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	<id>https://nemenmanlab.org/~ilya/index.php?action=history&amp;feed=atom&amp;title=Physics_212%2C_2019%3A_Lecture_10</id>
	<title>Physics 212, 2019: Lecture 10 - Revision history</title>
	<link rel="self" type="application/atom+xml" href="https://nemenmanlab.org/~ilya/index.php?action=history&amp;feed=atom&amp;title=Physics_212%2C_2019%3A_Lecture_10"/>
	<link rel="alternate" type="text/html" href="https://nemenmanlab.org/~ilya/index.php?title=Physics_212,_2019:_Lecture_10&amp;action=history"/>
	<updated>2026-04-26T23:47:12Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
	<generator>MediaWiki 1.31.0</generator>
	<entry>
		<id>https://nemenmanlab.org/~ilya/index.php?title=Physics_212,_2019:_Lecture_10&amp;diff=3242&amp;oldid=prev</id>
		<title>Ilya: /* Your work */</title>
		<link rel="alternate" type="text/html" href="https://nemenmanlab.org/~ilya/index.php?title=Physics_212,_2019:_Lecture_10&amp;diff=3242&amp;oldid=prev"/>
		<updated>2019-02-17T18:28:25Z</updated>

		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Your work&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 18:28, 17 February 2019&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-l28&quot; &gt;Line 28:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 28:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;;Problem 2: Use the same extension of the RK2 algorithm to solve the nonlinear pendulum problem. Compare the results to the built-in ODE solver.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;;Problem 2: Use the same extension of the RK2 algorithm to solve the nonlinear pendulum problem. Compare the results to the built-in ODE solver.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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: #222; 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;=&lt;/del&gt;==Scripts for this Lecture&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;=&lt;/del&gt;==&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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;==Scripts for this Lecture==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;::[[media:SystemsOfODEs.txt|Solving Systems of ODEs]] Jupyter notebook&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;::[[media:SystemsOfODEs.txt|Solving Systems of ODEs]] Jupyter notebook&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Ilya</name></author>
		
	</entry>
	<entry>
		<id>https://nemenmanlab.org/~ilya/index.php?title=Physics_212,_2019:_Lecture_10&amp;diff=3240&amp;oldid=prev</id>
		<title>Ilya: /* Nonlinear pendulum */</title>
		<link rel="alternate" type="text/html" href="https://nemenmanlab.org/~ilya/index.php?title=Physics_212,_2019:_Lecture_10&amp;diff=3240&amp;oldid=prev"/>
		<updated>2019-02-17T18:26:41Z</updated>

		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Nonlinear pendulum&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
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				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 18:26, 17 February 2019&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-l13&quot; &gt;Line 13:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 13:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;==Nonlinear pendulum==&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;==Nonlinear pendulum==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;Consider a non-idealized pendulum, which undergoes oscillations with a non-infinitesimal amplitude. Then the restoring torque that it experiences is &amp;lt;math&amp;gt;M=mgl \sim \theta&amp;lt;/math&amp;gt;, where &amp;lt;math&amp;gt;m&amp;lt;/math&amp;gt; is the mass, &amp;lt;math&amp;gt;l&amp;lt;/math&amp;gt; is the pendulum length, and &amp;lt;math&amp;gt;\theta&amp;lt;/math&amp;gt; is the angle its axis forms with the vertical. Newton's equations of motion give for this system &amp;lt;math&amp;gt;\frac{d^2\theta}{dt^2}=gl\sin\theta&amp;lt;/math&amp;gt;. This seems like a single equation, but it is second order in the temporal derivative. It is then equivalent to two coupled first order differential equations &amp;lt;math&amp;gt;\omega =\frac{d\theta}{dt}&amp;lt;/math&amp;gt; and &amp;lt;math&amp;gt;\frac{d\omega}{dt^2}=gl\sin\theta&amp;lt;/math&amp;gt;, where &amp;lt;math&amp;gt;\omega&amp;lt;/math&amp;gt; is the angular velocity&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;Consider a non-idealized pendulum, which undergoes oscillations with a non-infinitesimal amplitude. Then the restoring torque that it experiences is &amp;lt;math&amp;gt;M=mgl \sim \theta&amp;lt;/math&amp;gt;, where &amp;lt;math&amp;gt;m&amp;lt;/math&amp;gt; is the mass, &amp;lt;math&amp;gt;l&amp;lt;/math&amp;gt; is the pendulum length, and &amp;lt;math&amp;gt;\theta&amp;lt;/math&amp;gt; is the angle its axis forms with the vertical. Newton's equations of motion give for this system &amp;lt;math&amp;gt;\frac{d^2\theta}{dt^2}=gl\sin\theta&amp;lt;/math&amp;gt;. This seems like a single equation, but it is second order in the temporal derivative. It is then equivalent to two coupled first order differential equations &amp;lt;math&amp;gt;\omega =\frac{d\theta}{dt}&amp;lt;/math&amp;gt; and &amp;lt;math&amp;gt;\frac{d\omega}{dt^2}=gl\sin\theta&amp;lt;/math&amp;gt;, where &amp;lt;math&amp;gt;\omega&amp;lt;/math&amp;gt; is the angular velocity&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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 style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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 style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;How would one verify the solution, once you write one? For small oscillations, &amp;lt;math&amp;gt;\sin \theta \approx \theta&amp;lt;/math&amp;gt;, and the pendulum becomes harmonic. For it, the period is known -- and one can check if the value of the period is recovered your code.&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;==Solving systems of ODEs==&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;==Solving systems of ODEs==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Ilya</name></author>
		
