The Echo Method for Axion Dark Matter Detection

The Echo Method for Axion Dark Matter Detection

Galileo Galilei Institute via YouTube Direct link

Large velocity dispersion

11 of 15

11 of 15

Large velocity dispersion

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Classroom Contents

The Echo Method for Axion Dark Matter Detection

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  1. 1 Intro
  2. 2 The echo idea
  3. 3 Decay rate
  4. 4 Stimulated decay as Bose-enhancement
  5. 5 Enhancement factor
  6. 6 What does the echo wave look like?
  7. 7 Properties of echo wave
  8. 8 Echo power at ground level
  9. 9 A model for the beam
  10. 10 Small velocity dispersion
  11. 11 Large velocity dispersion
  12. 12 Collected power
  13. 13 Sensitivity
  14. 14 Beam height
  15. 15 Two type of Antennas

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