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	<id>https://wiki.iac.isu.edu/index.php?action=history&amp;feed=atom&amp;title=Gamma_Emission</id>
	<title>Gamma Emission - Revision history</title>
	<link rel="self" type="application/atom+xml" href="https://wiki.iac.isu.edu/index.php?action=history&amp;feed=atom&amp;title=Gamma_Emission"/>
	<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Gamma_Emission&amp;action=history"/>
	<updated>2026-07-12T14:39:54Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
	<generator>MediaWiki 1.35.2</generator>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Gamma_Emission&amp;diff=100115&amp;oldid=prev</id>
		<title>Abdehait: /* Photoabosrption and Scattering */</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Gamma_Emission&amp;diff=100115&amp;oldid=prev"/>
		<updated>2015-04-04T00:29:48Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Photoabosrption and Scattering&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left diff-editfont-monospace&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&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 00:29, 4 April 2015&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l7&quot; &gt;Line 7:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 7:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;the figures show that the highest intensity is for the photon of energy of 42, 54, and 440 keV, and the rest of the relative intensities for the other energies are below 26 percent. &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;So most probable, if &lt;/del&gt;U-233 emits a photon, it will transit the drift region up to 99%, but it may interact with Ar/CO2 gas by photoabsorption  according to G4 simulation &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;for a photon that carries one of the energies mentioned above&lt;/del&gt;, and &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;travels through a 1 cm wide region of Ar/CO2 gas. &lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;the figures show that the highest intensity is for the photon of energy of 42, 54, and 440 keV, and the rest of the relative intensities for the other energies are below 26 percent. &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;If &lt;/ins&gt;U-233 emits a photon &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;that carries one of the energies mentioned above, and travels through a 1 cm wide region of Ar/CO2 gas&lt;/ins&gt;, it will transit the drift region up to 99&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;.96&lt;/ins&gt;%, but &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;within 0.04 % &lt;/ins&gt;it may interact with Ar/CO2 gas by photoabsorption  according to G4 simulation, and &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;when an interaction happens,  &lt;/ins&gt;an electron leaves the atom &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;carrying &lt;/ins&gt;almost the same as the photon energy, its primary, secondary, and number of photons that are combined will be estimated by the previous simulations for beta particles.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt; &lt;/div&gt;&lt;/td&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt; &lt;/div&gt;&lt;/td&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;If &lt;/del&gt;an electron leaves the atom &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;by photoabsorption, it will carry &lt;/del&gt;almost the same as the photon energy, its primary, secondary, and number of photons that are combined &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;to its interations &lt;/del&gt;will be estimated by the previous simulations for &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;the &lt;/del&gt;beta particles.&lt;/div&gt;&lt;/td&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Gamma_Emission&amp;diff=100114&amp;oldid=prev</id>
		<title>Abdehait: /* Photoabosrption and Scattering */</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Gamma_Emission&amp;diff=100114&amp;oldid=prev"/>
		<updated>2015-04-04T00:25:10Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Photoabosrption and Scattering&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left diff-editfont-monospace&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&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 00:25, 4 April 2015&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l7&quot; &gt;Line 7:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 7:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;the figures show that the highest intensity is for the photon of energy of 42 keV, and the rest of the relative intensities for the other energies are below 26 percent. &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;As a result, Most &lt;/del&gt;probable, if U-233 emits a photon, it will &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;interacts &lt;/del&gt;with Ar/CO2 gas by photoabsorption, an electron &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;will will leave &lt;/del&gt;the atom &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;carrying &lt;/del&gt;almost the same as the photon energy, its primary, secondary, and number of photons that are combined to its interations will be estimated by the previous simulations for the beta particles.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;the figures show that the highest intensity is for the photon of energy of 42&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, 54, and 440 &lt;/ins&gt;keV, and the rest of the relative intensities for the other energies are below 26 percent. &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;So most &lt;/ins&gt;probable, if U-233 emits a photon, it will &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;transit the drift region up to 99%, but it may interact &lt;/ins&gt;with Ar/CO2 gas by photoabsorption &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt; according to G4 simulation for a photon that carries one of the energies mentioned above&lt;/ins&gt;, &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;and travels through a 1 cm wide region of Ar/CO2 gas. &lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt; &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt; &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;If &lt;/ins&gt;an electron &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;leaves &lt;/ins&gt;the atom &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;by photoabsorption, it will carry &lt;/ins&gt;almost the same as the photon energy, its primary, secondary, and number of photons that are combined to its interations will be estimated by the previous simulations for the beta particles.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Gamma_Emission&amp;diff=100105&amp;oldid=prev</id>
