When they finally published the results in 1939, they came to the attention of Lise Meitner, an Austrian-born physicist who had worked with Hahn on his nuclear experiments. She was the first to realize that Hahn’s barium and other lighter products from the neutron bombardment experiments were coming from the fission of U-235. Meitner and Frisch carried out further experiments which showed that the U-235 fission can release large amounts of energy both as electromagnetic radiation and as kinetic energy of the fragments (heating the bulk material where fission takes place). They realized that this made possible a chain reaction with an unprecedented energy yield.
Critical Energy – Threshold Energy for Fission
The critical energy depends on the nuclear structure and is quite large for light nuclei with Z < 90. For heavier nuclei with Z > 90, the critical energy is about 4 to 6 MeV for A-even nuclei, and generally is much lower for A-odd nuclei. It must be noted, some heavy nuclei (eg. 240Pu or 252Cf) exhibit fission even in the ground state (without externally added excitation energy). This phenomena is known as the spontaneous fission. This process occur without the addition of the critical energy by the quantum-mechanical process of quantum tunneling through the Coulomb barrier (similarly like alpha particles in the alpha decay). The spontaneous fission contributes to ensure sufficient neutron flux on source range detectors when reactor is subcritical in long term shutdown.
Prompt and Delayed Neutrons
But not all neutrons are released at the same time following fission. Even the nature of creation of these neutrons is different. From this point of view we usually divide the fission neutrons into two following groups:
- Prompt Neutrons. Prompt neutrons are emitted directly from fission and they are emitted within very short time of about 10-14 second.
- Delayed Neutrons. Delayed neutrons are emitted by neutron rich fission fragments that are called the delayed neutron precursors. These precursors usually undergo beta decay but a small fraction of them are excited enough to undergo neutron emission. The fact the neutron is produced via this type of decay and this happens orders of magnitude later compared to the emission of the prompt neutrons, plays an extremely important role in the control of the reactor.
See also: Prompt Neutrons
See also: Delayed Neutrons
Key Characteristics of Prompt Neutrons
- Prompt neutrons are emitted directly from fission and they are emitted within very short time of about 10-14 second.
- Most of the neutrons produced in fission are prompt neutrons – about 99.9%.
- For example a fission of 235U by thermal neutron yields 2.43 neutrons, of which 2.42 neutrons are prompt neutrons and 0.01585 neutrons are the delayed neutrons.
- The production of prompt neutrons slightly increase with incident neutron energy.
- Almost all prompt fission neutrons have energies between 0.1 MeV and 10 MeV.
- The mean neutron energy is about 2 MeV. The most probable neutron energy is about 0.7 MeV.
- In reactor design the prompt neutron lifetime (PNL) belongs to key neutron-physical characteristics of reactor core.
- Its value depends especially on the type of the moderator and on the energy of the neutrons causing fission.
- In an infinite reactor (without escape) prompt neutron lifetime is the sum of the slowing down time and the diffusion time.
- In LWRs the PNL increases with the fuel burnup.
- The typical prompt neutron lifetime in thermal reactors is on the order of 10-4 second.
- The typical prompt neutron lifetime in fast reactors is on the order of 10-7 second.
Key Characteristics of Delayed Neutrons
- The presence of delayed neutrons is perhaps most important aspect of the fission process from the viewpoint of reactor control.
- Delayed neutrons are emitted by neutron rich fission fragments that are called the delayed neutron precursors.
- These precursors usually undergo beta decay but a small fraction of them are excited enough to undergo neutron emission.
- The emission of neutron happens orders of magnitude later compared to the emission of the prompt neutrons.
- About 240 n-emitters are known between 8He and 210Tl, about 75 of them are in the non-fission region.
- In order to simplify reactor kinetic calculations it is suggested to group together the precursors based on their half-lives.
- Therefore delayed neutrons are traditionally represented by six delayed neutron groups.
- Neutrons can be produced also in (γ, n) reactions (especially in reactors with heavy water moderator) and therefore they are usually referred to as photoneutrons. Photoneutrons are usually treated no differently than regular delayed neutrons in the kinetic calculations.
- The total yield of delayed neutrons per fission, vd, depends on:
- Isotope, that is fissioned.
- Energy of a neutron that induces fission.
- Variation among individual group yields is much greater than variation among group periods.
- In reactor kinetic calculations it is convenient to use relative units usually referred to as delayed neutron fraction (DNF).
- At the steady state condition of criticality, with keff = 1, the delayed neutron fraction is equal to the precursor yield fraction β.
- In LWRs the β decreases with fuel burnup. This is due to isotopic changes in the fuel.
- Delayed neutrons have initial energy between 0.3 and 0.9 MeV with an average energy of 0.4 MeV.
- Depending on the type of the reactor, and their spectrum, the delayed neutrons may be more (in thermal reactors) or less effective than prompt neutrons (in fast reactors). In order to include this effect into the reactor kinetic calculations the effective delayed neutron fraction – βeff must be defined.
- The effective delayed neutron fraction is the product of the average delayed neutron fraction and the importance factor βeff = β . I.
- The weighted delayed generation time is given by τ = ∑iτi . βi / β = 13.05 s, therefore the weighted decay constant λ = 1 / τ ≈ 0.08 s-1.
- The mean generation time with delayed neutrons is about ~0.1 s, rather than ~10-5 as in section Prompt Neutron Lifetime, where the delayed neutrons were omitted.
- Their presence completely changes the dynamic time response of a reactor to some reactivity change, making it controllable by control systems such as the control rods.
- Basics of Nuclear Fission
- Chain reaction
- Youtube animation
- Principles of Nuclear Fission
- Nuclear Binding Energy
- Liquid Drop Model
- Critical Energy – Threshold Energy for Fission
- Energy Release from Fission
- Fission Fragments – Products of Nuclear Fission
- Prompt and Delayed Neutrons
- Key Characteristics of Prompt Neutrons
- Key Characteristics of Delayed Neutrons
- Capture-to-Fission Ratio
- Nuclear Fission Chain Reaction
- Distinction between Fissionable, Fissile and Fertile
- Neutron Nuclear Reactions