<?xml version="1.0" encoding="UTF-8"?>
<rss xmlns:itunes="http://www.itunes.com/dtds/podcast-1.0.dtd" version="2.0">
  <channel>
    <title>Thermal and Statistical Physics</title>
    <link>http://odeo.com/channels/21682-Thermal-and-Statistical-Physics</link>
    <itunes:explicit>no</itunes:explicit>
    <description>&lt;A HREF="http://www.physics.purdue.edu/academic_programs/courses/phys416/"&gt;Physics 416&lt;/A&gt;&lt;BR&gt;
Thermal and Statistical Physics &lt;BR&gt;
Purdue University &lt;BR&gt; &lt;BR&gt;
Textbook:  Thermal Physics by Kittel and Kroemer &lt;BR&gt;&lt;BR&gt;
Lectures follow the text fairly closely, so if you're joining us from 
&lt;A HREF="http://www.itunes.com"&gt;iTunes&lt;/A&gt;, you might enjoy having a copy handy.</description>
    <itunes:summary>Physics 416
Thermal and Statistical Physics 
Purdue University  
Textbook:  Thermal Physics by Kittel and Kroemer 
Lectures follow the text fairly closely, so if you're joining us from 
iTunes, you might enjoy having a copy handy.</itunes:summary>
    <itunes:subtitle>Thermal and Statistical Physics Purdue University Phys 416</itunes:subtitle>
    <language>en</language>
    <ttl>40</ttl>
    <itunes:image href="http://www.physics.purdue.edu/~erica/416/Phys416Podcast.jpg"/>
    <image url="http://www.physics.purdue.edu/~erica/416/Phys416Podcast.jpg" link="http://odeo.com/channels/21682-Thermal-and-Statistical-Physics" title="Thermal and Statistical Physics"/>
    <pubDate>Mon, 10 Sep 2007 00:02:43 -0700</pubDate>
    <lastBuildDate>Mon, 10 Sep 2007 00:02:43 -0700</lastBuildDate>
    <category>Formal Education</category>
    <itunes:category text="Education">
      <itunes:category text="Higher Education"/>
    </itunes:category>
    <item>
      <title>Lecture 4: Partition Function and Thermodynamic Identity</title>
      <link>http://odeo.com/episodes/12803363-Lecture-4-Partition-Function-and-Thermodynamic-Identity</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-09-10,12803363</guid>
      <pubDate>Mon, 10 Sep 2007 00:02:43 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://feeds.feedburner.com/~r/Physics416/~5/119471676/PHYS416_2005_08_31_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 5: Free Energy and Maxwell Relations</title>
      <link>http://odeo.com/episodes/12803383-Lecture-5-Free-Energy-and-Maxwell-Relations</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-09-10,12803383</guid>
      <pubDate>Mon, 10 Sep 2007 00:02:17 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://feeds.feedburner.com/~r/Physics416/~5/119471675/PHYS416_2005_09_07_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 6:  Ideal Gas Law, Planck Blackbody Radiation</title>
      <link>http://odeo.com/episodes/12803393-Lecture-6-Ideal-Gas-Law-Planck-Blackbody-Radiation</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-09-10,12803393</guid>
      <pubDate>Mon, 10 Sep 2007 00:01:16 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://feeds.feedburner.com/~r/Physics416/~5/119471674/PHYS416_2005_09_12_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 2: Multiplicity Function</title>
      <link>http://odeo.com/episodes/16615823-Lecture-2-Multiplicity-Function</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-09-09,16615823</guid>
      <pubDate>Sun, 09 Sep 2007 23:20:36 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://feeds.feedburner.com/~r/Physics416/~5/154361716/PHYS416_2005_08_24_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 4: Partition Function and Thermodynamic Identity</title>
      <link>http://odeo.com/episodes/23311949-Lecture-4-Partition-Function-and-Thermodynamic-Identity</link>
      <description>Boltzmann Factor, Partition Function and how to calculate everything else from it.Live near lakes because they have a high heat capacity. Energy and Heat Capacity of a two state system, Definition of a reversible process, Definition of pressure, The Thermodynamic Identity, Thermodynamically Conjugate variables.Digressions: Is toasting bread a reversible process? Do microwaves get water hotter than other heating methods? Lecture 4 Audio</description>
      <itunes:subtitle>Boltzmann Factor, Partition Function and how to calculate everything else from it.Live near lakes because they have a high heat capacity. Energy and Heat Capacity of a two state system, Definition of a reversible process, Definition of pressure, The Thermodynamic Identity, Thermodynamically Conjugate variables.Digressions: Is toasting bread a reversible process? Do microwaves get water hotter than other heating methods? Lecture 4 Audio</itunes:subtitle>
      <itunes:summary>Boltzmann Factor, Partition Function and how to calculate everything else from it.Live near lakes because they have a high heat capacity. Energy and Heat Capacity of a two state system, Definition of a reversible process, Definition of pressure, The Thermodynamic Identity, Thermodynamically Conjugate variables.Digressions: Is toasting bread a reversible process? Do microwaves get water hotter than other heating methods? Lecture 4 Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-09-09,23311949</guid>
      <pubDate>Sun, 09 Sep 2007 17:02:43 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://web.ics.purdue.edu/~erica/416/mp3/PHYS416_2005_08_31_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 4: Partition Function and Thermodynamic Identity</title>
      <link>http://odeo.com/episodes/24181119-Lecture-4-Partition-Function-and-Thermodynamic-Identity</link>
      <description>Boltzmann Factor, Partition Function and how to calculate everything else from it.Live near lakes because they have a high heat capacity. Energy and Heat Capacity of a two state system, Definition of a reversible process, Definition of pressure, The Thermodynamic Identity, Thermodynamically Conjugate variables.Digressions: Is toasting bread a reversible process? Do microwaves get water hotter than other heating methods? Lecture 4 Audio</description>
      <itunes:subtitle>Boltzmann Factor, Partition Function and how to calculate everything else from it.Live near lakes because they have a high heat capacity. Energy and Heat Capacity of a two state system, Definition of a reversible process, Definition of pressure, The Thermodynamic Identity, Thermodynamically Conjugate variables.Digressions: Is toasting bread a reversible process? Do microwaves get water hotter than other heating methods? Lecture 4 Audio</itunes:subtitle>
      <itunes:summary>Boltzmann Factor, Partition Function and how to calculate everything else from it.Live near lakes because they have a high heat capacity. Energy and Heat Capacity of a two state system, Definition of a reversible process, Definition of pressure, The Thermodynamic Identity, Thermodynamically Conjugate variables.Digressions: Is toasting bread a reversible process? Do microwaves get water hotter than other heating methods? Lecture 4 Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-09-09,24181119</guid>
