4.2. Reactor Power
At any time \(t\), the local power production at position \(\overrightarrow{r}\) is assumed to be given by the space-time separated function:
where \(\psi_{\text{t}}\left( t \right)\) is the dimensionless, normalized
power amplitude and \(S\left( \overrightarrow{r} \right)\) is the
steady-state reactor power in watts being produced in an axial node at
location \(\overrightarrow{r}\). In terms of input quantities,
\(S\left( \overrightarrow{r} \right)\) is given by the product of
POW
and PSHAPE
. Initially, the power amplitude has a value of unity and
\(S\left( \overrightarrow{r} \right)\) is normalized to the total
steady-state reactor power. Appendix 4.1 contains a description of the
internal normalization of PSHAPE performed by SAS4A/SASSYS‑1. The
time-dependent power amplitude is assumed to be made up of the sum of
two components:
where \(\psi_{\text{h}}\left( t \right)\) comes from the decay of fission and capture products. These two components have been separated to allow the simulation of both short- and long-term transients.
The direct fission component of the power amplitude is given by
where \(\phi \left( t \right)\) is the dimensionless, normalized fission power amplitude given by the point reactor kinetics model:
with the initial condition \(\phi\left( 0 \right) = 1\).
In Eq. (4.2-4), \(\delta k \left( t \right)\) is the net reactivity, \(\beta\) is the total effective delayed-neutron fraction, \(\Lambda\) is the effective prompt neutron generation time, and \(\lambda_{\text{i}}\) is the decay constant for the delayed-neutron precursor isotope whose normalized population is \(C_{\text{i}}\left( t \right)\). The physical interpretation of the terms in the point reactor kinetics equation is made by Henry [4-2] and also by Bell and Glasstone [4-3].