Astrophysics (Index)About

photodisintegration

(breakdown of a nucleus by a gamma ray)

Photodisintegration is a nuclear process triggered by a photon: a gamma ray entering a nucleus and exciting it sufficiently that it emits a subatomic particle, generally the same types as those emitted in radioactive decay. The term photofission is used if the nucleus splits into two nuclei of more-equal mass.

A photon with less energy may still have enough to ionize an atom (photoionization), and with even less, may still have enough to separate the atoms of a molecule (photodissociation).


(atoms,metals,nucleosynthesis)
Further reading:
https://en.wikipedia.org/wiki/Photodisintegration
https://en.wikipedia.org/wiki/Photofission
https://astronomy.swin.edu.au/cosmos/P/Photodisintegration
https://dictionary.obspm.fr/index.php?showAll=1&formSearchTextfield=photodisintegration

Referenced by pages:
neon burning
nuclear statistical equilibrium (NSE)
nucleosynthesis
photodissociation

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