      <pubDate>Sun, 09 Sep 2007 17:02:43 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://web.ics.purdue.edu/~erica/416/mp3/PHYS416_2005_08_31_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 5: Free Energy and Maxwell Relations</title>
      <link>http://odeo.com/episodes/23311944-Lecture-5-Free-Energy-and-Maxwell-Relations</link>
      <description>Helmholtz Free Energy is the right energy to use when temperature and volume are used as control variables. Free Energy and the Partition Function. Maxwell Relations -- you can derive them all. Legendre Transforms. Ideal Gas. Quantum Concentration.Why some slow processes are still irreversible, as with toast and frogs. Lecture Audio</description>
      <itunes:subtitle>Helmholtz Free Energy is the right energy to use when temperature and volume are used as control variables. Free Energy and the Partition Function. Maxwell Relations -- you can derive them all. Legendre Transforms. Ideal Gas. Quantum Concentration.Why some slow processes are still irreversible, as with toast and frogs. Lecture Audio</itunes:subtitle>
      <itunes:summary>Helmholtz Free Energy is the right energy to use when temperature and volume are used as control variables. Free Energy and the Partition Function. Maxwell Relations -- you can derive them all. Legendre Transforms. Ideal Gas. Quantum Concentration.Why some slow processes are still irreversible, as with toast and frogs. Lecture Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-09-09,23311944</guid>
      <pubDate>Sun, 09 Sep 2007 17:02:17 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://web.ics.purdue.edu/~erica/416/mp3/PHYS416_2005_09_07_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 5: Free Energy and Maxwell Relations</title>
      <link>http://odeo.com/episodes/24181118-Lecture-5-Free-Energy-and-Maxwell-Relations</link>
      <description>Helmholtz Free Energy is the right energy to use when temperature and volume are used as control variables. Free Energy and the Partition Function. Maxwell Relations -- you can derive them all. Legendre Transforms. Ideal Gas. Quantum Concentration.Why some slow processes are still irreversible, as with toast and frogs. Lecture Audio</description>
      <itunes:subtitle>Helmholtz Free Energy is the right energy to use when temperature and volume are used as control variables. Free Energy and the Partition Function. Maxwell Relations -- you can derive them all. Legendre Transforms. Ideal Gas. Quantum Concentration.Why some slow processes are still irreversible, as with toast and frogs. Lecture Audio</itunes:subtitle>
      <itunes:summary>Helmholtz Free Energy is the right energy to use when temperature and volume are used as control variables. Free Energy and the Partition Function. Maxwell Relations -- you can derive them all. Legendre Transforms. Ideal Gas. Quantum Concentration.Why some slow processes are still irreversible, as with toast and frogs. Lecture Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-09-09,24181118</guid>
      <pubDate>Sun, 09 Sep 2007 17:02:17 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://feedproxy.google.com/~r/Physics416/~5/QDV7vBs3mBU/PHYS416_2005_09_07_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 6:  Ideal Gas Law, Planck Blackbody Radiation</title>
      <link>http://odeo.com/episodes/23311943-Lecture-6-Ideal-Gas-Law-Planck-Blackbody-Radiation</link>
      <description>Deriving the ideal gas law. Equipartition Theorem. Entropy of Mixing.Hot things glow -- or how night vision goggles work (Planck blackbody radiation). Analyzing star spectra. Class discussions: Mixing 2 colors of Kool-Aid, and how to make heavy Kool-Aid out of deuterated water. Why deuterated water can extend the snow skiing season, but is unfortunately toxic. Lecture Audio</description>
      <itunes:subtitle>Deriving the ideal gas law. Equipartition Theorem. Entropy of Mixing.Hot things glow -- or how night vision goggles work (Planck blackbody radiation). Analyzing star spectra. Class discussions: Mixing 2 colors of Kool-Aid, and how to make heavy Kool-Aid out of deuterated water. Why deuterated water can extend the snow skiing season, but is unfortunately toxic. Lecture Audio</itunes:subtitle>
      <itunes:summary>Deriving the ideal gas law. Equipartition Theorem. Entropy of Mixing.Hot things glow -- or how night vision goggles work (Planck blackbody radiation). Analyzing star spectra. Class discussions: Mixing 2 colors of Kool-Aid, and how to make heavy Kool-Aid out of deuterated water. Why deuterated water can extend the snow skiing season, but is unfortunately toxic. Lecture Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-09-09,23311943</guid>
      <pubDate>Sun, 09 Sep 2007 17:01:16 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://web.ics.purdue.edu/~erica/416/mp3/PHYS416_2005_09_12_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 6:  Ideal Gas Law, Planck Blackbody Radiation</title>
      <link>http://odeo.com/episodes/24181117-Lecture-6-Ideal-Gas-Law-Planck-Blackbody-Radiation</link>
      <description>Deriving the ideal gas law. Equipartition Theorem. Entropy of Mixing.Hot things glow -- or how night vision goggles work (Planck blackbody radiation). Analyzing star spectra. Class discussions: Mixing 2 colors of Kool-Aid, and how to make heavy Kool-Aid out of deuterated water. Why deuterated water can extend the snow skiing season, but is unfortunately toxic. Lecture Audio</description>
      <itunes:subtitle>Deriving the ideal gas law. Equipartition Theorem. Entropy of Mixing.Hot things glow -- or how night vision goggles work (Planck blackbody radiation). Analyzing star spectra. Class discussions: Mixing 2 colors of Kool-Aid, and how to make heavy Kool-Aid out of deuterated water. Why deuterated water can extend the snow skiing season, but is unfortunately toxic. Lecture Audio</itunes:subtitle>
      <itunes:summary>Deriving the ideal gas law. Equipartition Theorem. Entropy of Mixing.Hot things glow -- or how night vision goggles work (Planck blackbody radiation). Analyzing star spectra. Class discussions: Mixing 2 colors of Kool-Aid, and how to make heavy Kool-Aid out of deuterated water. Why deuterated water can extend the snow skiing season, but is unfortunately toxic. Lecture Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-09-09,24181117</guid>
      <pubDate>Sun, 09 Sep 2007 17:01:16 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://feedproxy.google.com/~r/Physics416/~5/bRWgvTwoUjY/PHYS416_2005_09_12_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 2: Multiplicity Function</title>
