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14 декабря, 2021
The space-independent neutron kinetics equations are dn/dt = [{p — P)/A]n + £ ЛС;
І = 1
dCJdt = — ЛІСІ
where n is the neutron density (proportional to power level), p the reactivity, P the total delayed neutron fraction, A the neutron generation time, 2, the decay constant for ith delayed neutron precursor group, C, the concentration of the ith delayed neutron precursor, and the delayed neutron fraction for delayed neutron group i.
The transfer function obtained from these equations is
TABLE 5.1 Delayed Neutron Yield from Thermal Fission in 233U, 225U, and 239Pu“
From Keepin (1). |
where n0 is the steady-state neutron density. The delayed-neutron parameters needed for theoretical calculations of the frequency response are shown in Table 5.1. Zero-power frequency response results for a reactor with 235U fuel are shown in Fig. 5.1.
Fig. 5.1. (a)Amplitude for a 235U-fueled, zero-power reactor, (b) phase shift for a 235U — fueled, zero-power reactor. |
An approximate transfer function based on a single effective group of delayed neutrons is often used. The transfer function is
Sn _ n0(s + X) dp As(s + X + p/A)
where X is the average decay constant (sO. l sec-*).