Gamma electron coupled simulation

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SUMMARY

The discussion focuses on simulating gamma-ray interactions using MCNP6, specifically with gamma rays of 10 MeV incident on an aluminum disk to produce an electron spectrum that subsequently generates Cerenkov radiation in a CO2 gas cell. The user seeks clarification on whether to use the electron spectrum as an input source for further simulation or if mode p e is sufficient for observing Cerenkov light. It is confirmed that to observe Cerenkov radiation, a PHYS:e card must be activated, and specific parameters must be set, particularly for version 6.3 of MCNP6, which may vary in other versions.

PREREQUISITES
  • Understanding of MCNP6 simulation software
  • Knowledge of Cerenkov radiation principles
  • Familiarity with gamma-ray interactions and electron production
  • Awareness of the differences between MCNP6 versions
NEXT STEPS
  • Review the MCNP6 manual for version 6.3 regarding the PHYS:e card settings
  • Research the principles of Cerenkov radiation and its dependence on refractive index
  • Explore the effects of gas pressure on Cerenkov radiation production
  • Investigate the differences in simulation parameters across various MCNP6 versions
USEFUL FOR

Researchers and physicists involved in radiation physics, particularly those simulating gamma-ray interactions and Cerenkov radiation using MCNP6 software.

Salman Khan
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I am interested to simulate a problem in mcnp6, in which gamma rays (energy let say 10 Mev) incident on a aluminum disk and produce electron spectrum which further move in a gas (e.g co2)cell to produce chernkove radiation. Here gamma produce electron and electron further produce chernekov, in order to see chernkove photon mode p e only works?, or if I will get electron spectrum I will take it as input source and re simulate it to see chernkove light? Please guide thanks in advance
 
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Hi Salman,

The gas part confuses me a bit. To get Cerenkov (I also thought his name was spelled with an h) radiation the charged particle must travel faster than light through the medium. A trick, for those that don't know, that is possible because the speed of light through a transparent object is c/n where n is the refractive index. Unless the gas is under high pressure, the energy and implied refractive index seem a bit low.

Reading the manual, because I'm not familiar with the versions that transport visible light, mode p e should work but you need a PHYS:e card to turn on Cerenkov. Something like
Code:
PHYS : e 100 0 0 0 0 1 1 1 1 0 0 0 J 0.917 0.001 0.01
to use low numbers of Cerenkov photons with higher weight as recommended. This is for version 6.3 of the code and you should check the right manual for your version of the code, this command typically changes between versions.

Good luck and please let us know how well this works!
 
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Likes Astronuc and Salman Khan
Thanks Alex
 

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