      <link>http://odeo.com/episodes/23311957-Lecture-2-Multiplicity-Function</link>
      <description>Why is the most probable configuration important? Multiplicity Function is a gaussian in the two-state system.Weighted averages. Introduction to partition function. Lecture 2 Audio</description>
      <itunes:subtitle>Why is the most probable configuration important? Multiplicity Function is a gaussian in the two-state system.Weighted averages. Introduction to partition function. Lecture 2 Audio</itunes:subtitle>
      <itunes:summary>Why is the most probable configuration important? Multiplicity Function is a gaussian in the two-state system.Weighted averages. Introduction to partition function. Lecture 2 Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-09-09,23311957</guid>
      <pubDate>Sun, 09 Sep 2007 16:20:36 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://web.ics.purdue.edu/~erica/416/mp3/PHYS416_2005_08_24_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 2: Multiplicity Function</title>
      <link>http://odeo.com/episodes/24181121-Lecture-2-Multiplicity-Function</link>
      <description>Why is the most probable configuration important? Multiplicity Function is a gaussian in the two-state system.Weighted averages. Introduction to partition function. Lecture 2 Audio</description>
      <itunes:subtitle>Why is the most probable configuration important? Multiplicity Function is a gaussian in the two-state system.Weighted averages. Introduction to partition function. Lecture 2 Audio</itunes:subtitle>
      <itunes:summary>Why is the most probable configuration important? Multiplicity Function is a gaussian in the two-state system.Weighted averages. Introduction to partition function. Lecture 2 Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-09-09,24181121</guid>
      <pubDate>Sun, 09 Sep 2007 16:20:36 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://feedproxy.google.com/~r/Physics416/~5/ChKeMXGu16w/PHYS416_2005_08_24_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Final Review 2</title>
      <link>http://odeo.com/episodes/16615983-Final-Review-2</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,16615983</guid>
      <pubDate>Tue, 21 Aug 2007 15:33:16 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://feeds.feedburner.com/~r/Physics416/~5/154352890/FinalReview2.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Final Review 1</title>
      <link>http://odeo.com/episodes/16615963-Final-Review-1</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,16615963</guid>
      <pubDate>Tue, 21 Aug 2007 15:32:49 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://feeds.feedburner.com/~r/Physics416/~5/154352891/FinalReview1.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 24:  Fluctuation-Dissipation Theorem</title>
      <link>http://odeo.com/episodes/16615933-Lecture-24-Fluctuation-Dissipation-Theorem</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,16615933</guid>
      <pubDate>Tue, 21 Aug 2007 15:15:28 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://feeds.feedburner.com/~r/Physics416/~5/154352892/Lecture24.Fluctuation.Dissipation.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture23: Brownian Motion and Diffusion</title>
      <link>http://odeo.com/episodes/16615913-Lecture23-Brownian-Motion-and-Diffusion</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,16615913</guid>
      <pubDate>Tue, 21 Aug 2007 15:14:41 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://feeds.feedburner.com/~r/Physics416/~5/146544507/Lecture23.Brownian.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 22: Nucleation in First Order (Abrupt) Phase Transitions</title>
      <link>http://odeo.com/episodes/16615903-Lecture-22-Nucleation-in-First-Order-Abrupt-Phase-Transitions</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,16615903</guid>
      <pubDate>Tue, 21 Aug 2007 15:14:09 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://feeds.feedburner.com/~r/Physics416/~5/146544508/Lecture22.Nucleation.Snowflakes.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 21:  Alloys, Mixing, and Phase Separation</title>
      <link>http://odeo.com/episodes/16615893-Lecture-21-Alloys-Mixing-and-Phase-Separation</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,16615893</guid>
      <pubDate>Tue, 21 Aug 2007 15:12:38 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://feeds.feedburner.com/~r/Physics416/~5/146544509/Lecture21.Mixing.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 20:  Landau Theory of Phase Transitions; Oil, Water, and Alloys</title>
      <link>http://odeo.com/episodes/16615883-Lecture-20-Landau-Theory-of-Phase-Transitions-Oil-Water-and-Alloys</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,16615883</guid>
      <pubDate>Tue, 21 Aug 2007 15:11:54 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://feeds.feedburner.com/~r/Physics416/~5/146544510/Lecture20.LandauTheory.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 19:  Symmetries, Order Parameters, and the Failure of Reductionism</title>
      <link>http://odeo.com/episodes/16615873-Lecture-19-Symmetries-Order-Parameters-and-the-Failure-of-Reductionism</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,16615873</guid>
      <pubDate>Tue, 21 Aug 2007 15:10:59 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://feeds.feedburner.com/~r/Physics416/~5/146537827/Lecture19.Symmetry.Reductionism.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 18:  Van Der Waals and Geckos</title>
      <link>http://odeo.com/episodes/16615863-Lecture-18-Van-Der-Waals-and-Geckos</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,16615863</guid>
      <pubDate>Tue, 21 Aug 2007 15:09:12 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://feeds.feedburner.com/~r/Physics416/~5/146537833/Lecture18.VdW.Geckos.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Final Review 2</title>
      <link>http://odeo.com/episodes/23311881-Final-Review-2</link>
      <description>This is a final review for the last 1/4 of the course. This is a very short lecture, because we had a field trip to go see the prestigious Bagwell Lecture given by Purdue's very own Prof. Albert Overhauser of the world-famous Overhauser Effect. Lecture Audio</description>
      <itunes:subtitle>This is a final review for the last 1/4 of the course. This is a very short lecture, because we had a field trip to go see the prestigious Bagwell Lecture given by Purdue's very own Prof. Albert Overhauser of the world-famous Overhauser Effect. Lecture Audio</itunes:subtitle>
