Open fzeiser opened 5 years ago
So the effect is most visible for the lowest/highest energies. I guess we should implement a smoothing in Ex and Eg direction according to the detector resolution.
Here come the corresponding pictures from the master branch, ie. where z(Ex,Eg)=1
@jorgenem : This could also be a very natural way to include the population cross-section into the Oslo Method ;P
Issue: Need to take care of integer/half integer spins. For 240 Pu this was probably wrong now.
For curiosity I gave it a try to see what happens if I equally populate spins up to J=0.5
or J=4.5
(note the different scales!)
The effect of z
:
Jpop_max=0.5
Jpop_max=4.5
And the effect on the extracted gSF (keeping the same 1Gen matrix)
Jpop_max=0.5
Jpop_max=4.5
So the gSF get quite a different slope for higher gamma-ray energies (propagates from the nld)! This is consistent to what we have observed previously.
There is one thing to note. Now I generated the true 1Gen
matrix my populating all J
s proportionally to Jint
, however I analyze(fit the gSF) as if I had populated the only up to Jpop_max
(and these, equally). Therefore we see that the gSF from the fit get's a smaller slope for high Eg
's for Jpop_max=0.5
then for Jpop_max=4.5
and not the other way around (which we see in the experiment...)
@jorgenem and I wondered whether we need to include a sum depending on the population cross-section (or spin-parity distribution) and intrinsic spin-parity distribution in the fitting to the 1Gen matrix.
Created a test branch, where I implemented this in a hacky way: 30dfec9 This way we can see the effects, at least for one implementation.
Current assumption:
Results for this case:
Does not change very much but a bit, see next post with ideas!
A) Visualizing the sum and it's impact along the nld and Eg axis Note: Bug in the axis below: Should state
Eg
instead ofEx
B) Effect on the fitted matrix
C) Effect on the NLD and GSF
Ok, actually, you can't see the effect, as I didn't post the previous "picture" yet. But it basically just has an effect at low energies of the NLD and highest energies for gsf.