First off, I want to thank you for how quickly you are responding to my thread. I'll quote your response with my reasonings below:
Alex A said:
I also suspect the quantity of source material may be wrong, but this is a small thing.
While I was running a significantly shorter version of this problem (2000 nps) to check my inputs, I was printing all of the tables for my output file. One of the tables calculated the activity of the source cell. I kept adjusting the volume of the source cell until the output table showed an activity as close to 20 TBq as I was able to get. I think I ended at 19.x TBq.
Alex A said:
You are also doing a lot of photon simulation when your source and daughter are beta emitters.
I am aware that the isotopes are primarily beta emitters, but we are more concerned with the shielding of the gammas that are also produced (I work for a rad safety consultant company).
Alex A said:
And you have a forced collision card!
This was out of a little desperation and taken from a slightly similar problem I found online. It can be easily removed.
Alex A said:
PAR=SD I've never used. MCNP is usually verbose and unclever. This is really enlightened. I don't trust it at all. I think you are using it incorrectly but I can't be certain.
I picked par=sd because of this particular part of the MCNP manual which is in the list of added features for 6.2:
"The spontaneous-decay source option was extended to provide an all-particle decay option
(PAR=sd on the SDEF card) [8], which automatically generates the correct number of all types of
source decay particles if those particle types are included on the MODE card. Previously, a user
had to specify a distribution of such particle types and adjust the source normalization accordingly."
If I am reading this correctly, and I'm not sure I am, it reads as though MCNP will generate both the beta and gamma particles that come from the decay of Yb-177.
There is also this section: "The PAR=SD, SN, SP, SB, ST, SA, and ZZZAAA (with ERG=0) options require
time integration of daughter production at each level within a decay chain. This is facilitated by
setting all decay constants to unity and uniformly spacing all time bins within 20 s (or ~20 decay
levels), which will include all decay particle production within most decay chains (i.e., an
equilibrium production)."
Unfortunately, I don't know if I need to specify the time integration for the daughters, or if MCNP handles that with "setting all decay constants to unity...."
Alex A said:
You are using a ball of flesh (!) to calculate absorbed dose which should give the right answer but the same full cell to work out flux to convert to rem/hr and I think you should be using an empty cell for this.
This was again taken from the same similar problem I mentioned above. It is a masters thesis in which they are determining dose from a neutron source, which although I'm using a primarily beta emitter, does coincide to finding absorbed dose. My F4:P tally I haven't been using the data from because I don't fully understand flux anyways, so if that is not needed it can be dropped as I am only interested in the absorbed dose taken from the F6:P tally.
Thank you again for your help so far. It has been much easier to parse than the MCNP manual and the Primers I have found online.