      <itunes:summary>This is a final review for the last 1/4 of the course. This is a very short lecture, because we had a field trip to go see the prestigious Bagwell Lecture given by Purdue's very own Prof. Albert Overhauser of the world-famous Overhauser Effect. Lecture Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,23311881</guid>
      <pubDate>Tue, 21 Aug 2007 08:33:16 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://web.ics.purdue.edu/~erica/416/mp3/FinalReview2.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Final Review 2</title>
      <link>http://odeo.com/episodes/24181096-Final-Review-2</link>
      <description>This is a final review for the last 1/4 of the course. This is a very short lecture, because we had a field trip to go see the prestigious Bagwell Lecture given by Purdue's very own Prof. Albert Overhauser of the world-famous Overhauser Effect. Lecture Audio</description>
      <itunes:subtitle>This is a final review for the last 1/4 of the course. This is a very short lecture, because we had a field trip to go see the prestigious Bagwell Lecture given by Purdue's very own Prof. Albert Overhauser of the world-famous Overhauser Effect. Lecture Audio</itunes:subtitle>
      <itunes:summary>This is a final review for the last 1/4 of the course. This is a very short lecture, because we had a field trip to go see the prestigious Bagwell Lecture given by Purdue's very own Prof. Albert Overhauser of the world-famous Overhauser Effect. Lecture Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,24181096</guid>
      <pubDate>Tue, 21 Aug 2007 08:33:16 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://web.ics.purdue.edu/~erica/416/mp3/FinalReview2.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Final Review 1</title>
      <link>http://odeo.com/episodes/23311882-Final-Review-1</link>
      <description>This is a final review for the first 3/4 of the course. Lecture Audio</description>
      <itunes:subtitle>This is a final review for the first 3/4 of the course. Lecture Audio</itunes:subtitle>
      <itunes:summary>This is a final review for the first 3/4 of the course. Lecture Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,23311882</guid>
      <pubDate>Tue, 21 Aug 2007 08:32:49 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://web.ics.purdue.edu/~erica/416/mp3/FinalReview1.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Final Review 1</title>
      <link>http://odeo.com/episodes/24181097-Final-Review-1</link>
      <description>This is a final review for the first 3/4 of the course. Lecture Audio</description>
      <itunes:subtitle>This is a final review for the first 3/4 of the course. Lecture Audio</itunes:subtitle>
      <itunes:summary>This is a final review for the first 3/4 of the course. Lecture Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,24181097</guid>
      <pubDate>Tue, 21 Aug 2007 08:32:49 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://web.ics.purdue.edu/~erica/416/mp3/FinalReview1.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 24:  Fluctuation-Dissipation Theorem</title>
      <link>http://odeo.com/episodes/23311886-Lecture-24-Fluctuation-Dissipation-Theorem</link>
      <description>We finish two more examples of the Fluctuation-Dissipation Theorem. This is a theorem that pops up everywhere! It means that the very same microscopic processes responsible for establishing thermal equilibrium are the same microscopic processes that cause resistance in metals, drag in fluids, and other types of dissipation. We discuss thermal noise in resistors (also known as Johnson noise or Nyquist noise), and demonstrate the fluctuation-dissipation theorem in this system. We also derive the magnetic susceptibility of a collection of free spins in a magnetic field. It turns out (due to the fluctuation dissipation theorem, of course) that the higher the amount of thermal fluctuations in the system at thermal equilibrium, the easier it is to magnetize the system. Lecture Audio</description>
      <itunes:subtitle>We finish two more examples of the Fluctuation-Dissipation Theorem. This is a theorem that pops up everywhere! It means that the very same microscopic processes responsible for establishing thermal equilibrium are the same microscopic processes that cause resistance in metals, drag in fluids, and other types of dissipation. We discuss thermal noise in resistors (also known as Johnson noise or Nyquist noise), and demonstrate the fluctuation-dissipation theorem in this system. We also derive the magnetic susceptibility of a collection of free spins in a magnetic field. It turns out (due to the fluctuation dissipation theorem, of course) that the higher the amount of thermal fluctuations in the system at thermal equilibrium, the easier it is to magnetize the system. Lecture Audio</itunes:subtitle>
      <itunes:summary>We finish two more examples of the Fluctuation-Dissipation Theorem. This is a theorem that pops up everywhere! It means that the very same microscopic processes responsible for establishing thermal equilibrium are the same microscopic processes that cause resistance in metals, drag in fluids, and other types of dissipation. We discuss thermal noise in resistors (also known as Johnson noise or Nyquist noise), and demonstrate the fluctuation-dissipation theorem in this system. We also derive the magnetic susceptibility of a collection of free spins in a magnetic field. It turns out (due to the fluctuation dissipation theorem, of course) that the higher the amount of thermal fluctuations in the system at thermal equilibrium, the easier it is to magnetize the system. Lecture Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,23311886</guid>
      <pubDate>Tue, 21 Aug 2007 08:15:28 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://web.ics.purdue.edu/~erica/416/mp3/Lecture24.Fluctuation.Dissipation.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 24:  Fluctuation-Dissipation Theorem</title>
      <link>http://odeo.com/episodes/24181098-Lecture-24-Fluctuation-Dissipation-Theorem</link>
      <description>We finish two more examples of the Fluctuation-Dissipation Theorem. This is a theorem that pops up everywhere! It means that the very same microscopic processes responsible for establishing thermal equilibrium are the same microscopic processes that cause resistance in metals, drag in fluids, and other types of dissipation. We discuss thermal noise in resistors (also known as Johnson noise or Nyquist noise), and demonstrate the fluctuation-dissipation theorem in this system. We also derive the magnetic susceptibility of a collection of free spins in a magnetic field. It turns out (due to the fluctuation dissipation theorem, of course) that the higher the amount of thermal fluctuations in the system at thermal equilibrium, the easier it is to magnetize the system. Lecture Audio</description>
