<?xml version="1.0"?>
<feed xmlns="http://www.w3.org/2005/Atom" xml:lang="en">
	<id>https://notes.ashstewart.uk/index.php?action=history&amp;feed=atom&amp;title=Year_1_Sem_2%2FLC_Temperature_and_Matter%2FLecture_20</id>
	<title>Year 1 Sem 2/LC Temperature and Matter/Lecture 20 - Revision history</title>
	<link rel="self" type="application/atom+xml" href="https://notes.ashstewart.uk/index.php?action=history&amp;feed=atom&amp;title=Year_1_Sem_2%2FLC_Temperature_and_Matter%2FLecture_20"/>
	<link rel="alternate" type="text/html" href="https://notes.ashstewart.uk/index.php?title=Year_1_Sem_2/LC_Temperature_and_Matter/Lecture_20&amp;action=history"/>
	<updated>2026-10-13T15:09:39Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
	<generator>MediaWiki 1.46.0</generator>
	<entry>
		<id>https://notes.ashstewart.uk/index.php?title=Year_1_Sem_2/LC_Temperature_and_Matter/Lecture_20&amp;diff=420&amp;oldid=prev</id>
		<title>Ash: Import converted Year 1 Semester 2 lecture notes from 443937a7d37850a3c57dfa863f35e80d07f2ccbc</title>
		<link rel="alternate" type="text/html" href="https://notes.ashstewart.uk/index.php?title=Year_1_Sem_2/LC_Temperature_and_Matter/Lecture_20&amp;diff=420&amp;oldid=prev"/>
		<updated>2026-09-11T14:49:20Z</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_20.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 20: Fluid Dynamics&amp;lt;/b&amp;gt;&amp;lt;br&amp;gt;&lt;br /&gt;
Thu 26 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 19|← Previous lecture]] · [[Year 1 Sem 2/LC Temperature and Matter|Module]]&lt;br /&gt;
&lt;br /&gt;
== Fluid Dynamics ==&lt;br /&gt;
&lt;br /&gt;
Say we have no applied force, and the pressure at the liquid surface (for this weirdly shaped container) is &amp;lt;nowiki&amp;gt;$P_0$&amp;lt;/nowiki&amp;gt;. What is the pressure &amp;lt;nowiki&amp;gt;$P$&amp;lt;/nowiki&amp;gt; at some depth &amp;lt;nowiki&amp;gt;$h$&amp;lt;/nowiki&amp;gt;?&lt;br /&gt;
&lt;br /&gt;
[[File:TM-Y1S2-lec20-01.png|thumb|center|280px]]&lt;br /&gt;
&lt;br /&gt;
&amp;lt;div class=&amp;quot;pn-import-equation&amp;quot;&amp;gt;&amp;lt;nowiki&amp;gt;$$P = P_0 + \rho g h$$&amp;lt;/nowiki&amp;gt;&amp;lt;/div&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If, and only if, the fluid has constant density &amp;lt;nowiki&amp;gt;$\rho$&amp;lt;/nowiki&amp;gt;. If &amp;lt;nowiki&amp;gt;$\rho$&amp;lt;/nowiki&amp;gt; varied as a function of height, we’d need to start integrating.&lt;br /&gt;
&lt;br /&gt;
What if we applied a force to the liquid at the top of the spout?&lt;br /&gt;
&lt;br /&gt;
[[File:TM-Y1S2-lec20-02.png|thumb|center|280px]]&lt;br /&gt;
&lt;br /&gt;
Pressure in the liquid will increase, so the applied force to the walls of the container will increase. Pascal’s law says that this increase in pressure is applied to every part of the fluid (and the walls of the enclosure) equally and undiminished.&lt;br /&gt;
&lt;br /&gt;
=== Example: Hydraulic Presses ===&lt;br /&gt;
&lt;br /&gt;
