The precise boundaries of neutron energy ranges are not well defined, and differ between sources, but some common names and limits are given in the following table. The following is a detailed classification:
Thermal A
thermal neutron is a free neutron with a kinetic energy of about 0.025
eV (about 4.0×10−21
J or 2.4 MJ/kg, hence a speed of 2.19 km/s), which is the energy corresponding to the most probable speed at a temperature of 290 K (17 °C or 62 °F), the
mode of the
Maxwell–Boltzmann distribution for this temperature, Epeak =
k T. After a number of collisions with nuclei (
scattering) in a medium (
neutron moderator) at this temperature, those
neutrons which are not absorbed reach about this energy level. Thermal neutrons have a different and sometimes much larger effective
neutron absorption cross-section for a given
nuclide than fast neutrons, and can therefore often be absorbed more easily by an
atomic nucleus, creating a heavier, often
unstable isotope of the
chemical element as a result. This event is called
neutron activation.
Epithermal Epithermal neutrons are those with energies above the thermal energy at room temperature (i.e. 0.025 eV). Depending on the context, this can encompass all energies up to fast neutrons (as in e.g.). This includes neutrons produced by conversion of accelerated protons in a pitcher-catcher geometry
Cold (slow) neutrons Cold neutrons are thermal neutrons that have been equilibrated in a very cold substance such as liquid
deuterium. Such a
cold source is placed in the moderator of a research reactor or spallation source. Cold neutrons are particularly valuable for
neutron scattering experiments.
Ultracold neutrons are produced by inelastic scattering of cold neutrons in substances with a low neutron absorption cross section at a temperature of a few kelvins, such as solid
deuterium or superfluid
helium. An alternative production method is the mechanical deceleration of cold neutrons exploiting the Doppler shift. Ultra-cold neutrons reflect at all angles of incidence. This is because their momentum is comparable to the optical potential of materials. This effect is used to store them in bottles and study their fundamental properties e.g. lifetime, neutron electrical-dipole moment etc... The main limitations of the use of slow neutrons is the low flux and the lack of efficient optical devices (in the case of CN and VCN). Efficient neutron optical components are being developed and optimized to remedy this lack.
Fast A
fast neutron is a free neutron with a kinetic energy level close to 1
MeV (100
TJ/
kg), hence a speed of 14,000 km/
s or higher. They are named
fast neutrons to distinguish them from lower-energy thermal neutrons, and high-energy neutrons produced in cosmic showers or accelerators. Fast neutrons are produced by nuclear processes: •
Nuclear fission: thermal fission of produces neutrons with a mean energy of 2 MeV (200 TJ/kg, i.e. 20,000 km/s), which qualifies as "fast". However, the energy spectrum of these neutrons approximately follows a
right-skewed Watt distribution N(E) \propto \exp(-aE) \sinh(\sqrt{bE}), with a range of 0 to about 17 MeV, and a
mode of 0.75 MeV. ==Fast-neutron reactor and thermal-neutron reactor compared==