      <itunes:subtitle>We finish two more examples of the Fluctuation-Dissipation Theorem. This is a theorem that pops up everywhere! It means that the very same microscopic processes responsible for establishing thermal equilibrium are the same microscopic processes that cause resistance in metals, drag in fluids, and other types of dissipation. We discuss thermal noise in resistors (also known as Johnson noise or Nyquist noise), and demonstrate the fluctuation-dissipation theorem in this system. We also derive the magnetic susceptibility of a collection of free spins in a magnetic field. It turns out (due to the fluctuation dissipation theorem, of course) that the higher the amount of thermal fluctuations in the system at thermal equilibrium, the easier it is to magnetize the system. Lecture Audio</itunes:subtitle>
      <itunes:summary>We finish two more examples of the Fluctuation-Dissipation Theorem. This is a theorem that pops up everywhere! It means that the very same microscopic processes responsible for establishing thermal equilibrium are the same microscopic processes that cause resistance in metals, drag in fluids, and other types of dissipation. We discuss thermal noise in resistors (also known as Johnson noise or Nyquist noise), and demonstrate the fluctuation-dissipation theorem in this system. We also derive the magnetic susceptibility of a collection of free spins in a magnetic field. It turns out (due to the fluctuation dissipation theorem, of course) that the higher the amount of thermal fluctuations in the system at thermal equilibrium, the easier it is to magnetize the system. Lecture Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,24181098</guid>
      <pubDate>Tue, 21 Aug 2007 08:15:28 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://web.ics.purdue.edu/~erica/416/mp3/Lecture24.Fluctuation.Dissipation.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture23: Brownian Motion and Diffusion</title>
      <link>http://odeo.com/episodes/23311891-Lecture23-Brownian-Motion-and-Diffusion</link>
      <description>Brownian motion was discovered by a botanist named Brown, when he looked at water under a microscope, and observed pollen grains "jiggling" about in it. Einstein eventually explained it as due to the random collisions the pollen grain experienced from the water molecules. We compare the pollen grain to a drunk person walking home, and calculate how far the pollen grain can get by this type of diffusion. We also introduce the fluctuation-dissipation theorem, a far-reaching principle in advanced statistical mechanics that says that the microscopic thermal fluctuations in a system are the same microscopic processes that are responsible for things like drag, viscosity, and electrical resistance. (Why is that so cool? Because it means you can predict nonequilibrium properties -- those in the presence of an applied field like voltage -- to equilibrium properties like thermal fluctuations.) We also derive Fick's law of diffusion -- particles diffuse away from high concentrations. Go figure...</description>
      <itunes:subtitle>Brownian motion was discovered by a botanist named Brown, when he looked at water under a microscope, and observed pollen grains "jiggling" about in it. Einstein eventually explained it as due to the random collisions the pollen grain experienced from the water molecules. We compare the pollen grain to a drunk person walking home, and calculate how far the pollen grain can get by this type of diffusion. We also introduce the fluctuation-dissipation theorem, a far-reaching principle in advanced statistical mechanics that says that the microscopic thermal fluctuations in a system are the same microscopic processes that are responsible for things like drag, viscosity, and electrical resistance. (Why is that so cool? Because it means you can predict nonequilibrium properties -- those in the presence of an applied field like voltage -- to equilibrium properties like thermal fluctuations.) We also derive Fick's law of diffusion -- particles diffuse away from high concentrations. Go figure! Shown in class:Nice movies on the web about colloid particles in milk executing Brownian motion.There's a great applet on Brownian motion to play with here. Lecture Audio</itunes:subtitle>
      <itunes:summary>Brownian motion was discovered by a botanist named Brown, when he looked at water under a microscope, and observed pollen grains "jiggling" about in it. Einstein eventually explained it as due to the random collisions the pollen grain experienced from the water molecules. We compare the pollen grain to a drunk person walking home, and calculate how far the pollen grain can get by this type of diffusion. We also introduce the fluctuation-dissipation theorem, a far-reaching principle in advanced statistical mechanics that says that the microscopic thermal fluctuations in a system are the same microscopic processes that are responsible for things like drag, viscosity, and electrical resistance. (Why is that so cool? Because it means you can predict nonequilibrium properties -- those in the presence of an applied field like voltage -- to equilibrium properties like thermal fluctuations.) We also derive Fick's law of diffusion -- particles diffuse away from high concentrations. Go figure! Shown in class:Nice movies on the web about colloid particles in milk executing Brownian motion.There's a great applet on Brownian motion to play with here. Lecture Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,23311891</guid>
      <pubDate>Tue, 21 Aug 2007 08:14:41 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://feeds.feedburner.com/~r/Physics416/~5/146544507/Lecture23.Brownian.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture23: Brownian Motion and Diffusion</title>
      <link>http://odeo.com/episodes/24181099-Lecture23-Brownian-Motion-and-Diffusion</link>
      <description>Brownian motion was discovered by a botanist named Brown, when he looked at water under a microscope, and observed pollen grains "jiggling" about in it. Einstein eventually explained it as due to the random collisions the pollen grain experienced from the water molecules. We compare the pollen grain to a drunk person walking home, and calculate how far the pollen grain can get by this type of diffusion. We also introduce the fluctuation-dissipation theorem, a far-reaching principle in advanced statistical mechanics that says that the microscopic thermal fluctuations in a system are the same microscopic processes that are responsible for things like drag, viscosity, and electrical resistance. (Why is that so cool? Because it means you can predict nonequilibrium properties -- those in the presence of an applied field like voltage -- to equilibrium properties like thermal fluctuations.) We also derive Fick's law of diffusion -- particles diffuse away from high concentrations. Go figure...</description>
