Question

The GRAMS project plans to launch a liquid argon time projection chamber into space to detect these particles in the MeV range, potentially from sources like neutron star mergers and blazars. For 10 points each:
[10h] Name these particles previously detected with Compton telescopes. In time projection chambers, the tracks left by these particles are distinguished by a gap between the interaction vertex and the electromagnetic shower.
ANSWER: gamma rays [prompt on photons by asking “what are they known as in the MeV energy scale?”]
[10m] The VERITAS array in Arizona can detect atmospheric gamma rays by their emission of this phenomenon. This phenomenon is responsible for the characteristic blue glow of a nuclear reactor core.
ANSWER: Cherenkov light [or Cherenkov radiation]
[10e] The Fermi Telescope in low Earth orbit can detect and characterize gamma-ray bursts by observing their pair production into electrons and these antiparticles.
ANSWER: positrons [or e-plus]
<BW, Physics>

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Summary

Data

MITTufts A0101020
YaleTufts B0101020
Bowdoin CBU0101020
AmherstBoston College A001010
Clark WilsonBoston College B0101020
Bowdoin ABowdoin B001010
Brandeis AClark House001010
Brandeis BHarvard0101020