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Strangelet Search in Lunar Soil

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Exposure age to strangelet flux of moon is 500M years. ... dE Counter: 8.2um Si layer with front Au window (20nm) and rear Al window (150nm) ... – PowerPoint PPT presentation

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Title: Strangelet Search in Lunar Soil


1
Strangelet Search in Lunar Soil
  • Ke Han
  • Evan Finch
  • 12/15/2004

2
Strangelets 54O Density in Lunar Soil
  • Assuming
  • 1 event in 4.6 days in 0.167 m2 sterad for
    AMS-01.
  • AMS-01 can only count strangelet events with
    Betagt0.4.
  • Exposure age to strangelet flux of moon is 500M
    years.
  • Strangelet penetrating distance is 1m on average.
  • The ratio 54O/16O on the moon is 4.410-17
  • Jes Madsens theoretical calculation 2.310-17
    agrees with this number roughly.

3
Strangelets 54O Density in Lunar Soil
  • This ratio is 105 smaller than what we thought,
    because we neglected the solar modulation before.
  • When extending AMS-01 events with Betagt0.4, Jes
    Madsens new theory considering solar modulation
    gives only 10-40 gain for the range Betagt0. Our
    previous calculation gave a gain about 105.

4
Running Time
  • Assuming
  • 16O Beam Current in the Accelerator is 6uA.
  • The beam transmission efficiency through the
    accelerator is about 20.
  • For each magnet setting, the accelerator covers
    1/14 amu.
  • We can get
  • The 16O flux that will arrive at the detection
    system is 7.2 X 1012 ions / second.
  • For an hour run, we have 1.1 strangelets.
  • Running for 5 hours for each magnet setting to
    get about 5-6 strangelets.
  • Suppose strangelet isotopes other than 54O exist,
    we need only cover 2 amu thoroughly. Thats 140
    hours running time.
  • Or we would like to cover the whole Delta Range
    (548/-6), we need 980 hours.

5
Experiment Setup
  • Gold Foil Two different choices10um and 12um
  • dE Counter 8.2um Si layer with front Au window
    (20nm) and rear Al window (150nm)
  • E Counter Si layer should thicker than 18.1um so
    it can absorb all the energy.

6
Measurement Procedure
7
Measurement Procedure
8
Measurement Procedure
9
Measurement Procedure
10
Measurement Procedure
11
Background Beam Current
  • Considering about the source ratio in lunar soil,
    ion source sputtering efficiency, and charge 5
    stripping efficiency, we get the background beam
    current in the accelerator, assuming 16O
    current6uA.
  • The background beam current is useful for our
    calibration run.
  • They wont survive after the rigidity-selection
    magnets and Gold foil.

12
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13
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14
Background Ions in the E-dE Plot
15
Background Ions in the E-dE Plot
  • Two strangelets with 85 MeV (stripped charge 4)
    and 102 MeV (stripped charge 5) before the Gold
    foil.
  • Normal Oxygen with different incident energy fall
    near strangelets.
  • Oxygen accelerated from lunar soil will not have
    right rigidity to cross the magnets and then will
    not appear in E-dE plot.
  • The only concern about the background is the
    pick-up ions, that is, ions produced from the
    collision between the beam and gas in the
    accelerator.
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