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Atlas / Physics / The Nuclear Thread

Field · Emerged 1934 – 1942

Nuclear Fission

How can a nucleus be split, and how can splitting one make others split in turn?

5 chapters5 min read7 turning points1 open problem

Branched from
Nuclear Structure
Branched into
Not yet surveyed past here
Figures
Enrico Fermi, Ida Noddack, Otto Hahn, Fritz Strassmann, Lise Meitner, Otto Frisch, Leo Szilard, Niels Bohr, John Archibald Wheeler, J. Robert Oppenheimer, Paul Kazuo Kuroda

In brief

Fission is the splitting of a heavy nucleus, such as uranium, into two lighter ones. It releases about 200 million electronvolts, fifty million times more than burning one atom of carbon. It also releases two or three neutrons, which can split further nuclei. If enough of them do, the process sustains itself: a chain reaction.

Fission was discovered by chemists who did not at first believe their own results, and explained by a physicist in exile. It went from a puzzling trace of barium in December 1938 to a working reactor in December 1942 and two destroyed cities in August 1945. It now supplies about a tenth of the world's electricity. A natural reactor that ran two billion years ago in Gabon shows that nature found the trick first.

Key ideas

FissionEnters 1938 – 1939

The splitting of a heavy nucleus into two fragments of roughly half its size, releasing about 200 MeV of energy and a few free neutrons.

Slow neutronsEnters 1934

Neutrons slowed by collisions with light atoms, such as the hydrogen in water or the carbon in graphite, are far more likely to be captured by a nucleus than fast ones. A material that slows them is called a moderator.

Uranium-235Enters 1939

The rare isotope of uranium, 0.7% of natural uranium, that splits readily when it captures a slow neutron. The common isotope, uranium-238, does not.

Chain reaction and critical massEnters 1942

Each fission releases neutrons that cause more fissions. When on average exactly one goes on to cause another, the reaction is steady and the assembly is critical. More than one, and it grows.

Natural reactorEnters 1972

A uranium ore deposit in which a chain reaction started by itself, possible only when uranium-235 made up a larger share of natural uranium than it does today.

Chapter I

Beyond Uranium

When the neutron was found in 1932, physicists had a projectile that nuclei do not repel. In Rome, Enrico Fermi and his young group fired neutrons at every element they could get, and found that most of them became radioactive. In October 1934 they noticed that neutrons passed through paraffin wax, which is rich in hydrogen, became far more effective. Slowed by collisions, they lingered near nuclei and were captured more easily. Bombarding uranium, the heaviest element, gave activities that Fermi's group took to be new elements beyond it.

The chemist Ida Noddack objected in print that the uranium nucleus might instead have broken into several large pieces. Nobody took the idea up. Splitting a nucleus seemed impossible. Every known reaction chipped off at most an alpha particle.

Chapter II

Barium

In Berlin, the chemist Otto Hahn and the physicist Lise Meitner had worked together for thirty years. In July 1938 Meitner, Jewish by birth and no longer protected by her Austrian citizenship after the annexation of Austria, fled Germany. Hahn and Fritz Strassmann continued the uranium work. In December they found that one product, which they took for radium, behaved exactly like barium. It was barium, element 56. Hahn wrote to Meitner asking for "some fantastic explanation".

Over Christmas, in the Swedish village of Kungälv, Meitner and her nephew Otto Frisch found one. Bohr's liquid-drop picture of the nucleus suggested that a uranium nucleus, with so many protons repelling each other, is barely held together. A neutron can set it wobbling until it pinches in two. Meitner remembered how to compute the masses, and the missing mass came to about 200 MeV, just the energy the fragments should have. Frisch called the process fission, after the division of cells.

Chapter III

The Chain Reaction

Niels Bohr carried the news to America in January 1939. Within weeks the fission fragments had been seen in several laboratories, and each fission was found to release two or three neutrons. Bohr and John Wheeler showed that slow neutrons split only the rare isotope uranium-235. If the released neutrons could split more uranium-235, the reaction could sustain itself. Leo Szilard, who had imagined a nuclear chain reaction in 1933, persuaded Einstein to warn President Roosevelt.

On 2 December 1942, under the stands of a sports ground at the University of Chicago, Fermi's team withdrew the last control rod from a pile of graphite and uranium, and the neutron count rose steadily. The chain reaction worked. The Manhattan Project, led at Los Alamos by J. Robert Oppenheimer, turned it into weapons. One bomb destroyed Hiroshima on 6 August 1945 and another Nagasaki three days later. After the war, reactors were built to make electricity.

In 1972 French analysts found uranium from the Oklo mine in Gabon depleted in uranium-235. Two billion years earlier, uranium-235 had made up a larger share of natural uranium, and groundwater had moderated natural chain reactions in the ore. Paul Kuroda had predicted exactly this in 1956.

