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Photodisintegration

Photodisintegration (also called phototransmutation, or a photonuclear reaction) is a nuclear process in which an atomic nucleus absorbs a high-energy gamma ray, enters an excited state, and immediately decays by emitting a subatomic particle. It therefore decreases the mass number of the affected nucleus.

Art, Photodisintegration of beryllium & Photodisintegration of deuterium

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Photodisintegration of beryllium

PhotonBeryllium-9Antimony-124Neutron sourcesStartup neutron sources
7 related topics

Photodisintegration of deuterium

DeuteriumProtonNeutronJames ChadwickMaurice Goldhaber
6 related topics

Photodisintegration in lightning

Bursts of gamma-raysBremsstrahlung14 7N13 7NCosmic rays
6 related topics

Hypernovae

Solar massesSupernovaBlack holeRelativistic jetsMetals
5 related topics

Topics to explore

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Overview

Photodisintegration of deuterium

Photodisintegration of beryllium

Hypernovae

Photodisintegration in lightning

Photofission

Advanced semantic analysis

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Map overview Semantic statistics

Photodisintegration

Nodes43
Edges42
Triples4
Avg. degree1.95
Density0.046512
Components1

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Photodisintegration

Top relations

related to Hypernovae · 3
Photodisintegration → As, In, This
is a · 1
Photodisintegration → major factor in the supernova event

Important terminology Word statistics

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Important terminology

energy mass reaction reactions endothermic isotopes lighter process gamma nucleus also exothermic mev rays stable called absorbs iron heavier nuclei

Entity relationships Subject–Predicate–Object triples

SubjectPredicateObjectConfidenceSrc
Photodisintegrationis amajor factor in the supernova event0.90text
Photodisintegrationrelated to HypernovaeIn0.60section
Photodisintegrationrelated to HypernovaeAs0.60section
Photodisintegrationrelated to HypernovaeThis0.60section

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    Min side: 3
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