	</entry>
	<entry>
		<id>https://nemenmanlab.org/~ilya/index.php?title=Physics_212,_2019:_Lecture_10&amp;diff=3239&amp;oldid=prev</id>
		<title>Ilya: /* Predator-prey Lotka-Volterra model */</title>
		<link rel="alternate" type="text/html" href="https://nemenmanlab.org/~ilya/index.php?title=Physics_212,_2019:_Lecture_10&amp;diff=3239&amp;oldid=prev"/>
		<updated>2019-02-17T18:25:40Z</updated>

		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Predator-prey Lotka-Volterra model&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&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;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 18:25, 17 February 2019&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-l8&quot; &gt;Line 8:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 8:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;==Predator-prey Lotka-Volterra model==&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;==Predator-prey Lotka-Volterra model==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;Our second model that we will consider is the predator-prey model of population growth. You can read a lot about such generic systems, including their history, [https://en.wikipedia.org/wiki/Lotka–Volterra_equations here]. Briefly, we consider a prey animal species &amp;lt;math&amp;gt;x&amp;lt;/math&amp;gt;, which grows exponentially, but at the same time it's eaten by the predator species, denoted by &amp;lt;math&amp;gt;y&amp;lt;/math&amp;gt;. The dynamics of the prey is &amp;lt;math&amp;gt;\frac{dx}{dt}=rx - \alpha xy&amp;lt;/math&amp;gt;, where the second term denotes the capture of the prey. Indeed, the more prey animals there are, the easier it is to capture them, and the more predators there are, the more prey they will capture, resulting in the bilinear form &amp;lt;math&amp;gt;\alpha x y&amp;lt;/math&amp;gt;.&amp;#160; At the same time, when the predators eat, they have enough food to procreate -- but usually killing one prey only produces fewer than one predators. Further, predators also die a natural death. As a result, &amp;lt;math&amp;gt;\frac{dy}{dt}= \beta xy - d y&amp;lt;/math&amp;gt;, where &amp;lt;math&amp;gt;\beta&amp;lt;\alpha&amp;lt;/math&amp;gt;. This is an interesting dynamical system that exhibits oscillations -- number of preys goes up, they become abundant, this leads to the growth of the number of predators. Predators start eating prey, and collapse their number; then there's an insufficient number of prey to support the predator population, and the latter collapses as well. The whole cycle restarts with the renewed growth of prey at that point. One can think of more complicated similar systems of equations, but we will leave this to the homework project.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;Our second model that we will consider is the predator-prey model of population growth. You can read a lot about such generic systems, including their history, [https://en.wikipedia.org/wiki/Lotka–Volterra_equations here]. Briefly, we consider a prey animal species &amp;lt;math&amp;gt;x&amp;lt;/math&amp;gt;, which grows exponentially, but at the same time it's eaten by the predator species, denoted by &amp;lt;math&amp;gt;y&amp;lt;/math&amp;gt;. The dynamics of the prey is &amp;lt;math&amp;gt;\frac{dx}{dt}=rx - \alpha xy&amp;lt;/math&amp;gt;, where the second term denotes the capture of the prey. Indeed, the more prey animals there are, the easier it is to capture them, and the more predators there are, the more prey they will capture, resulting in the bilinear form &amp;lt;math&amp;gt;\alpha x y&amp;lt;/math&amp;gt;.&amp;#160; At the same time, when the predators eat, they have enough food to procreate -- but usually killing one prey only produces fewer than one predators. Further, predators also die a natural death. As a result, &amp;lt;math&amp;gt;\frac{dy}{dt}= \beta xy - d y&amp;lt;/math&amp;gt;, where &amp;lt;math&amp;gt;\beta&amp;lt;\alpha&amp;lt;/math&amp;gt;. This is an interesting dynamical system that exhibits oscillations -- number of preys goes up, they become abundant, this leads to the growth of the number of predators. Predators start eating prey, and collapse their number; then there's an insufficient number of prey to support the predator population, and the latter collapses as well. The whole cycle restarts with the renewed growth of prey at that point. One can think of more complicated similar systems of equations, but we will leave this to the homework project.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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 style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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 style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Note that oscillations are always around the same point, and we can calculate it by setting the value of derivative to zero in the dynamical equations, which gives &amp;lt;math&amp;gt;x=d/\beta,\,y=r/\alpha&amp;lt;/math&amp;gt;. One can thus verify our code by first setting the initial conditions exactly at this ''fixed point'', and then varying conditions and seeing that the fluctuations are always around the fixed point.&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;==Nonlinear pendulum==&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;==Nonlinear pendulum==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Ilya</name></author>
		