      <itunes:subtitle>Brownian motion was discovered by a botanist named Brown, when he looked at water under a microscope, and observed pollen grains "jiggling" about in it. Einstein eventually explained it as due to the random collisions the pollen grain experienced from the water molecules. We compare the pollen grain to a drunk person walking home, and calculate how far the pollen grain can get by this type of diffusion. We also introduce the fluctuation-dissipation theorem, a far-reaching principle in advanced statistical mechanics that says that the microscopic thermal fluctuations in a system are the same microscopic processes that are responsible for things like drag, viscosity, and electrical resistance. (Why is that so cool? Because it means you can predict nonequilibrium properties -- those in the presence of an applied field like voltage -- to equilibrium properties like thermal fluctuations.) We also derive Fick's law of diffusion -- particles diffuse away from high concentrations. Go figure! Shown in class:Nice movies on the web about colloid particles in milk executing Brownian motion.There's a great applet on Brownian motion to play with here. Lecture Audio</itunes:subtitle>
      <itunes:summary>Brownian motion was discovered by a botanist named Brown, when he looked at water under a microscope, and observed pollen grains "jiggling" about in it. Einstein eventually explained it as due to the random collisions the pollen grain experienced from the water molecules. We compare the pollen grain to a drunk person walking home, and calculate how far the pollen grain can get by this type of diffusion. We also introduce the fluctuation-dissipation theorem, a far-reaching principle in advanced statistical mechanics that says that the microscopic thermal fluctuations in a system are the same microscopic processes that are responsible for things like drag, viscosity, and electrical resistance. (Why is that so cool? Because it means you can predict nonequilibrium properties -- those in the presence of an applied field like voltage -- to equilibrium properties like thermal fluctuations.) We also derive Fick's law of diffusion -- particles diffuse away from high concentrations. Go figure! Shown in class:Nice movies on the web about colloid particles in milk executing Brownian motion.There's a great applet on Brownian motion to play with here. Lecture Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,24181099</guid>
      <pubDate>Tue, 21 Aug 2007 08:14:41 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://web.ics.purdue.edu/~erica/416/mp3/Lecture23.Brownian.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 22: Nucleation in First Order (Abrupt) Phase Transitions</title>
      <link>http://odeo.com/episodes/23311894-Lecture-22-Nucleation-in-First-Order-Abrupt-Phase-Transitions</link>
      <description>Supercooling Demonstration (thanks to special guest Prof. Ken Ritchie): Put filtered water in a plastic bottle in your freezer for, say, 4 hours. Now, carefully remove it from the freezer, and shake the bottle vigorously. We did this, and saw ice crystals begin to slowly form in the water, because the liquid water was supercooled, and the ice phase was technically more stable. (Some crystals even resembled snowflakes, and grew larger as they floated to the top.) You may have to experiment with how long you leave the bottle in the freezer. Too short a time, and nothing happens. If you freeze the bottle longer, a vigorous shake will turn the whole bottle white as crystals form everywhere. Too long, and it will all freeze in the freezer. Do try this at home! Today we discuss nucleation in first order (abrupt) phase transitions. The ice crystals in our supercooled bottle of water formed through nucleation -- tiny ice crystals grew larger over time. The arctic cod is a supercooled fish, ...</description>
      <itunes:subtitle>Supercooling Demonstration (thanks to special guest Prof. Ken Ritchie): Put filtered water in a plastic bottle in your freezer for, say, 4 hours. Now, carefully remove it from the freezer, and shake the bottle vigorously. We did this, and saw ice crystals begin to slowly form in the water, because the liquid water was supercooled, and the ice phase was technically more stable. (Some crystals even resembled snowflakes, and grew larger as they floated to the top.) You may have to experiment with how long you leave the bottle in the freezer. Too short a time, and nothing happens. If you freeze the bottle longer, a vigorous shake will turn the whole bottle white as crystals form everywhere. Too long, and it will all freeze in the freezer. Do try this at home! Today we discuss nucleation in first order (abrupt) phase transitions. The ice crystals in our supercooled bottle of water formed through nucleation -- tiny ice crystals grew larger over time. The arctic cod is a supercooled fish, living in water too salty to freeze even though it's at -1.9 degrees Celsius! The reason the fish doesn't freeze solid is due to antifreeze glycoproteins, which inhibit the growth of nucleated ice crystals. We calculate the energy barriers to nucleation at the liquid-gas transiton, and find that a nucleated liquid bubble in the gas phase must be large enough before it will turn the whole substance liquid. If it's too small, the bubble is unstable and converts back into gas. We also discuss: Slushy ice -- where is that on our phase diagram? Surface tension and faceting in crystals. Plant-eating bacteria which secrete enzymes that encourage ice nucleation on plants. And quite a bit about how snowflakes form. Much of today is from Jim Sethna's statistical mechanics book, and the part about snowflakes and ice formation is from research at my alma mater, Caltech, as presented at www.snowcrystals.com. Lecture Audio</itunes:subtitle>
