﻿<?xml version="1.0"?>
<feed xmlns="http://www.w3.org/2005/Atom" xml:lang="en">
	<id>https://scholarlywiki.org/index.php?action=history&amp;feed=atom&amp;title=Physics%3AQuantum_Fusion_reactions_and_Lawson_criterion</id>
	<title>Physics:Quantum Fusion reactions and Lawson criterion - Revision history</title>
	<link rel="self" type="application/atom+xml" href="https://scholarlywiki.org/index.php?action=history&amp;feed=atom&amp;title=Physics%3AQuantum_Fusion_reactions_and_Lawson_criterion"/>
	<link rel="alternate" type="text/html" href="https://scholarlywiki.org/index.php?title=Physics:Quantum_Fusion_reactions_and_Lawson_criterion&amp;action=history"/>
	<updated>2026-05-14T04:58:09Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
	<generator>MediaWiki 1.43.1</generator>
	<entry>
		<id>https://scholarlywiki.org/index.php?title=Physics:Quantum_Fusion_reactions_and_Lawson_criterion&amp;diff=603&amp;oldid=prev</id>
		<title>imported&gt;WikiHarold: Repair Quantum Collection B backlink template</title>
		<link rel="alternate" type="text/html" href="https://scholarlywiki.org/index.php?title=Physics:Quantum_Fusion_reactions_and_Lawson_criterion&amp;diff=603&amp;oldid=prev"/>
		<updated>2026-05-08T20:01:45Z</updated>

		<summary type="html">&lt;p&gt;Repair Quantum Collection B backlink template&lt;/p&gt;
&lt;table style=&quot;background-color: #fff; color: #202122;&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 20:01, 8 May 2026&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;4&quot; class=&quot;diff-notice&quot; lang=&quot;en&quot;&gt;&lt;div class=&quot;mw-diff-empty&quot;&gt;(No difference)&lt;/div&gt;
&lt;/td&gt;&lt;/tr&gt;
&lt;!-- diff cache key my_wiki:diff:1.41:old-112:rev-603 --&gt;
&lt;/table&gt;</summary>
		<author><name>imported&gt;WikiHarold</name></author>
	</entry>
	<entry>
		<id>https://scholarlywiki.org/index.php?title=Physics:Quantum_Fusion_reactions_and_Lawson_criterion&amp;diff=112&amp;oldid=prev</id>
		<title>imported&gt;WikiHarold: Repair Quantum Collection B backlink template</title>
		<link rel="alternate" type="text/html" href="https://scholarlywiki.org/index.php?title=Physics:Quantum_Fusion_reactions_and_Lawson_criterion&amp;diff=112&amp;oldid=prev"/>
		<updated>2026-05-08T20:01:45Z</updated>

		<summary type="html">&lt;p&gt;Repair Quantum Collection B backlink template&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{Short description|Criterion for ignition in nuclear fusion plasmas}}&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
{{Quantum book backlink|Plasma and fusion physics}}&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;The Lawson criterion&amp;#039;&amp;#039;&amp;#039; is a fundamental condition in [[Physics:Quantum Fusion|nuclear fusion]] physics that determines when a plasma can produce net energy.&amp;lt;ref name=&amp;quot;Lawson1955&amp;quot;&amp;gt;{{cite tech report |last=Lawson |first=J. D. |title=Some criteria for a useful thermonuclear reactor |date=1955 |institution=Atomic Energy Research Establishment}}&amp;lt;/ref&amp;gt;&amp;lt;ref name=&amp;quot;Lawson1957&amp;quot;&amp;gt;{{Cite journal |last=Lawson |first=J. D. |title=Some Criteria for a Power Producing Thermonuclear Reactor |journal=Proceedings of the Physical Society |volume=70 |pages=6–10 |year=1957 |doi=10.1088/0370-1301/70/1/303}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
It compares the rate of energy generated by fusion reactions to the rate of energy losses from the plasma. When fusion heating exceeds losses, the plasma can reach ignition.&amp;lt;ref&amp;gt;{{Cite journal |last1=Abu-Shawareb |first1=H. |title=Lawson Criterion for Ignition Exceeded in an Inertial Fusion Experiment |journal=Physical Review Letters |volume=129 |year=2022 |doi=10.1103/PhysRevLett.129.075001}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
In modern form, the Lawson criterion is expressed through the &amp;#039;&amp;#039;&amp;#039;triple product&amp;#039;&amp;#039;&amp;#039;:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;n T \tau_E&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;n&amp;lt;/math&amp;gt; is particle density, &amp;lt;math&amp;gt;T&amp;lt;/math&amp;gt; temperature, and &amp;lt;math&amp;gt;\tau_E&amp;lt;/math&amp;gt; the energy confinement time.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;div style=&amp;quot;float:right; border:1px solid #ccc; padding:4px; background:#ffffe6; margin:0 0 1em 1em; width:400px;&amp;quot;&amp;gt;&lt;br /&gt;
[[File:Fustion triple-product diagram Horvath.jpg|400px]]&lt;br /&gt;
&amp;lt;div style=&amp;quot;font-size:90%;&amp;quot;&amp;gt;Lawson criterion for various fusion approaches, showing the required triple product for ignition.&amp;lt;/div&amp;gt;&lt;br /&gt;
&amp;lt;/div&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Quantum basis of fusion reactions ==&lt;br /&gt;
&lt;br /&gt;
Fusion reactions depend on quantum tunnelling through the [[Physics:Quantum Fusion#Coulomb barrier|Coulomb barrier]]. The probability that two nuclei fuse is governed by the fusion cross section and its [[Physics:Quantum Fusion#Maxwellian average|Maxwellian average]]:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