	</entry>
	<entry>
		<id>https://nemenmanlab.org/~ilya/index.php?title=Physics_212,_2019:_Lecture_10&amp;diff=3238&amp;oldid=prev</id>
		<title>Ilya: /* Solving systems of ODEs */</title>
		<link rel="alternate" type="text/html" href="https://nemenmanlab.org/~ilya/index.php?title=Physics_212,_2019:_Lecture_10&amp;diff=3238&amp;oldid=prev"/>
		<updated>2019-02-17T18:23:20Z</updated>

		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Solving systems of ODEs&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;col class=&quot;diff-content&quot; /&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 18:23, 17 February 2019&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-l17&quot; &gt;Line 17:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 17:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;We will observe the oscillations, and how they can have different amplitudes depending on the initial condition, but always are around the same point.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;We will observe the oscillations, and how they can have different amplitudes depending on the initial condition, but always are around the same point.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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: #222; 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;===Your work&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;=&lt;/del&gt;==&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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;=Additional Python concepts==&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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;We imported the module ''time'' and used it to time the execution of different versions of integrators.&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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;&amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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;==Your work==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;;Problem 1: Write an extension of the RK2 algorithm to a system of coupled ODEs of an arbitrary size and use it to solve the Lotka-Volterra model. Compare the results to the built-in ODE solver. Start with the multidimensional version of the Euler algorithm Jupyter notebook. &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;;Problem 1: Write an extension of the RK2 algorithm to a system of coupled ODEs of an arbitrary size and use it to solve the Lotka-Volterra model. Compare the results to the built-in ODE solver. Start with the multidimensional version of the Euler algorithm Jupyter notebook. &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;;Problem 2: Use the same extension of the RK2 algorithm to solve the nonlinear pendulum problem. Compare the results to the built-in ODE solver.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;;Problem 2: Use the same extension of the RK2 algorithm to solve the nonlinear pendulum problem. Compare the results to the built-in ODE solver.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Ilya</name></author>
		
	</entry>
	<entry>
		<id>https://nemenmanlab.org/~ilya/index.php?title=Physics_212,_2019:_Lecture_10&amp;diff=3237&amp;oldid=prev</id>
		<title>Ilya: /* Your work */</title>
		<link rel="alternate" type="text/html" href="https://nemenmanlab.org/~ilya/index.php?title=Physics_212,_2019:_Lecture_10&amp;diff=3237&amp;oldid=prev"/>
		<updated>2019-02-17T18:22:30Z</updated>