If we apply a force &amp;lt;nowiki&amp;gt;$F_1$&amp;lt;/nowiki&amp;gt; to a liquid in some very small cross-sectional area &amp;lt;nowiki&amp;gt;$a_1$&amp;lt;/nowiki&amp;gt;, then the pressure this results in must be applied to all points in the liquid: &amp;lt;div class=&amp;quot;pn-import-equation&amp;quot;&amp;gt;&amp;lt;nowiki&amp;gt;$$P = \frac{F_1}{a_1}$$&amp;lt;/nowiki&amp;gt;&amp;lt;/div&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Therefore, on the “output” of the press:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;div class=&amp;quot;pn-import-equation&amp;quot;&amp;gt;&amp;lt;nowiki&amp;gt;$$P = \frac{F_2}{a_2}$$&amp;lt;/nowiki&amp;gt;&amp;lt;/div&amp;gt;&lt;br /&gt;
&lt;br /&gt;
If &amp;lt;nowiki&amp;gt;$a_2$&amp;lt;/nowiki&amp;gt; is much larger than &amp;lt;nowiki&amp;gt;$a_1$&amp;lt;/nowiki&amp;gt;, the output force &amp;lt;nowiki&amp;gt;$F_2$&amp;lt;/nowiki&amp;gt; must be proportionally larger than the input force &amp;lt;nowiki&amp;gt;$F_1$&amp;lt;/nowiki&amp;gt; such that: &amp;lt;div class=&amp;quot;pn-import-equation&amp;quot;&amp;gt;&amp;lt;nowiki&amp;gt;$$F_2 = \frac{F_1 a_2}{a_1}$$&amp;lt;/nowiki&amp;gt;&amp;lt;/div&amp;gt;&lt;br /&gt;
&lt;br /&gt;
This effectively lets us magnify forces.&lt;br /&gt;
&lt;br /&gt;
=== Fluid in a Pipe ===&lt;br /&gt;
&lt;br /&gt;
In a steady state (a state with does not change with respect to time) the amount of water that passes a given point must also be constant with respect to time.&lt;br /&gt;
&lt;br /&gt;
[[File:TM-Y1S2-lec20-03.png|thumb|center|600px]]&lt;br /&gt;
&lt;br /&gt;
For this to be a steady state, the amount of liquid passing both points must be the same (otherwise liquid would get stuck and build up). Therefore, we must see: &amp;lt;div class=&amp;quot;pn-import-equation&amp;quot;&amp;gt;&amp;lt;nowiki&amp;gt;$$A_1 v_1 = A_2 v_2$$&amp;lt;/nowiki&amp;gt;&amp;lt;/div&amp;gt;&lt;br /&gt;
&lt;br /&gt;
For &amp;lt;nowiki&amp;gt;$v_1 \neq v_2$&amp;lt;/nowiki&amp;gt;, a force must be applied to the liquid to change velocity. This force comes from the neighbouring fluid molecules.&lt;br /&gt;
&lt;br /&gt;
Previously, we saw: &amp;lt;div class=&amp;quot;pn-import-equation&amp;quot;&amp;gt;&amp;lt;nowiki&amp;gt;$$P = P_0 + \rho g h$$&amp;lt;/nowiki&amp;gt;&amp;lt;/div&amp;gt;&lt;br /&gt;
&lt;br /&gt;
To account for the liquid now being non-stationary and having a velocity, we need to add a term accounting for pressure from kinetic energy: &amp;lt;div class=&amp;quot;pn-import-equation&amp;quot;&amp;gt;&amp;lt;nowiki&amp;gt;$$P + \rho gh + \frac{1}{2} \rho v^2$$&amp;lt;/nowiki&amp;gt;&amp;lt;/div&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Here, &amp;lt;nowiki&amp;gt;$P$&amp;lt;/nowiki&amp;gt; is called static pressure, &amp;lt;nowiki&amp;gt;$\rho g h$&amp;lt;/nowiki&amp;gt; is called hydrostatic pressure and &amp;lt;nowiki&amp;gt;$\frac{1}{2} \rho v^2$&amp;lt;/nowiki&amp;gt; is called dynamic pressure. This full equation becomes useful in a context like this:&lt;br /&gt;
&lt;br /&gt;
[[File:TM-Y1S2-lec20-04.png|thumb|center|280px]]&lt;br /&gt;
&lt;br /&gt;
&amp;lt;div style=&amp;quot;text-align:center&amp;quot;&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;b&amp;gt;End of Module&amp;lt;/b&amp;gt;&lt;br /&gt;
&lt;br /&gt;
&amp;lt;/div&amp;gt;&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
[[Year 1 Sem 2/LC Temperature and Matter/Lecture 19|← Previous lecture]] · [[Year 1 Sem 2/LC Temperature and Matter|Module]]&lt;/div&gt;</summary>
		<author><name>Ash</name></author>
	</entry>
</feed>