s-process
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
Ask Britannica AI about this topic
Britannica doesn't have a full article on this topic, so we've curated a list of our relevant coverage.


