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I don't understand about variance reduction technique. Some one explain PHYS:N, PHYS:P and cutoff. when do I use them?
Thank you!
Thank you!
The discussion revolves around variance reduction techniques in MCNP (Monte Carlo N-Particle Transport Code), specifically focusing on the PHYS:N, PHYS:P, and cutoff parameters. Participants seek clarification on when and how to use these techniques, as well as specific card specifications for a point isotropic source in a cone of directions.
Participants do not appear to reach a consensus on the use of variance reduction techniques, as there are multiple requests for clarification and additional information. The discussion remains unresolved regarding the specific applications and implications of the techniques mentioned.
Some limitations include potential missing assumptions about the specific MCNP version being used and the context in which the variance reduction techniques are applied. There may also be unresolved mathematical steps related to the card specifications.
Here is an appendix to a thesis with some discussion of PHYS:Pneohohoho said:I don't understand about variance reduction technique. Some one explain PHYS:N, PHYS:P and cutoff. when do I use them?
Thank you!
The energy physics cutoff card defines the simple or detailed physics treatment in photon interaction. It has a form,
PHYS:P EMCPF IDES NOCOH
where EMCPF is upper energy limit (in MeV) for detailed photon physics treatment, IDES determines whether photons will produce electrons in MODE E problems or bremsstrahlung photons with the thick target bremsstrahlung model, and NOCOH controls whether coherent scattering occurs or not. For example, PHYS:P 0.2 0 0, tells that Photons with energy greater than 200 keV will be tracked using the simple physics treatment, photons will produce electrons in MODE E problems or bremsstrahlung photons with the thick target bremsstrahlung model, and coherent scattering is considered.
The history cutoff (NPS) card is one type of problem cutoff card used in the simulation. It terminates the Monte Carlo calculations after N histories have been computed.