		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Your work&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 18:22, 17 February 2019&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-l18&quot; &gt;Line 18:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 18:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;===Your work===&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;===Your work===&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: #222; 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;;Problem 1: Write an extension of the RK2 algorithm to a system of coupled ODEs of an arbitrary size &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;ands &lt;/del&gt;it to solve the Lotka-Volterra model. Compare the results to the built-in ODE solver. &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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;;Problem 1: Write an extension of the RK2 algorithm to a system of coupled ODEs of an arbitrary size &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;and use &lt;/ins&gt;it to solve the Lotka-Volterra model. Compare the results to the built-in ODE solver&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;. Start with the multidimensional version of the Euler algorithm Jupyter notebook&lt;/ins&gt;. &amp;#160;&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: #222; 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;;Problem 2: Use the same extension of the RK2 algorithm to solve the nonlinear pendulum problem. Compare the results to the built-in ODE solver. &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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;;Problem 2: Use the same extension of the RK2 algorithm to solve the nonlinear pendulum problem. Compare the results to the built-in ODE solver.&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: #222; 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;&amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;===Scripts for this Lecture===&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;===Scripts for this Lecture===&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;::[[media:SystemsOfODEs.txt|Solving Systems of ODEs]] Jupyter notebook&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;::[[media:SystemsOfODEs.txt|Solving Systems of ODEs]] Jupyter notebook&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Ilya</name></author>
		
	</entry>
	<entry>
		<id>https://nemenmanlab.org/~ilya/index.php?title=Physics_212,_2019:_Lecture_10&amp;diff=3236&amp;oldid=prev</id>
		<title>Ilya: /* Solving systems of ODEs */</title>
		<link rel="alternate" type="text/html" href="https://nemenmanlab.org/~ilya/index.php?title=Physics_212,_2019:_Lecture_10&amp;diff=3236&amp;oldid=prev"/>
		<updated>2019-02-17T04:46:23Z</updated>

		<summary type="html">&lt;p&gt;‎&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Solving systems of ODEs&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&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: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 04:46, 17 February 2019&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-l14&quot; &gt;Line 14:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 14:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;==Solving systems of ODEs==&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;==Solving systems of ODEs==&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;How do we solve such coupled, nonlinear dynamical systems numerically? In fact, an almost trivial extension of either the Euler or the RK2 method will work for this goal. In the attached Jupyter notebook, we solve the Lotka-Volterra predator-prey system by the extension of the Euler method to two variables, and we compare the solution to that obtained by the built-in ODE solver.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;How do we solve such coupled, nonlinear dynamical systems numerically? In fact, an almost trivial extension of either the Euler or the RK2 method will work for this goal. In the attached Jupyter notebook, we solve the Lotka-Volterra predator-prey system by the extension of the Euler method to two variables, and we compare the solution to that obtained by the built-in ODE solver.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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 style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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 style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;We will observe the oscillations, and how they can have different amplitudes depending on the initial condition, but always are around the same point.&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;===Your work===&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;===Your work===&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Ilya</name></author>
		
