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1. Nuclear Reactor Kinetics Craig Marianno
NE 113
2. Effective Multiplication Factor (keff)
3. keff and Power Power is directly proportional to neutron density
keff = 1.0000 ? critical (power constant)
keff < 1.0000 ? subcritical (power decreasing)
keff > 1.0000 ? supercritical (power increasing)
4. k Excess Any difference between a given value for keff and 1.0000 is called the “excess” multiplication factor (?k)
?k = keff - 1.0000 = k excess
5. Reactivity When keff is close to 1.0000, ?k and ? and nearly the same.
Example: keff = 0.98
6. Delayed Neutrons Single most important characteristic for reactor control
Delayed neutrons ? decay of fission products (precursers)
Prompt neutrons ? fission
Fraction of delayed neutrons = ?
Delayed neutrons are more effective than prompt because they are “born” at a somewhat lower energy.
7. Delayed Neutrons
8. Delayed Neutrons
9. Delayed Neutrons While it is true that they are only a small fraction of the total neutron population, they play a vital role in reactor kinetics.
Why?
They significantly increase the neutron cycle lifetime!
10. Prompt Critical
11. Prompt Critical
12. Reactivity in Dollars From our previous example:
13. Neutron Lifetime For reactor kinetics, it is important to know the average time elapsing between the release of a neutron in a fission reaction and its loss from the system either by absorption of escape. This is typically called the “prompt neutron lifetime”. This time can be divided into:
1) Slowing Down Time
2) Thermal Neutron Lifetime (Diffusion Time)
14. Neutron Lifetime
15. Neutron Lifetime(infinite medium - prompt only) ?a = total thermal macroscopic absorption cross section
?a = absorption mean free path
v = mean velocity (2200 m s-1)
Note: - finite size reduces average lifetime due to leakage
- ?a for a core includes all materials
16. Effective Neutron Lifetime(delayed neutrons included) ?eff = effective fraction of delayed neutrons
?eff = effective decay constant of precursors
? = reactivity
17. Reactor Kinetics We need to construct an expression for the number of neutrons per second in the reactor during a given “neutron cycle”.
We could use:
n
k
l
18. Reactor Kinetics Solving:
19. Reactor Period To make the previous equation easier, we can define the reactor period (T) as T = l / ?k.
The reactor period represents the length of time required to change the reactor power by a factor of e (2.718). This is why it is sometimes referred to as the “e folding time”.
20. Reactor Kinetics(Prompt Example) Assuming the following, what is the increase in power for a ?k = 0.0025 ($0.357) at the end of 1.0 s?
?a = 13.2 cm
v = 2200 m s-1
21. Reactor Kinetics(Delayed Example) Assuming the following, what is the increase in power for a ? = 0.0025 ($0.357) at the end of 1.0 s?
? = 0.0813 s-1 ?eff = 0.007
v = 2200 m s-1 l = 6.0X10-5 s