I’m in the process of designing a new nuclear fusion research facility. I am currently working on radiation protection issues.
The device generates a neutron flux during operation.It is necessary to protect both personnel and electronics from the effects of these particles (both direct and indirect, which we’ll talk about later ).
I have more or less learned how to use this wonderful package for calculating neutron flux attenuation in walls with different channels (which is one of the optimization tasks). But there are also a couple of questions on this part.
- “Interface”. In version 0.10 after launching the code (openmc.run()), the console printed a logo and gradually printed the progress of execution (first, loading of various data then the number of the current banch). However, the situation in version 0.11 is very strange. It doesn’t print anything for a long time, but sometimes it prints everything up to some banch. For example, with 400 banachas, it prints after the 40th and 22*th.
Is it possible to set up a normal mode of printing progress?
This happens both on the virtual machine on Ubuntu and on the server node. The openmc package was installed on them independently by different people. - The question of random results.
The montecarlo method is based on a random distribution.
However, when I run the same task several times in the output file, the values are absolutely the same. They change only when particle parameters change (banchi*quantity in one banch). Either I don’t understand something in the physics of the process or I use the code incorrectly. Maybe you need to restart the random procedure or something like that?
In addition, there is a question about the appearance of a gamma photons, and their propagation / absorption in radiation shielding.
As far as I understand, at the moment there is no direct method of determining the photon flux/current through the tally.
I thought it would be an option to look at the neutron energy spectrum at different depths of the shielding wall and estimate the depth of the main photon generation. And then, according to the data available for their absorption, we can estimate the remaining flux and the resulting radiation load. But that is difficult and less accurate option .
Is there a more adequate way to assess the effect of gamma radiation at this point?
Or maybe it is possible to determine the gamma flow directly in the near future?
Sorry about a such long message)