g, bp, bn
    decays
  • Measure half lives, branching ratios, decay
    energies

3
Implantation DSSD Configurations
  • Two configurations proposed
  • 8cm x 24cm
  • cocktail mode
  • many isotopes measured simultaneously
  • b) 8cm x 8cm
  • high efficiency mode
  • concentrate on particular isotope(s)

4
DSSD Segmentation
  • We need to implant at high rates and to observe
    implant decay correlations
  • for decays with long half lives.
  • DSSD segmentation ensures average time between
    implants for given x,y
  • quasi-pixel gtgt decay half life to be observed.
  • Implantation profile
  • sx sy 2cm
  • sz 1mm
  • Implantation rate (8cm x 24cm) 10kHz, kHz per
    isotope (say)
  • Longest half life to be observed seconds
  • Implies quasi-pixel dimensions 0.5mm x 0.5mm
  • Segmentation also has instrumentation performance
    benefits

5
DSSD
  • Technology well established
  • (e.g. GLAST LAT tracker)
  • 6 wafer technology
  • 10cm x 10cm area
  • 1mm wafer thickness
  • Integrated components
  • a.c. coupling
  • polysilicon bias resistors
  • important for ASICs
  • Series strip bonding

8.95 cm square Hamamatsu-Photonics SSD before
cutting from the 6-inch wafer. The thickness is
400 microns, and the strip pitch is 228 microns.
6
AIDA DSSD Array Design
Implantation depth? Stopping power? Ge b
detector? Calibration? Radiation damage? Cooling?
courtesy B.Rubio
  • 8cm x 8cm DSSDs
  • common wafer design for 8cm x 24cm and 8cm x 8cm
    configurations
  • 8cm x 24cm
  • 3 adjacent wafers horizontal strips series
    bonded
  • 128 pn junction strips, 128 nn ohmic strips
    per wafer
  • strip pitch 625mm
  • wafer thickness 1mm
  • DE, Veto and 6 intermediate planes
  • 4096 channels (8cm x 24cm)
  • overall package sizes (silicon, PCB, connectors,
    enclosure )
  • 10cm x 26cm x 4cm or 10cm x 10cm x 4cm

7
AIDA Instrumentation Requirements
  • Large number of channels required, limited
    available space and cost mandate
  • use of Application Specific Integrated Circuit
    (ASIC) technology.
  • Requirements
  • Selectable gain low 20GeV FSR (use
    reset)

  • intermediate 1GeV FSR

  • high 20MeV FSR
  • Noise s 5keV rms.
  • Selectable threshold minimum 25keV _at_ high
    gain ( assume 5s )
  • Integral and differential non-linearity
  • Autonomous overload recovery ms
  • Signal processing time lt10ms (decay-decay
    correlations)
  • Receive timestamp data
  • Timing trigger for coincidences with other
    detector systems
  • DSSD segmentation reduces input loading of
    preamplifier and enables

8
AIDA ASIC Concept
  • Example design concept
  • 1 channel of 16 channel ASIC (shown with
    external FPGA and ADC)
  • - FEE-integrated DAQ
  • - Digital data via fibre-optic cable to PC-based
    data concentrator/event builder

courtesy I.Lazarus, CCLRC DL
9
AIDA General Arrangement
10
DSSD/Kapton Package
11
AIDA 128 channel FEE Card Concept
16 ch ASIC (with ADC?)
128 detector signals in 1 data fibre out
Power Supplies and other components
Virtex 4FX FPGA
Fibre Driver (Laser) for Ethernet
Ethernet MAC
Estimated size 80x220mm, Estimated power 25W
per 128ch (800W total)
courtesy I.Lazarus, CCLRC DL
12
NUSTAR Common DAQ Interfaces
Data output stage standard format and output
medium e.g. 10G Ethernet fibre Correlate by
timestamp
Clock and Timestamp BUTIS Common Clocks 10/200MH
z lt100ps/km
Slow Control Common database loaded
into local controllers over Ethernet
Front End Electronics
Detector
Detector HV etc.
courtesy I.Lazarus, CCLRC DL
13
AIDA System Concept
BUTIS Timestamps
PC Farm
Data Output
Switch
Slow Control
courtesy I.Lazarus, CCLRC DL
14
AIDA Current Status
  • Edinburgh Liverpool CCLRC DL CCLRC RAL
    collaboration
  • - 4 year grant period
  • - DSSD design, prototype and production
  • - ASIC design, prototype and production
  • - Integrated Front End FEE PCB development and
    production
  • - Systems integration
  • - Software development
  • Deliverable fully operational DSSD array to
    DESPEC
  • Proposal approved EPSRC Physics Prioritisation
    panel meeting April 2006
  • EPSRC award announcement letters received June
    2006
  • Detailed specification development has commenced
  • M0 specification finalised and critical review

15
Resources
  • Cost
  • Total value of fEC proposal c. 2.3M (incl. PG
    c. 2.6M)
  • Support Manpower
  • CCLRC DL c. 4.2 SY FEE PCB Design
  • DAQ h/w s/w
  • CCLRC RAL c. 3.5 SY ASIC Design simulation
  • ASIC Production
  • Edinburgh/Liverpool c. 4.5 SY DSSD Design
    production
  • FEE PCB production
  • Mechanical housing/support
  • Platform grant support CCLRC DL/Edinburgh/Liverp
    ool

16
AIDA Workplan
17
AIDA Project Partners
  • The University of Edinburgh (lead RO)
  • Phil Woods et al.
  • The University of Liverpool
  • Rob Page et al.
  • CCLRC DL RAL
  • John Simpson et al.
  • Project Manager Tom Davinson
  • Further information http//www.ph.ed.ac.uk/td/AI
    DA

18
Outstanding Issues
  • Threshold
  • How low is low enough?
  • Package size
  • 10cm x 26cm x 4cm (10cm x 10cm x 4cm)
  • Range of implantation energies and species
  • 50-150MeV/u ?
  • Corresponding ranges in Si
  • U 0.6 - 3.0mm
  • Sn 0.8 - 4.5mm
  • Ni 1.0 6.5mm
  • Energy and time resolution (decay)
  • lt 10keV FWHM
  • lt 10ns FWHM
  • Energy and time resolution (implant)
  • 1 ?
  • ?
  • External trigger (to gamma/neutron/whatever
    arrays)
  • prompt? delayed? time resolution?

19
Acknowledgements
Presentation includes material from other
people. Thanks to Ian Lazarus (CCLRC DL) Haik
Simon (GSI) Berta Rubio (IFIC, CSIC University of
Valencia)
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