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	<title>Year 1 Sem 2/LC Temperature and Matter/Lecture 14 - Revision history</title>
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		<title>Ash: Import converted Year 1 Semester 2 lecture notes from 443937a7d37850a3c57dfa863f35e80d07f2ccbc</title>
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		<updated>2026-09-11T14:49:18Z</updated>

		<summary type="html">&lt;p&gt;Import converted Year 1 Semester 2 lecture notes from 443937a7d37850a3c57dfa863f35e80d07f2ccbc&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;&amp;lt;!-- Converted from ashstewart7/university at 443937a7d37850a3c57dfa863f35e80d07f2ccbc; Temperature and Matter/lec_14.tex. --&amp;gt;&lt;br /&gt;
&amp;lt;div class=&amp;quot;pn-lecture-meta&amp;quot;&amp;gt;&lt;br /&gt;
&amp;lt;b&amp;gt;Lecture 14: Statistical Physics I: Introduction&amp;lt;/b&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
Thu 05 Mar 2026 13:00&lt;br /&gt;
&amp;lt;/div&amp;gt;&lt;br /&gt;
&lt;br /&gt;
[[Year 1 Sem 2/LC Temperature and Matter/Lecture 13|← Previous lecture]] · [[Year 1 Sem 2/LC Temperature and Matter|Module]] · [[Year 1 Sem 2/LC Temperature and Matter/Lecture 15|Next lecture →]]&lt;br /&gt;
&lt;br /&gt;
== Stefan-Boltzmann Law ==&lt;br /&gt;
&lt;br /&gt;
We can integrate across the whole spectrum to work out total energy emitted per unit time: &amp;lt;div class=&amp;quot;pn-import-equation&amp;quot;&amp;gt;&amp;lt;nowiki&amp;gt;$$\dot{Q} = \epsilon \sigma A T^4$$&amp;lt;/nowiki&amp;gt;&amp;lt;/div&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Where &amp;lt;nowiki&amp;gt;$\sigma = 5.67 \times 10^{-8} \mathrm{W m^{-2} K^{-1}}$&amp;lt;/nowiki&amp;gt; is the Stefan-Boltzmann constant, &amp;lt;nowiki&amp;gt;$\epsilon$&amp;lt;/nowiki&amp;gt; is the emissivity, &amp;lt;nowiki&amp;gt;$A$&amp;lt;/nowiki&amp;gt; is the surface area of the radiating body and &amp;lt;nowiki&amp;gt;$T$&amp;lt;/nowiki&amp;gt; is the temperature.&lt;br /&gt;
&lt;br /&gt;
== Kinetic Theory of Gases ==&lt;br /&gt;
&lt;br /&gt;
We’ve now finished the module on temperature and move into statistical physics. We start wth a kinetic theory of the motion of gas molecules. Gas molecules move “randomly” (effectively, it’s not computationally viable to determine what’s actually going on), with vastly different velocities and positions.&lt;br /&gt;
&lt;br /&gt;
We would love to describe a gas using the individual molecules that make it up, but that’s really difficult to do for &amp;lt;nowiki&amp;gt;$\sim 10^{23}$&amp;lt;/nowiki&amp;gt; molecules so it’s not viable and we have to use statistical physics to describe it.&lt;br /&gt;
&lt;br /&gt;
We’ve previously touched upon the Maxwell-Boltzmann distribution to describe the velocities of particles as a statistical distribution wrt temperature:&lt;br /&gt;
&lt;br /&gt;
[[File:TM-Y1S2-lec07-1.png|thumb|center|800px]]&lt;br /&gt;
&lt;br /&gt;
These statistical approximations improve as we increase the number of particles, and for very large numbers they become good approximations. We can in statistical physics have a probability &amp;lt;nowiki&amp;gt;$&amp;gt;1$&amp;lt;/nowiki&amp;gt;. This seems mathematically strange, but we interpret it to mean that (if the probability represents the probability of an event occurring in a measurement), the event will take place multiple times. We still cannot have any probabilities &amp;lt;nowiki&amp;gt;$&amp;lt;0$&amp;lt;/nowiki&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
The rest of the lecture then turned into a fun tangent on statistics which isn’t examinable and needs no notes.&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
[[Year 1 Sem 2/LC Temperature and Matter/Lecture 13|← Previous lecture]] · [[Year 1 Sem 2/LC Temperature and Matter|Module]] · [[Year 1 Sem 2/LC Temperature and Matter/Lecture 15|Next lecture →]]&lt;/div&gt;</summary>
		<author><name>Ash</name></author>
	</entry>
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