Somewhere inside a working reactor a single neutron is drifting between atoms at a few kilometres a second. It is not aimed and nobody launched it. In a moment it will wander close enough to one particular nucleus to be swallowed, and that nucleus will tear itself in half and fling out two or three more neutrons of its own. Each of those can do the same thing to a neighbour. Left to itself the count goes 1, 2, 4, 8, 16, and twenty steps later it is over a million. Held in check, it goes 1, 1, 1, 1 for years, and a country keeps its lights on.
The difference between those two sequences is a set of metal rods that can be lowered a few centimetres. This lesson takes you through what fission actually is, why a uranium-235 nucleus has to catch a neutron before it can split, and how the arithmetic of one generation feeding the next turns a single split into a power station or into a disaster. You will learn to draw the chain-reaction diagram the specification asks for, count neutrons in and out of a reactor core, compare the energy of one split nucleus with the energy of burning, and finish by weighing the one problem nobody has fully solved: what to do with the waste.
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Nuclear fission is a reaction in which a nucleus is split (or fissured ). Controlled fission is a reality, whereas controlled fusion is a hope for the future. Hundreds of nuclear fission power plants around the world attest to the fact that controlled fission is practical and, at least in the short
"College Physics: Fission" by OpenStax, OpenStax, Rice University, licensed under CC BY 4.0 (https://creativecommons.org/licenses/by/4.0/). Source: https://openstax.org/books/college-physics/pages/32-6-fission. Access for free at https://openstax.org/books/college-physics/pages/1-introduction
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