Collinear Laser Spectroscopy at ISAC

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Collinear Laser Spectroscopy at ISAC

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for 100mW of laser power and 50pA of isobar beam. 1.5 Hz.pA-1. 0.225 Hz.pA-1. 3.25 Hz.mW-1 ... Amongst the isobars, about 1pA is La. An estimate of the signal ... – PowerPoint PPT presentation

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Title: Collinear Laser Spectroscopy at ISAC


1
Collinear Laser Spectroscopy at ISAC
  • ISAC Seminar
  • May 2005
  • Thomas Cocolios
  • McGill University

2
Outline
  • Nucleus properties
  • Collinear Laser Spectroscopy
  • Interest in the Lanthanides
  • Experiment specifics

3
Hyperfine Structure
m
4
Isotope Shit
Isotope 1
Isotope 2
5
Collinear Laser Spectroscopy
Laser beam
Accelerated beam (several tens of keV)
6
Doppler Compression
For DE 3 eV n 18578.8 cm-1
7
Interest in Lanthanum
  • Models predict a change in deformation at
    low neutron number, observable with ltr2gt.
  • Study of Lanthanum has been limited to long
    lived isotopes so far.

8
Studied Transition
9
Observed Spectrum
Microwave OLIS Source providing up to 2nA at the
detection region At the biggest peak, the signal
goes up to 9000 600 8400Hz which gives
4.2Hz/pA Background 600Hz gt Noise
25Hz
10
Background
11
Prediction with RIB
  • Amongst the isobars, about 1pA is La. An estimate
    of the signal then is 4 Hz
  • Signal-to-noise is then 1-to-5 over one second
    and does not permit peak identification
  • Signal-to-noise increases as the square-root of
    the time gt it takes 10 times better
    signal-to-noise (2-to-1 ratio) for proper
    identification. For a scan of 500 channels, it
    then takes 500102 50000s 14 hours
  • TOO LONG !!

12
Improvements
  • Reducing Laser induced backgrounds by knife-edged
    apertures, widen apertures, blacken plates.
  • Laser Scattered Light ? Hz.mW-1 gt 33 Hz
  • Shielding the activity at the source to bring
    that share of the background to 0 Hz.

TOTAL background 64 Hz Noise 8 Hz Scan
8000s 2 hrs 15 min
TOTAL background 140 Hz Noise 12 Hz Scan
18000s 5 hrs
13
Conclusion
  • Unknown metastable population from surface source
    limits prediction
  • Long acquisition requires laser and energy
    stability
  • At least one last offline test before going for
    radioactive beam
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