M Class_Work/nuce2101/final/latex/main.aux M Class_Work/nuce2101/final/latex/main.fdb_latexmk M Class_Work/nuce2101/final/latex/main.fls M Class_Work/nuce2101/final/latex/main.log M Class_Work/nuce2101/final/latex/main.pdf M Class_Work/nuce2101/final/latex/main.synctex.gz M Class_Work/nuce2101/final/latex/problem1.tex M Class_Work/nuce2101/final/latex/problem2.tex
80 lines
2.6 KiB
TeX
80 lines
2.6 KiB
TeX
\section*{Problem 1}
|
|
|
|
\subsection*{Part A}
|
|
|
|
\(K_{eff}\) is the effective growth or decay of the neutron population based on
|
|
the prompt reactions. This block can be represented by basic physical quantities
|
|
by using the six factor formula:
|
|
|
|
\[ k_{eff} = \eta f p \epsilon P_{FNL} P_{TNL} \]
|
|
|
|
where:
|
|
|
|
\begin{itemize}
|
|
\item \(\eta\) is the thermal neutron fission factor
|
|
\item \(f\) is the thermal neutron absorption factor
|
|
\item \(p\) is the resonance escape probability
|
|
\item \(\epsilon\) is the fast fission neutron production factor
|
|
\item \(P_{FNL}\) is the fast non-leakage probability
|
|
\item \(P_{TNL}\) is the thermal non-leakage probability
|
|
\end{itemize}
|
|
|
|
\subsection*{Part B}
|
|
|
|
We start with a set of equations representing our neutron populations:
|
|
|
|
\[ N_{in} = N_{f} \]
|
|
\[ N_{f} = N_{p} + N_{decay} + S \Delta t \]
|
|
\[ N_{t} = N_{d} + N_{p} \]
|
|
\[ N_t = K_{eff}N_{in} \]
|
|
|
|
Now, how are these related? Well, the total number of neutrons is split between
|
|
the neutrons that are prompt neutrons and those that are destined to become
|
|
delayed neutrons. We can represent the fraction between the two as:
|
|
|
|
\[ N_t = (1-\beta)K_{eff} N_{in} + \sum_{i=1}^6 \lambda_i C_i \Delta t + S \Delta t \]
|
|
|
|
where
|
|
|
|
\[ N_d = \sum_{i=1}^6 K_{eff} \beta_i N_{in} \]
|
|
and
|
|
\[ N_p = (1-\beta) K_{eff} N_{in} \]
|
|
|
|
Then we find the change in neutron population:
|
|
|
|
\[ N_f - N_i = (1-\beta) K_{eff} N_i + \sum_{i=1}^6 \lambda_i C_i \Delta t + S \Delta t - N_i \]
|
|
|
|
and take the 'derivative':
|
|
|
|
\[ \frac{N_f - N_i}{\Delta t} = \frac{(1- \frac{1}{K_eff} - \beta) K_{eff} N_i}{\Delta t} + \sum_{i=1}^6 \lambda_i C_i + S \]
|
|
|
|
then after a little more substitution found in Fundamental Kinetics Ideas:
|
|
|
|
\[ \dot N(t) = \frac{(\rho - \beta) N(t)}{\Lambda} + \sum_{i=1}^6 \lambda_i C_i + S \]
|
|
|
|
and not forgetting our precursors:
|
|
|
|
\[\dot C_i(t) = \frac{\beta_i}{\Lambda}N(t) - \lambda_i C_i\]
|
|
|
|
|
|
\subsection*{Part C}
|
|
|
|
The prompt jump assumption assumes that the speed of the prompt cycle is so fast
|
|
that we can effectively ignore the dynamics of the prompt neutron effects. It is
|
|
equivalent to us only using the outside loop, and not considering additions from
|
|
\(N_p\).
|
|
|
|
|
|
\subsection*{Part D}
|
|
|
|
First, the number of prompt neutrons would increase dramatically. This would
|
|
happen over the first hundreds of milliseconds. Then, over a much longer time
|
|
horizon (seconds, minutes), the delayed number of neutrons would increase as the
|
|
precursors catch up to the reactivity increase.
|
|
|
|
|
|
\subsection*{Part E}
|
|
|
|
Power turning has to do with start-up rate and the rate at which the total
|
|
neutron population is changing. For this diagram, turning means that \(\dot N_f\) changes sign.
|