Fusion energy has the potential to supply safe, clean, and nearly limitless power. Although fusion reactions can occur for light nuclei weighting less than iron, most elements will not fuse unless they are in the interior of a star. To create burning plasmas in experimental fusion power reactors such as tokamaks and stellarators, scientists seek a fuel that is relatively easy to produce, store, and bring to fusion. The current best bet for fusion reactors is deuterium-tritium fuel. This fuel reaches fusion conditions at lower temperatures compared to other elements and releases more energy than other fusion reactions.
Deuterium and tritium are isotopes of hydrogen, the most abundant element in the universe. Whereas all isotopes of hydrogen have one proton, deuterium also has one neutron and tritium has two neutrons, so their ion masses are heavier than protium, the isotope of hydrogen with no neutrons. When deuterium and tritium fuse, they create a helium nucleus, which has two protons and two neutrons. The reaction releases an energetic neutron. Fusion power plants would convert energy released from fusion reactions into electricity to power our homes, businesses, and other needs.
Fortunately, deuterium is common. About 1 out of every 5,000 hydrogen atoms in seawater is in the form of deuterium. This means our oceans contain many tons of deuterium. When fusion power becomes a reality, just one gallon of seawater could produce as much energy as 300 gallons of gasoline.
Tritium is a radioactive isotope that decays relatively quickly (it has a 12-year half-life) and is rare in nature. Fortunately, exposing the more abundant element of lithium to energetic neutrons in a fusion reactor can generate tritium. A working fusion power plant could potentially use lithium to breed the tritium it needs to close the deuterium-tritium fuel cycle since lithium can be obtained from the Earth’s crust via ore mining and from salt deserts.
DOE Office of Science: Contributions to Deuterium-Tritium Fuel
Part of the mission of The Department of Energy Office of Science, Fusion Energy Sciences (FES) program is to develop a practical fusion energy source. FES works with the Advanced Scientific Computing Research program using scientific computing to advance fusion science and understand the effect of ion mass on various plasma phenomena. At Office of Science user facilities such as the DIII-D tokamak and NSTX-U spherical tokamak, scientists study the impact of ion mass on plasma confinement, transport, and turbulence. The confinement of fusion products such as the helium ion is also studied in presence of helical magnetic fields. The Office of Science Nuclear Physics program develops the fundamental nuclear science underpinning the understanding of fusion by creating nuclear reaction databases, generating nuclear isotopes, and elucidating aspects of nucleosynthesis.
Deuterium-Tritium Fuel Facts
- Water made from deuterium is about 10 percent heavier than ordinary water. That’s why it is sometimes referred to as “heavy water.” It will actually sink to the bottom of a glass of ordinary water.
- Sources of tritium on Earth include natural production from interactions with cosmic rays, energy-producing nuclear fission reactors such as the heavy water CANDU reactor, and nuclear weapons testing.
- To avoid certain R&D challenges including structural material damage from energetic neutrons, fusion scientists are interested also in aneutronic fusion reactions (such as deuterium-helium-3 and proton-boron fusion) even though these fusion reactions occur at higher ion temperatures than for deuterium and tritium.
Resources and Related Terms
- How does fusion energy work?
- U.S. DOE Office of Science Fusion Energy Sciences program
- Science Up-Close: Developing a Cookbook for Efficient Fusion Energy
- Fusion Research Ignites Innovation
Matthew Lanctot (U.S. DOE Office of Science)
Scientific terms can be confusing. DOE Explains offers straightforward explanations of key words and concepts in fundamental science. It also describes how these concepts apply to the work that the Department of Energy’s Office of Science conducts as it helps the United States excel in research across the scientific spectrum.