**Fission neutrons** are neutrons produced in nuclear fission. They have typical spectrum and it is known the **fission neutrons** are of importance in any chain-reacting system. Neutrons trigger the nuclear fission of some nuclei (^{235}U, ^{238}U or even ^{232}Th). What is crucial the fission of such nuclei produces **2, 3 or more** free 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.

## Spectrum of Fission Neutrons

### Region of Fast Neutrons

The first part of the **neutron flux spectrum** in thermal reactors, is the **region of fast neutrons**. All neutrons produced by fission are born as **fast neutrons** with high kinetic energy.

At first we have to distinguish between **fast neutrons** and prompt neutrons. The prompt neutrons can be sometimes** incorretly** confused with the fast neutrons. But there is an essential difference between them.** Fast neutrons** are neutrons categorized according to the **kinetic energy**, while** prompt neutrons** are categorized according to the** time of their release**.

Most of the neutrons produced in fission are prompt neutrons. Usually **more than 99 percent** of the fission neutrons are the prompt neutrons, but the exact fraction is dependent on the nuclide to be fissioned and is also dependent on an incident neutron energy (usually increases with energy). For example a fission of ^{235}U by thermal neutron yields **2.43 neutrons**, of which **2.42 neutrons are the prompt neutrons** and 0.01585 neutrons **(0.01585/2.43=0.0065=ß)** are **the delayed neutrons**.

The vast of the prompt neutrons and even the delayed neutrons are born as fast neutrons (i.e. with kinetic energy higher than > 1 keV). But these two groups of **fission neutrons** have different energy spectra, therefore they contribute to the fission spectrum differently. Since **more than 99 percent** of the fission neutrons are the prompt neutrons, it is obvious, that they will dominate the entire spectrum.

Therefore the fast neutron spectrum can be described by following points:

- Almost all 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**.

The fast neutron spectrum can be approximated by the following (normalized to one) distribution:

The neutrons released during fission with an average energy of **2 MeV** in a reactor on average undergo a **number of collisions** (elastic or inelastic) before they are absorbed. As a result of these collisions** they lose energy**, so that the **reactor spectrum is not identical to the fission spectrum**, it is always **‘softer’** than the fission spectrum. The fact is that the fission spectrum is the part of the reactor spectrum.

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