      <itunes:summary>Supercooling Demonstration (thanks to special guest Prof. Ken Ritchie): Put filtered water in a plastic bottle in your freezer for, say, 4 hours. Now, carefully remove it from the freezer, and shake the bottle vigorously. We did this, and saw ice crystals begin to slowly form in the water, because the liquid water was supercooled, and the ice phase was technically more stable. (Some crystals even resembled snowflakes, and grew larger as they floated to the top.) You may have to experiment with how long you leave the bottle in the freezer. Too short a time, and nothing happens. If you freeze the bottle longer, a vigorous shake will turn the whole bottle white as crystals form everywhere. Too long, and it will all freeze in the freezer. Do try this at home! Today we discuss nucleation in first order (abrupt) phase transitions. The ice crystals in our supercooled bottle of water formed through nucleation -- tiny ice crystals grew larger over time. The arctic cod is a supercooled fish, living in water too salty to freeze even though it's at -1.9 degrees Celsius! The reason the fish doesn't freeze solid is due to antifreeze glycoproteins, which inhibit the growth of nucleated ice crystals. We calculate the energy barriers to nucleation at the liquid-gas transiton, and find that a nucleated liquid bubble in the gas phase must be large enough before it will turn the whole substance liquid. If it's too small, the bubble is unstable and converts back into gas. We also discuss: Slushy ice -- where is that on our phase diagram? Surface tension and faceting in crystals. Plant-eating bacteria which secrete enzymes that encourage ice nucleation on plants. And quite a bit about how snowflakes form. Much of today is from Jim Sethna's statistical mechanics book, and the part about snowflakes and ice formation is from research at my alma mater, Caltech, as presented at www.snowcrystals.com. Lecture Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,23311894</guid>
      <pubDate>Tue, 21 Aug 2007 08:14:09 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://feeds.feedburner.com/~r/Physics416/~5/146544508/Lecture22.Nucleation.Snowflakes.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 22: Nucleation in First Order (Abrupt) Phase Transitions</title>
      <link>http://odeo.com/episodes/24181100-Lecture-22-Nucleation-in-First-Order-Abrupt-Phase-Transitions</link>
      <description>Supercooling Demonstration (thanks to special guest Prof. Ken Ritchie): Put filtered water in a plastic bottle in your freezer for, say, 4 hours. Now, carefully remove it from the freezer, and shake the bottle vigorously. We did this, and saw ice crystals begin to slowly form in the water, because the liquid water was supercooled, and the ice phase was technically more stable. (Some crystals even resembled snowflakes, and grew larger as they floated to the top.) You may have to experiment with how long you leave the bottle in the freezer. Too short a time, and nothing happens. If you freeze the bottle longer, a vigorous shake will turn the whole bottle white as crystals form everywhere. Too long, and it will all freeze in the freezer. Do try this at home! Today we discuss nucleation in first order (abrupt) phase transitions. The ice crystals in our supercooled bottle of water formed through nucleation -- tiny ice crystals grew larger over time. The arctic cod is a supercooled fish, ...</description>
      <itunes:subtitle>Supercooling Demonstration (thanks to special guest Prof. Ken Ritchie): Put filtered water in a plastic bottle in your freezer for, say, 4 hours. Now, carefully remove it from the freezer, and shake the bottle vigorously. We did this, and saw ice crystals begin to slowly form in the water, because the liquid water was supercooled, and the ice phase was technically more stable. (Some crystals even resembled snowflakes, and grew larger as they floated to the top.) You may have to experiment with how long you leave the bottle in the freezer. Too short a time, and nothing happens. If you freeze the bottle longer, a vigorous shake will turn the whole bottle white as crystals form everywhere. Too long, and it will all freeze in the freezer. Do try this at home! Today we discuss nucleation in first order (abrupt) phase transitions. The ice crystals in our supercooled bottle of water formed through nucleation -- tiny ice crystals grew larger over time. The arctic cod is a supercooled fish, living in water too salty to freeze even though it's at -1.9 degrees Celsius! The reason the fish doesn't freeze solid is due to antifreeze glycoproteins, which inhibit the growth of nucleated ice crystals. We calculate the energy barriers to nucleation at the liquid-gas transiton, and find that a nucleated liquid bubble in the gas phase must be large enough before it will turn the whole substance liquid. If it's too small, the bubble is unstable and converts back into gas. We also discuss: Slushy ice -- where is that on our phase diagram? Surface tension and faceting in crystals. Plant-eating bacteria which secrete enzymes that encourage ice nucleation on plants. And quite a bit about how snowflakes form. Much of today is from Jim Sethna's statistical mechanics book, and the part about snowflakes and ice formation is from research at my alma mater, Caltech, as presented at www.snowcrystals.com. Lecture Audio</itunes:subtitle>
      <itunes:summary>Supercooling Demonstration (thanks to special guest Prof. Ken Ritchie): Put filtered water in a plastic bottle in your freezer for, say, 4 hours. Now, carefully remove it from the freezer, and shake the bottle vigorously. We did this, and saw ice crystals begin to slowly form in the water, because the liquid water was supercooled, and the ice phase was technically more stable. (Some crystals even resembled snowflakes, and grew larger as they floated to the top.) You may have to experiment with how long you leave the bottle in the freezer. Too short a time, and nothing happens. If you freeze the bottle longer, a vigorous shake will turn the whole bottle white as crystals form everywhere. Too long, and it will all freeze in the freezer. Do try this at home! Today we discuss nucleation in first order (abrupt) phase transitions. The ice crystals in our supercooled bottle of water formed through nucleation -- tiny ice crystals grew larger over time. The arctic cod is a supercooled fish, living in water too salty to freeze even though it's at -1.9 degrees Celsius! The reason the fish doesn't freeze solid is due to antifreeze glycoproteins, which inhibit the growth of nucleated ice crystals. We calculate the energy barriers to nucleation at the liquid-gas transiton, and find that a nucleated liquid bubble in the gas phase must be large enough before it will turn the whole substance liquid. If it's too small, the bubble is unstable and converts back into gas. We also discuss: Slushy ice -- where is that on our phase diagram? Surface tension and faceting in crystals. Plant-eating bacteria which secrete enzymes that encourage ice nucleation on plants. And quite a bit about how snowflakes form. Much of today is from Jim Sethna's statistical mechanics book, and the part about snowflakes and ice formation is from research at my alma mater, Caltech, as presented at www.snowcrystals.com. Lecture Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,24181100</guid>
      <pubDate>Tue, 21 Aug 2007 08:14:09 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://feedproxy.google.com/~r/Physics416/~5/IMxysnYDpTw/Lecture22.Nucleation.Snowflakes.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 21:  Alloys, Mixing, and Phase Separation</title>