	</entry>
	<entry>
		<id>https://nemenmanlab.org/~ilya/index.php?title=Physics_212,_2019:_Lecture_10&amp;diff=3235&amp;oldid=prev</id>
		<title>Ilya at 04:44, 17 February 2019</title>
		<link rel="alternate" type="text/html" href="https://nemenmanlab.org/~ilya/index.php?title=Physics_212,_2019:_Lecture_10&amp;diff=3235&amp;oldid=prev"/>
		<updated>2019-02-17T04:44:11Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 04:44, 17 February 2019&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-l12&quot; &gt;Line 12:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 12:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;Consider a non-idealized pendulum, which undergoes oscillations with a non-infinitesimal amplitude. Then the restoring torque that it experiences is &amp;lt;math&amp;gt;M=mgl \sim \theta&amp;lt;/math&amp;gt;, where &amp;lt;math&amp;gt;m&amp;lt;/math&amp;gt; is the mass, &amp;lt;math&amp;gt;l&amp;lt;/math&amp;gt; is the pendulum length, and &amp;lt;math&amp;gt;\theta&amp;lt;/math&amp;gt; is the angle its axis forms with the vertical. Newton's equations of motion give for this system &amp;lt;math&amp;gt;\frac{d^2\theta}{dt^2}=gl\sin\theta&amp;lt;/math&amp;gt;. This seems like a single equation, but it is second order in the temporal derivative. It is then equivalent to two coupled first order differential equations &amp;lt;math&amp;gt;\omega =\frac{d\theta}{dt}&amp;lt;/math&amp;gt; and &amp;lt;math&amp;gt;\frac{d\omega}{dt^2}=gl\sin\theta&amp;lt;/math&amp;gt;, where &amp;lt;math&amp;gt;\omega&amp;lt;/math&amp;gt; is the angular velocity&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;Consider a non-idealized pendulum, which undergoes oscillations with a non-infinitesimal amplitude. Then the restoring torque that it experiences is &amp;lt;math&amp;gt;M=mgl \sim \theta&amp;lt;/math&amp;gt;, where &amp;lt;math&amp;gt;m&amp;lt;/math&amp;gt; is the mass, &amp;lt;math&amp;gt;l&amp;lt;/math&amp;gt; is the pendulum length, and &amp;lt;math&amp;gt;\theta&amp;lt;/math&amp;gt; is the angle its axis forms with the vertical. Newton's equations of motion give for this system &amp;lt;math&amp;gt;\frac{d^2\theta}{dt^2}=gl\sin\theta&amp;lt;/math&amp;gt;. This seems like a single equation, but it is second order in the temporal derivative. It is then equivalent to two coupled first order differential equations &amp;lt;math&amp;gt;\omega =\frac{d\theta}{dt}&amp;lt;/math&amp;gt; and &amp;lt;math&amp;gt;\frac{d\omega}{dt^2}=gl\sin\theta&amp;lt;/math&amp;gt;, where &amp;lt;math&amp;gt;\omega&amp;lt;/math&amp;gt; is the angular velocity&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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: #222; 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;Runge-Kutta 2 integration of &lt;/del&gt;systems of ODEs==&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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;Solving &lt;/ins&gt;systems of ODEs==&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: #222; 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;How do we solve such coupled, nonlinear dynamical systems numerically?&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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;How do we solve such coupled, nonlinear dynamical systems numerically? &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;In fact, an almost trivial extension of either the Euler or the RK2 method will work for this goal. In the attached Jupyter notebook, we solve the Lotka-Volterra predator-prey system by the extension of the Euler method to two variables, and we compare the solution to that obtained by the built-in ODE solver.&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;===Your work===&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;===Your work===&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: #222; 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;;Problem 1: &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;Use &lt;/del&gt;a &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;different differential equation from those provided &lt;/del&gt;to &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;show that Runge&lt;/del&gt;-&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;Kutta &lt;/del&gt;2 &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;has error &amp;lt;math&amp;gt;O(dt^2)&amp;lt;/math&amp;gt;, and &lt;/del&gt;the &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;scaling &lt;/del&gt;of the &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;error is not a scaling due &lt;/del&gt;to the &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;equation being solved, but largely due &lt;/del&gt;to the &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;methods used to solve it. Do this &lt;/del&gt;in &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;a Jupyter notebook&lt;/del&gt;.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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;;Problem 1: &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Write an extension of the RK2 algorithm to &lt;/ins&gt;a &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;system of coupled ODEs of an arbitrary size ands it &lt;/ins&gt;to &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;solve the Lotka-Volterra model. Compare the results to the built&lt;/ins&gt;-&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;in ODE solver. &lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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;;Problem &lt;/ins&gt;2&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;: Use &lt;/ins&gt;the &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;same extension &lt;/ins&gt;of the &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;RK2 algorithm &lt;/ins&gt;to &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;solve the nonlinear pendulum problem. Compare &lt;/ins&gt;the &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;results &lt;/ins&gt;to the &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;built-&lt;/ins&gt;in &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;ODE solver&lt;/ins&gt;. &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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;&amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;===Scripts for this Lecture===&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;===Scripts for this Lecture===&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: #222; 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;::[[media:&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;growthfunctions2019&lt;/del&gt;.txt | &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;GrowthFunctions&lt;/del&gt;]] &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;-- module defining different growth functions.&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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;::[[media:&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;SystemsOfODEs&lt;/ins&gt;.txt|&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Solving Systems of ODEs&lt;/ins&gt;]] &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Jupyter &lt;/ins&gt;notebook&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: #222; 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;::[[media:Integrators2019.txt | Integrators]] -- module defining different integrators (Euler and Runge-Kutta, which we will use during the next lecture).&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #222; 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;::[[media:moduleTwo2019.txt | Module 2]] -- catch-all scripts I used during the class.&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #222; 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;::[[media:IntegrateODE.txt | Module 2 as a &lt;/del&gt;notebook&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;]] -- integration as a notebook.&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Ilya</name></author>
		
