experimental techniques
play

Experimental Techniques Nick Esker Postdoc, EMMA group - PowerPoint PPT Presentation

Experimental Techniques Nick Esker Postdoc, EMMA group neesker@triumf.ca Three sessions for all detection schemes.. My Goal: This is a very large area of active research, with ~100 years of history from Roentgen & the Curies to


  1. Experimental Techniques Nick Esker Postdoc, EMMA group neesker@triumf.ca

  2. Three sessions for all detection schemes….. • My Goal: This is a very large area of active research, with ~100 years of history from Roentgen & the Curies to present. I want you all to be able to tackle a modern experiment without getting too distracted / off- put by the “how” • Three sessions IS NOT ENOUGH!!!! I’m purposefully ignoring: • Accelerators, reactors • Relativistic effects • Electronics / DAQ • Statistics

  3. How this’ll work • We’ve a lot of material to cover. Too much. • I’m a strong believer in “active learning” • 40-50 min of lecturing (with plenty of questions ) • 10-15 min of small group activity, working on some toy problems • PLEASE ASK QUESTIONS!!!! • Resources: • Knoll: Nuclear Instrumentation • Krane: Nuclear Physics

  4. The Plan TM Day 1 – Nov 6 Day 2 – Nov 15 Day 3 – Nov 17 • Radiation interaction • Manipulating matter • Charge particles with matter counting w/ gas • E and B fields • α, β , γ , n 0 , SF decay • Geiger-Mueller • lasers • Scintillators • Prop. counters • Examples • Semiconductors • Organic • Recoil separators • Inorganic • Si detectors • Traps • Light detectors • HPGe detectors • Potpourri • Examples at TRIUMF • PMT, MCP • Active targets • Examples at TRIUMF • 0 νν detectors • HE calorimeters

  5. Ionizing radiation’s interaction with matter • Sources of ionizing radiation? • Accelerators and Reactors (& HE lasers) • Multiple secondary sources • Nuclear decay • α, β , γ , n 0 , SF decay

  6. Nuclear decay • α • β • γ • n 0 • SF

  7. Nuclear decay

  8. “Heavy” charged ions 10 MeV / u, Z beam = 6,7,8,10,18

  9. “Heavy”, charged ions • Bragg Curve • Energy ( E ), range in matter ( x ), and timing ( t ) are all affected by straggling, which widen their distributions

  10. Believing Bragg by Bethe-Bloch

  11. Beyond heavy… • e -

  12. Photons and matter

  13. Photons and matter • Three regimes

  14. n 0 interactions • Elastic collision with the nucleus • Capture cross section dependent • Look for secondary forms of radiation

  15. E deposited in matter • So, at this point, we’ve covered a couple general ways to deposit E of our ionizing radiation into some material. Once it’s there, how can we detect it?

  16. Scintillating • What makes a good scintillator?

  17. Scintillators • Organic • Inorganic

  18. Efficiency of scintillation

  19. Detecting Light - PMT

  20. Detecting Light - MCP

  21. Concluding remarks

  22. Active scintillators @ TRIUMF • DRAGON’s gas target

  23. Active scintillators @ TRIUMF • DESCANT neutron detectors

  24. Exercise 1. Calculate the scintillation efficiency of anthracene if a 1.5 MeV alpha particle is stopped in the medium, which created 20,300 photons with average wavelength of 447 nm 2. Starting from the full Bethe-Bloch, derive the non-relativistic Bethe-Bloch from the lecture 3. An ion chamber with parallel plate electrodes, spaced 5 cm apart, is filled with methane up to 1 atm and operated at 1 kV. Knowing the W -value of methane (27.3 eV/ ion pair), calculate the maximum e collection time. (Might need to look up mobility of ions in electric field, gas)

Download Presentation
Download Policy: The content available on the website is offered to you 'AS IS' for your personal information and use only. It cannot be commercialized, licensed, or distributed on other websites without prior consent from the author. To download a presentation, simply click this link. If you encounter any difficulties during the download process, it's possible that the publisher has removed the file from their server.

Recommend


More recommend