		<title>Abdehait: /* Photoabosrption and Scattering */</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Gamma_Emission&amp;diff=100105&amp;oldid=prev"/>
		<updated>2015-04-02T16:55:39Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Photoabosrption and Scattering&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left diff-editfont-monospace&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&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 16:55, 2 April 2015&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l7&quot; &gt;Line 7:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 7:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;the figures show that the highest intensity is for the photon of energy of 42 keV, and the rest of the relative intensities for the other energies are below 26 percent. As a result, if U-&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;233phton is&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;the figures show that the highest intensity is for the photon of energy of 42 keV, and the rest of the relative intensities for the other energies are below 26 percent. As a result&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, Most probable&lt;/ins&gt;, if U-&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;233 emits a photon, it will interacts with Ar/CO2 gas by photoabsorption, an electron will will leave the atom carrying almost the same as the photon energy, its primary, secondary, and number of photons that are combined to its interations will be estimated by the previous simulations for the beta particles.&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Gamma_Emission&amp;diff=100102&amp;oldid=prev</id>
		<title>Abdehait: /* Photoabosrption and Scattering */</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Gamma_Emission&amp;diff=100102&amp;oldid=prev"/>
		<updated>2015-04-02T16:48:27Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Photoabosrption and Scattering&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left diff-editfont-monospace&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&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 16:48, 2 April 2015&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l3&quot; &gt;Line 3:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 3:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;U-233 emits gamma particles  that interact with Ar/CO2 gas. U-233 emits gamma particles in the range as it is inside the gaseous chamber, the energy range for those gammas is 42 keV to 807 keV. (Ref.) the figures below show the expected photon interactions in Ar/CO2 90/10  and the relative intensity for emitting them,&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;U-233 emits gamma particles  that interact with Ar/CO2 gas. U-233 emits gamma particles in the range as it is inside the gaseous chamber, the energy range for those gammas is 42 keV to 807 keV. (Ref.) the figures below show the expected photon interactions in Ar/CO2 90/10  and the relative intensity for emitting them,&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;figure &lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;[[File:re_gamma_percent.png | 300px]]&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;figure&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;[[File:ref_xcom_gamma_xsections.png | 300px]]&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt; &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;the figures show that the highest intensity is for the photon of energy of 42 keV, and the rest of the relative intensities for the other energies are below 26 percent. As a result, if U-233phton is&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;the figures show that the highest intensity is for the photon of energy of 42 keV, and the rest of the relative intensities for the other energies are below 26 percent. As a result, if U-233phton is&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
	<entry>
		<id>https://wiki.iac.isu.edu/index.php?title=Gamma_Emission&amp;diff=100088&amp;oldid=prev</id>
		<title>Abdehait: Created page with &quot;=Photoabosrption and Scattering=  U-233 emits gamma particles  that interact with Ar/CO2 gas. U-233 emits gamma particles in the range as it is inside the gaseous chamber, the en…&quot;</title>
		<link rel="alternate" type="text/html" href="https://wiki.iac.isu.edu/index.php?title=Gamma_Emission&amp;diff=100088&amp;oldid=prev"/>
		<updated>2015-04-02T15:09:54Z</updated>

		<summary type="html">&lt;p&gt;Created page with &amp;quot;=Photoabosrption and Scattering=  U-233 emits gamma particles  that interact with Ar/CO2 gas. U-233 emits gamma particles in the range as it is inside the gaseous chamber, the en…&amp;quot;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;=Photoabosrption and Scattering=&lt;br /&gt;
&lt;br /&gt;
U-233 emits gamma particles  that interact with Ar/CO2 gas. U-233 emits gamma particles in the range as it is inside the gaseous chamber, the energy range for those gammas is 42 keV to 807 keV. (Ref.) the figures below show the expected photon interactions in Ar/CO2 90/10  and the relative intensity for emitting them,&lt;br /&gt;
&lt;br /&gt;
figure &lt;br /&gt;
figure&lt;br /&gt;
&lt;br /&gt;
the figures show that the highest intensity is for the photon of energy of 42 keV, and the rest of the relative intensities for the other energies are below 26 percent. As a result, if U-233phton is&lt;/div&gt;</summary>
		<author><name>Abdehait</name></author>
	</entry>
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