f = n_1 n_2 \langle \sigma v \rangle&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The quantity &amp;lt;math&amp;gt;\langle \sigma v \rangle&amp;lt;/math&amp;gt; depends strongly on temperature and is determined by the interplay between the Maxwell–Boltzmann distribution and the quantum tunnelling probability, producing the so-called &amp;#039;&amp;#039;[[Physics:Quantum Fusion#Gamow peak|Gamow peak]]&amp;#039;&amp;#039;.&amp;lt;ref&amp;gt;{{Cite journal |last=Bethe |first=H. A. |last2=Critchfield |first2=C. L. |title=The Formation of Deuterons by Proton Combination |journal=Physical Review |volume=54 |year=1938 |pages=248–254 |doi=10.1103/PhysRev.54.248}}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;{{Cite book |last=Clayton |first=D. D. |title=Principles of Stellar Evolution and Nucleosynthesis |publisher=University of Chicago Press |year=1983}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
This quantum-mechanical tunnelling probability ultimately determines the fusion reactivity and therefore sets the conditions required by the Lawson criterion.&lt;br /&gt;
&lt;br /&gt;
== Energy balance ==&lt;br /&gt;
&lt;br /&gt;
The Lawson criterion is derived from plasma energy balance:&lt;br /&gt;
&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Net power = Fusion − Radiation loss − Conduction loss&amp;#039;&amp;#039;&amp;#039;&lt;br /&gt;
&lt;br /&gt;
Fusion power density:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
P_{fusion} = n_1 n_2 \langle \sigma v \rangle E_{fusion}&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Radiative losses (bremsstrahlung) scale as:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
P_B = 1.4 \cdot 10^{-34} N^2 T^{1/2}&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;N&amp;lt;/math&amp;gt; is particle density.&lt;br /&gt;
&lt;br /&gt;
== Confinement time and nτ formulation ==&lt;br /&gt;
&lt;br /&gt;
The energy confinement time is defined as:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
\tau_E = \frac{W}{P_{loss}}&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
with plasma energy density:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
W = 3 n T&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Using these relations gives the Lawson condition:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
n \tau_E \ge \frac{12T}{E_{ch}\langle\sigma v\rangle}&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
For the deuterium–tritium reaction:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
n \tau_E \gtrsim 1.5 \times 10^{20} \,\mathrm{m^{-3}\,s}&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
at temperatures near:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
T \approx 25\text{–}30\,\mathrm{keV}&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Triple product ==&lt;br /&gt;
&lt;br /&gt;
A more useful figure of merit is the triple product:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
n T \tau_E&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
For D–T fusion:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
n T \tau_E \gtrsim 3 \times 10^{21} \,\mathrm{keV\,s\,m^{-3}}&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Magnetic vs inertial confinement ==&lt;br /&gt;
&lt;br /&gt;
The Lawson criterion applies to both:&lt;br /&gt;
&lt;br /&gt;
=== Magnetic confinement ===&lt;br /&gt;
* low density, long confinement  &lt;br /&gt;
* [[Physics:Quantum Tokamak|tokamaks]]  &lt;br /&gt;
&lt;br /&gt;
=== Inertial confinement ===&lt;br /&gt;
* high density, short confinement  &lt;br /&gt;
&lt;br /&gt;
In inertial systems:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
\rho R \gtrsim 1 \,\mathrm{g/cm^2}&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Non-thermal systems ==&lt;br /&gt;
&lt;br /&gt;
The Lawson criterion assumes thermal equilibrium. Non-thermal systems such as fusors or Polywell devices accelerate particles directly.&lt;br /&gt;
&lt;br /&gt;
In such systems, energy losses remain the primary limitation.&lt;br /&gt;
&lt;br /&gt;
== Physical interpretation ==&lt;br /&gt;
&lt;br /&gt;
The Lawson criterion combines three essential requirements:&lt;br /&gt;
&lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Density&amp;#039;&amp;#039;&amp;#039; → collision frequency  &lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Temperature&amp;#039;&amp;#039;&amp;#039; → tunnelling probability  &lt;br /&gt;
* &amp;#039;&amp;#039;&amp;#039;Confinement time&amp;#039;&amp;#039;&amp;#039; → interaction duration  &lt;br /&gt;
&lt;br /&gt;
Only when all three are sufficiently large does fusion become self-sustaining.&lt;br /&gt;
&lt;br /&gt;
== See also ==&lt;br /&gt;
{{#invoke:PhysicsQC|tocHeadingAndList|Physics:Quantum basics/See also}}&lt;br /&gt;
&lt;br /&gt;
== References ==&lt;br /&gt;
{{reflist|3}}&lt;br /&gt;
&lt;br /&gt;
{{Author|Harold Foppele}}&lt;br /&gt;
&lt;br /&gt;
{{Sourceattribution|Lawson criterion|1}}&lt;/div&gt;</summary>
		<author><name>imported&gt;WikiHarold</name></author>
	</entry>
</feed>