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Uranium-236

Isotope of uranium

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Through Radioactive waste, Nuclear fission and Gamma ray

Creation and yield

The fissile isotope uranium-235 fuels most nuclear reactors. When 235U absorbs a thermal neutron, one of two processes can occur. About 85.5% of the time, it will fission; about 14.5% of the time, it will not fission, instead emitting gamma radiation and yielding 236U. Thus, the yield of 236U per 235U+n reaction is about 14.5%, and the yield of fission products is about 85.5%. In comparison, the yields of the most abundant individual fission products like caesium-137, strontium-90, and technetium-99 are between 6% and 7%, and the combined yield of medium-lived (10 years and up) and long-lived fission products is about 32%, or a few percent less as some are transmuted by neutron capture.

The second-most used fissile isotope plutonium-239 can similarly fission or not on absorbing a thermal neutron, the latter giving plutonium-240, a major component of reactor-grade plutonium (plutonium recycled from spent fuel that was originally made with enriched natural uranium and then used once in an LWR). 240Pu decays with a half-life of 6561 years into 236U. In a closed nuclear fuel cycle, most 240Pu will fission (possibly after more than one neutron capture) before it decays, but 240Pu discarded as nuclear waste will decay over thousands of years. As 240Pu has a shorter half-life than 239Pu, the grade of any sample of plutonium mostly composed of those two isotopes will slowly increase, while the total amount of plutonium in the sample will slowly decrease over centuries and millennia. Alpha decay of 240Pu produces uranium-236, while 239Pu decays to uranium-235.

While the largest part of uranium-236 has been produced by neutron capture in nuclear power reactors, that part is nearly all stored in nuclear reactors and waste repositories and has not been released to the environment. The most significant environmental contribution is the 238U(n,3n)236U reaction by fast neutrons in thermonuclear weapons. The nuclear testing of the 1940s, 1950s, and 1960s (atmospheric testing ended 1963) has raised the environmental abundance levels significantly above the expected natural levels.

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