	</entry>
	<entry>
		<id>https://nemenmanlab.org/~ilya/index.php?title=Physics_212,_2019:_Lecture_10&amp;diff=3234&amp;oldid=prev</id>
		<title>Ilya at 04:39, 17 February 2019</title>
		<link rel="alternate" type="text/html" href="https://nemenmanlab.org/~ilya/index.php?title=Physics_212,_2019:_Lecture_10&amp;diff=3234&amp;oldid=prev"/>
		<updated>2019-02-17T04:39:00Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
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				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 04:39, 17 February 2019&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-l1&quot; &gt;Line 1:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 1:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;{{PHYS212-2019}}&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;{{PHYS212-2019}}&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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: #222; 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;In this lecture, we will introduce models that involved coupled, nonlinear ordinary differential equations, as well as methods for solving them.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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;To date, we only considered simple dynamics, which has a single dynamical variable, whose first temporal derivative is determined by the variable itself. &lt;/ins&gt;In this lecture, we will introduce models that involved coupled, nonlinear ordinary differential equations, as well as methods for solving them.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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 colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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 style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;==Growth with carrying capacity==&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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 first model we will consider is the Malthusian growth with carrying capacity -- where a population grows nearly exponentially fast, before it reaches the maximum population size that can be supported by the environment, &amp;lt;math&amp;gt;dn/dt = r n(n_0-n)&amp;lt;/math&amp;gt;, where &amp;lt;math&amp;gt;n_0&amp;lt;/math&amp;gt; is known as the carrying capacity. During the previous lecture and the lab, you were supposed to solve the corresponding ODE numerically -- and you will have noticed how the growth starts quickly, and then saturates. &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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 first model we will consider is the Malthusian growth with carrying capacity -- where a population grows nearly exponentially fast, before it reaches the maximum population size that can be supported by the environment, &amp;lt;math&amp;gt;dn/dt = r n(n_0-n)&amp;lt;/math&amp;gt;, where &amp;lt;math&amp;gt;n_0&amp;lt;/math&amp;gt; is known as the carrying capacity. During the previous lecture and the lab, you were supposed to solve the corresponding ODE numerically -- and you will have noticed how the growth starts quickly, and then saturates. &amp;#160;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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: #222; 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;Our second model that we will consider is the predator-prey model of population growth. You can read a lot about such generic systems, including their history, [https://en.wikipedia.org/wiki/Lotka–Volterra_equations here]. Briefly, we consider a prey animal species &amp;lt;math&amp;gt;x&amp;lt;/math&amp;gt;, which grows exponentially, but at the same time it's eaten by the predator species, denoted by &amp;lt;math&amp;gt;y&amp;lt;/math&amp;gt;. The dynamics of the prey is &amp;lt;math&amp;gt;\frac{dx}{dt}=rx - \alpha xy&amp;lt;/math&amp;gt;, where the second term denotes the capture of the prey. Indeed, the more prey animals there are, the easier it is to capture them, and the more predators there are, the more prey they will capture, resulting in the bilinear form &amp;lt;math&amp;gt;\alpha x y&amp;lt;/math&amp;gt;.&amp;#160; At the same time, when the predators eat, they have enough food to procreate -- but usually killing one prey only produces fewer than one predators. Further, predators also die a natural death. As a result, &amp;lt;math&amp;gt;\frac{dy}{dt}= \beta xy - d y&amp;lt;/math&amp;gt;, where &amp;lt;math&amp;gt;\beta&amp;lt;\alpha&amp;lt;/math&amp;gt;. This is an interesting dynamical system that exhibits oscillations -- number of preys goes up, they become abundant, this leads to the growth of the number of predators. Predators start eating prey, and collapse their number; then there's an insufficient number of prey to support the predator population, and the latter collapses as well. The whole cycle restarts with the renewed growth of prey at that point.