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s-process

physics
Also known as: slow neutron capture, slow neutron process, slow process(Show More)

Quick Summary

The s-process, or slow neutron capture, is a key mechanism in astrophysics responsible for creating heavier chemical elements. This process occurs when atomic nuclei capture neutrons at a relatively slow rate. If a nucleus captures a neutron and becomes unstable, it undergoes beta decay (converting a neutron into a proton) before it can capture another neutron. This allows for the gradual buildup of heavier elements, particularly those with more protons.

The s-process is believed to happen during the stable phases of stellar evolution. In contrast, the r-process (rapid neutron capture) occurs in more explosive stellar events. Together, these neutron capture processes help explain the observed abundances of elements heavier than iron in the universe.1

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