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Gamma Ray Spectroscopy
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Gamma rays are MeV photons. They are typically emitted in the electronic transitions radioactive nuclei, and carry information on nuclear binding and energy levels. They are recently of increased astrophysical interest, as "gamma-ray bursters" seem to be telling us something about the mechanics of stellar collapse. In this experiment, you will establish the function of a NaI crystal + photomultiplier system to detect gamma-rays, and use the system to study some interesting nuceli. Co-60, used for medical radiation treatment, is a standard gamma ray reference source. Na-22 undergoes beta decay to positrons, and you can see the gammas rays that result when they annihilate with electrons. The gamma ray energy spectra also contain information about how gamma rays interact with matter. |
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Detection and measurement of gamma rays
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NaI crystal photomultiplier, NIM electronics, computer controlled ADC and histogramming with the Amptek "Pocket MCA"
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Interactions of photons with matter: Compton effect, photoelectric effect
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Mass of the electron via photon energy when electron annihilates with positron
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- Required reading:
- R. Eisberg and R. Resnick, Quantum Physics of Atoms, Molecules, Solids, Nuclei, and Particles, Chapter X.
- A. Melissinos and J. Napolitano, Experiments in Modern Physics, 2nd Ed. 8.1-8.2.5 and 8.4.
- "Gamma Ray Spectroscopy", 441-442 Write-up and Guidelines.
- Recommended reading:
- G. Gilmore and J. Hemingway, Practical Gamma-ray Spectrometry (A great book just crammed with useful information.)
- W.R.Leo, Techniques for Nuclear and Particle Physics Experiments
- G.F.Knoll, Radiation Detection and Measurement, Chapter
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SWIFT and GLAST: new satellites to observe gamma ray bursts
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ROTSE is worldwide network to see optical follow-up to gamma-ray burst. Invented and based at Michigan.
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