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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;==Predator-prey Lotka-Volterra model==&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: #222; 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; &lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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;Our second model that we will consider is the predator-prey model of population growth. You can read a lot about such generic systems, including their history, [https://en.wikipedia.org/wiki/Lotka–Volterra_equations here]. Briefly, we consider a prey animal species &amp;lt;math&amp;gt;x&amp;lt;/math&amp;gt;, which grows exponentially, but at the same time it's eaten by the predator species, denoted by &amp;lt;math&amp;gt;y&amp;lt;/math&amp;gt;. The dynamics of the prey is &amp;lt;math&amp;gt;\frac{dx}{dt}=rx - \alpha xy&amp;lt;/math&amp;gt;, where the second term denotes the capture of the prey. Indeed, the more prey animals there are, the easier it is to capture them, and the more predators there are, the more prey they will capture, resulting in the bilinear form &amp;lt;math&amp;gt;\alpha x y&amp;lt;/math&amp;gt;.&amp;#160; At the same time, when the predators eat, they have enough food to procreate -- but usually killing one prey only produces fewer than one predators. Further, predators also die a natural death. As a result, &amp;lt;math&amp;gt;\frac{dy}{dt}= \beta xy - d y&amp;lt;/math&amp;gt;, where &amp;lt;math&amp;gt;\beta&amp;lt;\alpha&amp;lt;/math&amp;gt;. This is an interesting dynamical system that exhibits oscillations -- number of preys goes up, they become abundant, this leads to the growth of the number of predators. Predators start eating prey, and collapse their number; then there's an insufficient number of prey to support the predator population, and the latter collapses as well. The whole cycle restarts with the renewed growth of prey at that point. &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;One can think of more complicated similar systems of equations, but we will leave this to the homework project.&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: #222; 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;==Runge-Kutta 2 integration==&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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 colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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 style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;==Nonlinear pendulum==&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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 style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;Consider a non-idealized pendulum, which undergoes oscillations with a non-infinitesimal amplitude. Then the restoring torque that it experiences is &amp;lt;math&amp;gt;M=mgl \sim \theta&amp;lt;/math&amp;gt;, where &amp;lt;math&amp;gt;m&amp;lt;/math&amp;gt; is the mass, &amp;lt;math&amp;gt;l&amp;lt;/math&amp;gt; is the pendulum length, and &amp;lt;math&amp;gt;\theta&amp;lt;/math&amp;gt; is the angle its axis forms with the vertical. Newton's equations of motion give for this system &amp;lt;math&amp;gt;\frac{d^2\theta}{dt^2}=gl\sin\theta&amp;lt;/math&amp;gt;. This seems like a single equation, but it is second order in the temporal derivative. It is then equivalent to two coupled first order differential equations &amp;lt;math&amp;gt;\omega =\frac{d\theta}{dt}&amp;lt;/math&amp;gt; and &amp;lt;math&amp;gt;\frac{d\omega}{dt^2}=gl\sin\theta&amp;lt;/math&amp;gt;, where &amp;lt;math&amp;gt;\omega&amp;lt;/math&amp;gt; is the angular velocity&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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 style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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 style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;==Runge-Kutta 2 integration of systems of ODEs==&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt;&amp;#160;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; 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 style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;How do we solve such coupled, nonlinear dynamical systems numerically?&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;===Your work===&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;&amp;#160;&lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; 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;===Your work===&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Ilya</name></author>
		