Chapter IV

A Closer Look: Fifty Million Times Coal

Meitner's estimate. Just after splitting, two fragments each carrying 46 protons touch. A nucleus of 118 particles has a radius of about 1.2×1181/3≈5.91.2 \times 118^{1/3} \approx 5.9 femtometres, so their centres are about 11.8 fm apart. The electrical energy pushing them apart is

E=1.44 MeV fm×46×4611.8 fm≈260 MeV.E = \frac{1.44\ \text{MeV fm} \times 46 \times 46}{11.8\ \text{fm}} \approx 260\ \text{MeV} .

The binding-energy curve gives the same order. Uranium binds each of its 235 particles by about 7.6 MeV, the fragments by about 8.5 MeV, and 235×0.9≈210235 \times 0.9 \approx 210 MeV. The measured value is about 200 MeV per fission.

Compared with burning. Burning one carbon atom to carbon dioxide releases about 4 eV. One fission releases 200 MeV, fifty million times more. Per kilogram:

FuelEnergy per atomEnergy per kilogram
Carbon, burned4.1 eV3.3×1073.3 \times 10^{7} J
Uranium-235, fissioned200 MeV8.2×10138.2 \times 10^{13} J

A kilogram of uranium-235 contains 1000/235×6.022×1023≈2.56×10241000 / 235 \times 6.022 \times 10^{23} \approx 2.56 \times 10^{24} atoms. Multiplying by 200 MeV, or 3.2×10−113.2 \times 10^{-11} J, gives 8.2×10138.2 \times 10^{13} J, about 2.5 million times the energy of a kilogram of carbon.

Hiroshima. The yield of the Hiroshima bomb is estimated at about 15 kilotons of TNT, which is 15×4.18×1012≈6.3×101315 \times 4.18 \times 10^{12} \approx 6.3 \times 10^{13} J. Dividing by the energy per kilogram, about 0.76 kg of uranium actually fissioned, of the roughly 64 kg in the bomb. Less than the mass of a bag of sugar destroyed a city.

Oklo. Uranium-235 decays faster than uranium-238, with half-lives of 0.70 and 4.47 billion years. Today it is 0.72% of natural uranium. Running both decays back two billion years gives 3.7%, similar to the enriched fuel of a modern water-cooled reactor. That is why natural reactors could run then and cannot now.

Chapter V

After Fission

Fission gave the twentieth century its most powerful weapon and a low-carbon source of electricity, and both have been fiercely argued over ever since. Reactors also supply the isotopes of nuclear medicine and the neutrons of many physics experiments. The bomb made the next step possible: its heat could ignite the fusion of hydrogen, the subject of fusion energy. And the splitting itself is still not fully understood. No theory yet predicts, from the forces between protons and neutrons, how a nucleus will break.

Applications

Where it is used

  • Energy

    Nuclear power

    Fission reactors boil water with the heat of fission fragments. About 440 reactors supply roughly a tenth of the world's electricity with almost no carbon emissions. The accidents at Chernobyl in 1986 and Fukushima in 2011, and the long-lived waste, have kept the technology contested.

    › Sources (1)
  • Medicine

    Reactor-made isotopes

    Most medical isotopes are made in research reactors. Molybdenum-99, a fission product, decays into technetium-99m, the workhorse of nuclear medicine imaging. Shortages when a few ageing reactors shut down for repairs, as in 2009 and 2010, delayed scans around the world.

  • Fundamental constants

    Oklo as a test of physics

    The Oklo reactors captured neutrons at rates that depend very sensitively on nuclear energy levels, which in turn depend on the strength of electromagnetism. The isotopes left behind show that the fine-structure constant has changed by less than about one part in ten million over two billion years.

    › Sources (1)
    • Shlyakhter, A. I. (1976). Direct test of the constancy of fundamental nuclear constants. Nature 264: 340.

Open problems

Where the map runs out

Open

Can fission be calculated from first principles?

Open as of 2026. Large computer calculations now follow a splitting nucleus, but still rely on fitted forces.

More than eighty years after its discovery, fission is still described largely by models tuned to data. Why uranium usually splits into unequal fragments, one near mass 95 and one near 140, what share of energy each fragment receives, and how many neutrons it emits, cannot yet be predicted precisely from the forces between protons and neutrons.

Why it is hard

A fissioning nucleus is hundreds of particles rearranging collectively while exchanging energy with their own motion, a problem between the single-particle picture of the shell model and the collective picture of the liquid drop. The nuclear force itself is known only approximately.

What resolving it unlocks

Reliable data for reactors and waste management, fission of exotic nuclei in the stellar explosions that make heavy elements, and a test of nuclear theory in its hardest regime.

› Sources (1)
  • Schunck, N. & Robledo, L. M. (2016). Microscopic theory of nuclear fission: a review. Reports on Progress in Physics 79: 116301.

Further reading

  1. Rhodes, R. (1986). The Making of the Atomic Bomb. Simon & Schuster.

    The classic history, from the physics of the 1930s to Hiroshima. Pulitzer prize winner.

  2. Sime, R. L. (1996). Lise Meitner: A Life in Physics. University of California Press.

    The biography that restored Meitner's place in the discovery of fission.

  3. Frisch, O. R. (1979). What Little I Remember. Cambridge University Press.

    Frisch's memoir, including the walk in the snow that explained fission.