Where are the Beta Particles in a Muon Detector?

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Discussion Overview

The discussion revolves around the detection of beta particles in a muon detector setup, specifically focusing on the challenges faced when attempting to calibrate the detector using a strontium-90 source. Participants explore the interaction of beta particles with scintillator materials and the comparison of detection signals from muons and beta particles.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant describes their setup with PMTs and scintillators and notes the lack of signal from strontium-90 despite detecting muons.
  • Another participant suggests that the beta particles, with a maximum energy of 0.5 MeV, may not deposit enough energy to be detected compared to the higher energy cosmic rays.
  • A third participant mentions the use of a multichannel analyzer and a single channel analyzer, indicating that while muons are detected, no signals from beta particles are observed, despite having background activity from the strontium source.
  • Concerns are raised about the coupling of the scintillator to the phototubes and the potential for light loss, which could affect detection of beta particles.
  • Participants discuss adjusting the gain settings on the PMTs to potentially improve detection of the beta signal.

Areas of Agreement / Disagreement

Participants express varying hypotheses about the detection of beta particles, with no consensus on the exact cause of the lack of signal. Multiple competing views on the effectiveness of the setup and the behavior of beta particles versus muons remain unresolved.

Contextual Notes

Participants mention the need to consider stopping powers and background radiation, but there are unresolved aspects regarding the calibration process and the specific configurations of the detector components.

Who May Find This Useful

Individuals interested in particle detection, scintillator technology, and experimental setups in nuclear physics may find this discussion relevant.

Getterdog
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This may be a pretty basic question ,but i'll through it out any way. As a project i built a muon detector from 2 matched PMTs and 2 4x6x1 plastic PVT scintillators. And pulse processing NIM modules. I was getting pretty good coincidence reading,some what less than predicted.ie ( 1 count/sqcm/min) However ,when I wanted to calibrate by using a small sample on strontium 90 (.5Mev beta ) i get no signal anywhere. I made sure there was no obstruction between it and the scintillator. Now from what i understand the average muon
energy at Earth surface is around 2Gev. I am assuming the beta fully is stopped by the scintillator. I am not sure the bethe bloch formula is valid for the speed of the beta, So where should i be looking for this signal?
Should the gain be turned way down to see the beta? I am trying to get an idea of where the strontium signal is compared to the muons. Thanks j
 
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Hmm, it's interesting. At 0.5 MeV of kinetic energy the electron will stop within the material. Remember that 0.5 MeV is the maximum kinetic energy for the electron, but the energy spectrum is continuous and the most probable energy is less.

If you have a cosmic ray background with an average energy of 2-3 GeV, the beta signal can be very low in comparison; or not, I don't know what fraction of its energy will deposit the cosmic ray inside your detector, maybe you should compute the stopping powers for both and compare (will the cosmic ray lose more than 0.5 MeV?). Anyway, don't forget to put the high voltage of the PMT in the region of the plateau.

Then, you can measure the background due to environmental radiation (including cosmic rays) to characterize it; next, place the source near the detector and start measuring. You must remove the background to extract the signal from the beta.

To get good statistics, you must take measures for a long time both to measure the background and the signal.
 
Thanks. Well ,on my multichannel analyzer,I saw no spikes,but I do register the muons. Also I used a single channel analyzer with a discriminator,to weed out the dark counts and saw nothing over that level. My Geiger counter shows I’ve got plenty of activity from the strontium, way over the dark count rate from the tubes. I adjusted the gains on both tubes so that they both drop off the dark counts at the same voltage on my amplifier chain. From what I can gather,the velocity of the beta is an order of magnitude lower than the muons. Next I’ll try dropping below the nominal voltage of the tubes to see if it shows up. Any other ideas? Thanks
 
Hard to say without actually looking at your equipment, but here's a few possibilities. How is the scintillator coupled to the phototubes? You have scintillator that is 4x6x1. How do you match it to the shape of the phototube so that you are collecting all of the light? Is the scintillator well polished and everything very light tight? Your betas could be under the background.
 

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