The nucleus of an atom stores a staggering amount of energy, roughly a million times more than any chemical bond. Two processes can unlock it: splitting a heavy nucleus apart (fission) or forcing light nuclei together (fusion). Both release energy, but they work in very different ways and under very different conditions.
You will learn how uranium-235 is split by neutron bombardment, how the resulting chain reaction is controlled inside a nuclear reactor, and why fusion, the process that powers every star, remains so difficult to reproduce on Earth. The topic also covers the advantages and limitations of nuclear power compared with fossil fuels.
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Explain nuclear fission
"Physics: Nuclear Fission and Fusion" by OpenStax, OpenStax, Rice University, licensed under CC BY 4.0 (https://creativecommons.org/licenses/by/4.0/). Source: https://openstax.org/books/physics/pages/22-4-nuclear-fission-and-fusion. Access for free at https://openstax.org/books/physics/pages/1-introduction
While basking in the warmth of the summer sun, a student reads of the latest breakthrough in achieving sustained thermonuclear power and vaguely recalls hearing about the cold fusion controversy. The three are connected. The Sun’s energy is produced by nuclear fusion (see Figure 32.13 ). Thermonucle
"College Physics: Fusion" 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/32-5-fusion. Access for free at https://openstax.org/books/college-physics/pages/1-introduction
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