beta delayed neutron covariances tim johnson, libby mccutchan, alejandro sonzogni national nuclear...
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Beta Delayed Neutron Covariances
Tim Johnson, Libby McCutchan, Alejandro Sonzogni
National Nuclear Data Center
Beta Delayed Neutron CRP #2 - Alejandro Sonzogni
Many bn emitters have high fission yield values, in particular Br (Z=35), Rb (Z=37), I (Z=53) and Cs (Z=55)
Chart colored by 235U fission yields, highlighted by Qbn>0
Beta Delayed Neutron CRP #3 - Alejandro Sonzogni
Link between basic and more macroscopic quantities used in applied nuclear physics
nd: Delayed nu-bar, number of neutrons for single fission event. It can be calculated as:
nd =S CFYi Pni , about 0.015/fission for 235U
CFY: cumulative fission yield.
Pn: beta-delayed neutron probability.
Pn and T1/2 values of beta-delayed neutron emitters are relevant in nuclear power and astrophysics.
Beta Delayed Neutron CRP #4 - Alejandro Sonzogni
Following Loaiza et al. & Than Dat et al., the recommended delayed nubars (MF=1, MT455) are plotted for a number of systems.
Beta Delayed Neutron CRP #5 - Alejandro Sonzogni
Same plot as before, for summation calculations using JEFF-3.1 yields and ENDF/B-VII.1 decay data
232Th 238U 235U 241Pu238Np
233U 239Pu
252Cf
Beta Delayed Neutron CRP #6 - Alejandro Sonzogni
232Th 238U
As before, but plotting lighter and heavier fission fragments contributions
Beta Delayed Neutron CRP #8 - Alejandro Sonzogni
Disagreements in fission yields for 237Np
ENDDF/B yields are larger than JEFF’s for neutron rich nuclide
Beta Delayed Neutron CRP #12 - Alejandro Sonzogni
Delayed neutron activity Covariances
Ad(t): Delayed neutron activity following the decay of an equilibrated system
To obtain Ad(t), we solve the Bateman’s equations:dNi(t)/dt=-liNi +S lki Nk , with boundary conditions:dNi(0)/dt=0, that is, Ni(0)~CFYi/li , then:
Ad(t)= S li Pni Ni(t)
We use a Monte Carlo method, the only correlation in fission yields is that they are normalized to 2, and the branching ratios are normalized to 1.
Beta Delayed Neutron CRP #13 - Alejandro Sonzogni
Delayed neutron activity Covariances
For N histories, we obtain Adi(tk), so the average value would be:
<Ad(tk)>= N-1 S Adi(tk)
The uncertainty as:
D2Ad(tk)= <Ad(tk) Ad(tk)> - <Ad(tk)><Ad(tk)>
And the covariance matrix:
s(Ad(tk), Ad(tj) )=skj=<Ad(tk) Ad(tj)> - <Ad(tk)><Ad(tj)>
Covariances are obtained by a Monte Carlo method
Beta Delayed Neutron CRP #16 - Alejandro Sonzogni
Delayed neutron activity divided by Keepin’s values
Beta Delayed Neutron CRP #18 - Alejandro Sonzogni
Six group parameters fit
In the ENDF-6 libraries, the delayed neutron activity is given as a sum of 6 or 8 exponential terms:
Ad(t)= S ai exp(-li t)
In order to properly propagate uncertainties, we not only need the uncertainties in ai and li, but also the correlations:
< ai ak >, < ai lk >, < li lk>
For each history, we fit Ad(t) with a Keepin-like function, using Keepin’s parameter as a starting point.
Beta Delayed Neutron CRP #20 - Alejandro Sonzogni
Six-group fit
The ak have uncertainties in the 10-17%, while the lk in 2-10%, due to a more uncertain fission yield data
Beta Delayed Neutron CRP #22 - Alejandro Sonzogni
6-group Parameters Correlation Matrix
a2 & a4 anticorrelation
l4 & l5 correlation
Beta Delayed Neutron CRP #23 - Alejandro Sonzogni
Conclusions
Delayed nu-bars and neutron activities have been very precisely measured. In summation calculations decay data is of good quality, but there are problems in the fission yields data.
Our work test the relatively short-lived (T1/2 < 100 s) subset of fission yields. We look forward to the next generation experiments and the results of the current WPEC Subgroup.
We will generate covariance matrices for all targets of interest.
Beta Delayed Neutron CRP #24 - Alejandro Sonzogni
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