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Imaging Nuclear Reactions

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Washington University team had detectors with 32 strips in each direction. ... This allows extra electron and hole energy levels which will increase the ... – PowerPoint PPT presentation

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Title: Imaging Nuclear Reactions


1
Imaging Nuclear Reactions
  • Zhon Butcher
  • 2006 REU Program
  • Cyclotron Institute
  • Mentor Dr. Robert Tribble

2
Applications of Nuclear Imaging
  • Space Telescopes Cosmic radiation
    identification and direction of origin.
  • Imaging reactions in the nuclear physics
    laboratory.

3
How Imaging Works in the Lab
  • Several detectors are placed around the reaction
    site covering a given solid angle.
  • Detectors determine particle identity and
    position.
  • The resulting image gives a picture of the
    reactions that took place in the chamber.

4
Particle Identification
  • Telescopes Front detector and rear detector.
  • Front detector picks up energy loss as the
    particle passes through.
  • Rear detector picks up residual energy.
  • Particle identification determined by

5
Methods for Position Determination
  • Many small detectors coupled with a large amount
    of electronics (clustering).
  • Resistive strip detectors.
  • Double sided strip detectors.
  • Resistive sheets.

6
1-D Position Sensitive Detector
7
Resistive Strip Detectors
  • Consist of many resistive strips placed alongside
    one another.
  • Good resolution in the X direction, poor
    resolution in the Y direction (or vice versa
    depending on orientation).

8
PSSDs
9
Double Sided Strip Detectors
  • Two sheets of strips placed one in front of the
    other so the strips form a grid.
  • Results in better position resolution
  • Washington University team had detectors with 32
    strips in each direction.
  • 64 strips per detector x 4 detectors 256
    channels for position reconstruction

10
Double sided PSSDs
11
Resistive Sheets
  • A single resistive sheet spans the entire active
    area of the detector.
  • Advantages
  • Fewer signals to process.
  • Less electronic equipment.
  • Detector Types
  • Duo-lateral Generates two signals from each face
    of the detector, two from the front and two from
    the back.
  • Tetra-lateral Generates five signals, one from
    each corner of the resistive side, and one signal
    from the back.

12
Tetra Lateral Detectors
Particle impinging position calculated by
13
Signal Processing
ADC
Preamplifier
Spectroscopy Amplifier
Preamplifier
Spectroscopy Amplifier
Detector
Computer
Preamplifier
Spectroscopy Amplifier
Preamplifier
Spectroscopy Amplifier
Gate Generator
Discriminator
Preamplifier
Timing Amplifier
Rear signal
14
How Silicon Detectors Work
15
Current Through Semiconductor
16
Doped Semiconductor
  • What is doping?
  • Doping is the integration of impurities into the
    lattice structure of the semiconductor.
  • This allows extra electron and hole energy levels
    which will increase the conductivity of the
    semiconductor.

17
Experiment
  • To characterize the Micron Semiconductors
    tetra-lateral detectors in terms of energy and
    position resolution as well as non-linearity in
    position reconstruction.
  • Three tetra-lateral type PSDs were investigated.
    One 200 mm and one 400 mm thick detectors with a
    resistive strip around the active area, and one
    200 mm without a resistive strip.
  • Optimal strip resistance is approx. 1/10th the
    resistance of the detector active area.

18
Setup
  • The detectors were placed in a vacuum chamber
    with a radioactive source. (241Am and 228Th were
    used)
  • The distance between the source and the detector
    was approx 25cm for 241Am and 10cm for 228Th

19
Calibration Masks
  • Two masks were used to cover the detectors.

20
Position Reconstruction 200mm
Position reconstruction of impinging alpha
particles for the 200 mm thick detector with and
without a resistive strip.
21
Position Reconstruction 400 mm
Position reconstruction of impinging alpha
particles with and without a mask for the 400 mm
thick detector with a resistive strip.
22
Energy Resolution
  • Energy Spectrum of alpha decay from 228Th with
    400mm detector

Energy Resolution Approx 10
23
Results
  • The position resolution was determined to be
    around 3-4 mm and energy resolution of 8 for
    both the 400 mm and 200 mm thick detectors with
    the resistive strip.
  • The resistive strip has a major contribution in
    reducing the position reconstruction distortion.

For more information see T.Doke et.al. NIM A261
(1987) 605
24
Conclusion
  • The position resolution for the tetra-lateral
    PSDs strongly depends on the resistivity of the
    resistive sheet, electrode termination resistors,
    the filter components of the preamplifiers, and
    the shaping times of the amplifiers.
  • The measurements done were employing the use of
    Indiana University preamplifiers and CAEN
    amplifiers (3 ms shaping time). Further
    investigation of these dependencies is ongoing.

25
Acknowledgements
  • Special thanks to
  • Dr. Robert Tribble
  • Dr. Livius Trache
  • Dr. Adriana Banu
  • Matthew McCleskey
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