	</entry>
	<entry>
		<id>https://nemenmanlab.org/~ilya/index.php?title=Physics_212,_2019:_Lecture_10&amp;diff=3233&amp;oldid=prev</id>
		<title>Ilya: Created page with &quot;{{PHYS212-2019}}  In this lecture, we will introduce models that involved coupled, nonlinear ordinary differential equations, as well as methods for solving them.  The first m...&quot;</title>
		<link rel="alternate" type="text/html" href="https://nemenmanlab.org/~ilya/index.php?title=Physics_212,_2019:_Lecture_10&amp;diff=3233&amp;oldid=prev"/>
		<updated>2019-02-17T04:31:05Z</updated>

		<summary type="html">&lt;p&gt;Created page with &amp;quot;{{PHYS212-2019}}  In this lecture, we will introduce models that involved coupled, nonlinear ordinary differential equations, as well as methods for solving them.  The first m...&amp;quot;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{PHYS212-2019}}&lt;br /&gt;
&lt;br /&gt;
In this lecture, we will introduce models that involved coupled, nonlinear ordinary differential equations, as well as methods for solving them.&lt;br /&gt;
&lt;br /&gt;
The first model we will consider is the Malthusian growth with carrying capacity -- where a population grows nearly exponentially fast, before it reaches the maximum population size that can be supported by the environment, &amp;lt;math&amp;gt;dn/dt = r n(n_0-n)&amp;lt;/math&amp;gt;, where &amp;lt;math&amp;gt;n_0&amp;lt;/math&amp;gt; is known as the carrying capacity. During the previous lecture and the lab, you were supposed to solve the corresponding ODE numerically -- and you will have noticed how the growth starts quickly, and then saturates. &lt;br /&gt;
&lt;br /&gt;
Our second model that we will consider is the predator-prey model of population growth. You can read a lot about such generic systems, including their history, [https://en.wikipedia.org/wiki/Lotka–Volterra_equations here]. Briefly, we consider a prey animal species &amp;lt;math&amp;gt;x&amp;lt;/math&amp;gt;, which grows exponentially, but at the same time it's eaten by the predator species, denoted by &amp;lt;math&amp;gt;y&amp;lt;/math&amp;gt;. The dynamics of the prey is &amp;lt;math&amp;gt;\frac{dx}{dt}=rx - \alpha xy&amp;lt;/math&amp;gt;, where the second term denotes the capture of the prey. Indeed, the more prey animals there are, the easier it is to capture them, and the more predators there are, the more prey they will capture, resulting in the bilinear form &amp;lt;math&amp;gt;\alpha x y&amp;lt;/math&amp;gt;.  At the same time, when the predators eat, they have enough food to procreate -- but usually killing one prey only produces fewer than one predators. Further, predators also die a natural death. As a result, &amp;lt;math&amp;gt;\frac{dy}{dt}= \beta xy - d y&amp;lt;/math&amp;gt;, where &amp;lt;math&amp;gt;\beta&amp;lt;\alpha&amp;lt;/math&amp;gt;. This is an interesting dynamical system that exhibits oscillations -- number of preys goes up, they become abundant, this leads to the growth of the number of predators. Predators start eating prey, and collapse their number; then there's an insufficient number of prey to support the predator population, and the latter collapses as well. The whole cycle restarts with the renewed growth of prey at that point.&lt;br /&gt;
 &lt;br /&gt;
==Runge-Kutta 2 integration==&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
===Your work===&lt;br /&gt;
;Problem 1: Use a different differential equation from those provided to show that Runge-Kutta 2 has error &amp;lt;math&amp;gt;O(dt^2)&amp;lt;/math&amp;gt;, and the scaling of the error is not a scaling due to the equation being solved, but largely due to the methods used to solve it. Do this in a Jupyter notebook.&lt;br /&gt;
&lt;br /&gt;
===Scripts for this Lecture===&lt;br /&gt;
::[[media:growthfunctions2019.txt | GrowthFunctions]] -- module defining different growth functions.&lt;br /&gt;
::[[media:Integrators2019.txt | Integrators]] -- module defining different integrators (Euler and Runge-Kutta, which we will use during the next lecture).&lt;br /&gt;
::[[media:moduleTwo2019.txt | Module 2]] -- catch-all scripts I used during the class.&lt;br /&gt;
::[[media:IntegrateODE.txt | Module 2 as a notebook]] -- integration as a notebook.&lt;/div&gt;</summary>
		<author><name>Ilya</name></author>
		
	</entry>
</feed>