The deuterium–tritium fusion reaction

Deuterium–tritium fusion (sometimes abbreviated D+T) is a type of nuclear fusion in which one deuterium nucleus fuses with one tritium nucleus, giving one helium nucleus, one free neutron, and 17.6 MeV of energy. It is the best known fusion reaction for fusion devices.

Tritium, one of the reactants required for this type of fusion, is radioactive. In fusion reactors, a 'breeding blanket' made of lithium is placed on the walls of the reactor, as lithium, when exposed to energetic neutrons, will produce tritium.

Concept

In deuterium–tritium fusion, one deuterium nucleus fuses with one tritium nucleus, yielding one helium nucleus, a free neutron, and 17.6 MeV, which is derived from approximately 0.02 AMUs.[1] The amount of energy obtained is described by the mass-energy relation: . 80% of the energy (14.1 MeV) becomes kinetic energy of the neutron traveling at 1⁄6 the speed of light.

The mass difference between D+T and neutron+4He is decribed by the semi-empirical mass formula that describes the relation between mass defects and binding energy in a nucleus.

Reactant sourcing

About 1 in every 5,000 hydrogen atoms in seawater is deuterium, making it easy to acquire.[1][2]

Tritium, however, is a radioactive isotope, and difficult to source naturally. This can be circumvented by exposing the more readily available lithium to energetic neutrons, which produces tritium nuclei.[1][2] In addition, the deuterium–tritium reaction itself emits a free neutron, which can be used to bombard lithium.[3] A 'breeding blanket', which consists of lithium, is often placed along the walls of fusion reactors such that free neutrons created during deuterium–tritium fusion react with it to produce more tritium.[4][5] This process is called tritium breeding.

Use in fusion reactors

Deuterium–tritium fusion is planned to be used in ITER,[4] as well as many other proposed fusion reactors. It provides many advantages over other types of fusion, as it has a relatively low minimum temperature of 100 million degrees C.[6]

See also

References

  1. 1 2 3 "Nuclear Fusion". Georgia State University. Retrieved January 29, 2021.
  2. 1 2 Lanctot, Matthew. "DOE Explains...deuterium–tritium Fusion Reactor Fuel". Department of Energy. Retrieved April 12, 2021.
  3. ↑ Cowley, Steve. "Introduction to Fusion Part I." (PDF). SULI. Retrieved January 30, 2021.
  4. 1 2 "Fueling the Fusion Reaction". ITER. Retrieved February 12, 2021.
  5. ↑ "Tritium: a challenging fuel for fusion". EUROfusion. November 8, 2017. Retrieved February 16, 2021.
  6. ↑ Schneider, Ursula (August 1, 2001). "Fusion: Energy of the Future". International Atomic Energy Agency. Retrieved February 13, 2021.
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