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	<title>Photodisintegration - Revision history</title>
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	<updated>2026-04-21T14:07:58Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
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	<entry>
		<id>https://wikimd.com/index.php?title=Photodisintegration&amp;diff=5987155&amp;oldid=prev</id>
		<title>Prab: CSV import</title>
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		<updated>2024-07-14T02:12:49Z</updated>

		<summary type="html">&lt;p&gt;CSV import&lt;/p&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #202122; text-align: center;&quot;&gt;Revision as of 02:12, 14 July 2024&lt;/td&gt;
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		<author><name>Prab</name></author>
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	<entry>
		<id>https://wikimd.com/index.php?title=Photodisintegration&amp;diff=5391558&amp;oldid=prev</id>
		<title>Prab: CSV import</title>
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		<updated>2024-03-11T08:27:35Z</updated>

		<summary type="html">&lt;p&gt;CSV import&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;&amp;#039;&amp;#039;&amp;#039;Photodisintegration&amp;#039;&amp;#039;&amp;#039; is a nuclear process in which an atomic nucleus absorbs a high-energy gamma ray, causing it to enter an excited state and immediately emit a subatomic particle. This process is a key mechanism in the [[astrophysics|astrophysical]] production of heavy elements, particularly in environments with high-energy radiation, such as [[supernova]]e and active galactic nuclei.&lt;br /&gt;
&lt;br /&gt;
== Overview ==&lt;br /&gt;
&lt;br /&gt;
Photodisintegration is a type of [[nuclear reaction]] that occurs when a nucleus absorbs a gamma ray and emits a particle. This process is the reverse of [[photoelectric effect|photoelectric]] and [[Compton scattering]], where a gamma ray is absorbed and an electron is emitted. &lt;br /&gt;
&lt;br /&gt;
In photodisintegration, the absorbed gamma ray has enough energy to overcome the [[nuclear binding energy]], causing the nucleus to emit a particle. The emitted particle can be a proton, neutron, alpha particle, or another nucleus, depending on the specific reaction.&lt;br /&gt;
&lt;br /&gt;
== Role in Astrophysics ==&lt;br /&gt;
&lt;br /&gt;
Photodisintegration plays a crucial role in the production of heavy elements in the universe. In high-energy environments such as supernovae and active galactic nuclei, the intense radiation can cause nuclei to undergo photodisintegration. This process can lead to the production of heavy elements through a series of reactions known as the [[r-process]].&lt;br /&gt;
&lt;br /&gt;
The r-process, or rapid neutron-capture process, involves the rapid absorption of neutrons by a nucleus, followed by beta decay. Photodisintegration can provide the necessary neutrons for this process, contributing to the synthesis of heavy elements.&lt;br /&gt;
&lt;br /&gt;
== See Also ==&lt;br /&gt;
&lt;br /&gt;
* [[Nuclear physics]]&lt;br /&gt;
* [[Nuclear reaction]]&lt;br /&gt;
* [[Gamma ray]]&lt;br /&gt;
* [[Supernova]]&lt;br /&gt;
* [[r-process]]&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
&lt;br /&gt;
&amp;lt;references /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[Category:Physics]]&lt;br /&gt;
[[Category:Nuclear physics]]&lt;br /&gt;
[[Category:Astrophysics]]&lt;br /&gt;
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{{medicine-stub}}&lt;/div&gt;</summary>
		<author><name>Prab</name></author>
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