      <link>http://odeo.com/episodes/23311897-Lecture-21-Alloys-Mixing-and-Phase-Separation</link>
      <description>Oil and water -- they don't mix. Or do they? Due to the entropy of mixing, any tiny amount of impurity is highly favored entropically. This means that in general, you can get a small amount of a substance to mix into another. But take that too far, and they no longer mix, but "phase separate" into 2 different concentrations. We discuss this from the following perspectives: energy, entropy, and free energy. Examples: binary alloy with interactions, and a mixture of He3 (fermions) and He4 (bosons).Class discussion: Can you get oil and water to mix if you heat them in a pressure cooker? Lecture Audio</description>
      <itunes:subtitle>Oil and water -- they don't mix. Or do they? Due to the entropy of mixing, any tiny amount of impurity is highly favored entropically. This means that in general, you can get a small amount of a substance to mix into another. But take that too far, and they no longer mix, but "phase separate" into 2 different concentrations. We discuss this from the following perspectives: energy, entropy, and free energy. Examples: binary alloy with interactions, and a mixture of He3 (fermions) and He4 (bosons).Class discussion: Can you get oil and water to mix if you heat them in a pressure cooker? Lecture Audio</itunes:subtitle>
      <itunes:summary>Oil and water -- they don't mix. Or do they? Due to the entropy of mixing, any tiny amount of impurity is highly favored entropically. This means that in general, you can get a small amount of a substance to mix into another. But take that too far, and they no longer mix, but "phase separate" into 2 different concentrations. We discuss this from the following perspectives: energy, entropy, and free energy. Examples: binary alloy with interactions, and a mixture of He3 (fermions) and He4 (bosons).Class discussion: Can you get oil and water to mix if you heat them in a pressure cooker? Lecture Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,23311897</guid>
      <pubDate>Tue, 21 Aug 2007 08:12:38 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://feeds.feedburner.com/~r/Physics416/~5/146544509/Lecture21.Mixing.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 21:  Alloys, Mixing, and Phase Separation</title>
      <link>http://odeo.com/episodes/24181101-Lecture-21-Alloys-Mixing-and-Phase-Separation</link>
      <description>Oil and water -- they don't mix. Or do they? Due to the entropy of mixing, any tiny amount of impurity is highly favored entropically. This means that in general, you can get a small amount of a substance to mix into another. But take that too far, and they no longer mix, but "phase separate" into 2 different concentrations. We discuss this from the following perspectives: energy, entropy, and free energy. Examples: binary alloy with interactions, and a mixture of He3 (fermions) and He4 (bosons).Class discussion: Can you get oil and water to mix if you heat them in a pressure cooker? Lecture Audio</description>
      <itunes:subtitle>Oil and water -- they don't mix. Or do they? Due to the entropy of mixing, any tiny amount of impurity is highly favored entropically. This means that in general, you can get a small amount of a substance to mix into another. But take that too far, and they no longer mix, but "phase separate" into 2 different concentrations. We discuss this from the following perspectives: energy, entropy, and free energy. Examples: binary alloy with interactions, and a mixture of He3 (fermions) and He4 (bosons).Class discussion: Can you get oil and water to mix if you heat them in a pressure cooker? Lecture Audio</itunes:subtitle>
      <itunes:summary>Oil and water -- they don't mix. Or do they? Due to the entropy of mixing, any tiny amount of impurity is highly favored entropically. This means that in general, you can get a small amount of a substance to mix into another. But take that too far, and they no longer mix, but "phase separate" into 2 different concentrations. We discuss this from the following perspectives: energy, entropy, and free energy. Examples: binary alloy with interactions, and a mixture of He3 (fermions) and He4 (bosons).Class discussion: Can you get oil and water to mix if you heat them in a pressure cooker? Lecture Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,24181101</guid>
      <pubDate>Tue, 21 Aug 2007 08:12:38 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://feedproxy.google.com/~r/Physics416/~5/r9N-f9Ibnfs/Lecture21.Mixing.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 20:  Landau Theory of Phase Transitions; Oil, Water, and Alloys</title>
      <link>http://odeo.com/episodes/23311900-Lecture-20-Landau-Theory-of-Phase-Transitions-Oil-Water-and-Alloys</link>
      <description>Now that we know what order parameters are (see last lecture), we'll use the order parameter of a phase to construct the Landau free energy. The Landau free energy depends on the order parameter, and retains all the symmetries of the physical system. It's amazing how much you can get from symmetry, and we're able to see how it is that a ferromagnet can have what's called a continuous phase transition. That is, starting from zero temperature with a saturated magnetization, upon raising the temperature, the magnetization slowly decreases, until it has smoothly (continuously, in fact) gone to zero. This makes it a continous transition. We also show what a first order (discontinuous) phase transition would look like. First order phase transitions can exhibit supercooling and superheating. We also discuss the physics of alloys like bronze, and under what conditions two different materials will mix and form a binary mixture, and under what conditions there will be phase separation into 2 ...</description>
      <itunes:subtitle>Now that we know what order parameters are (see last lecture), we'll use the order parameter of a phase to construct the Landau free energy. The Landau free energy depends on the order parameter, and retains all the symmetries of the physical system. It's amazing how much you can get from symmetry, and we're able to see how it is that a ferromagnet can have what's called a continuous phase transition. That is, starting from zero temperature with a saturated magnetization, upon raising the temperature, the magnetization slowly decreases, until it has smoothly (continuously, in fact) gone to zero. This makes it a continous transition. We also show what a first order (discontinuous) phase transition would look like. First order phase transitions can exhibit supercooling and superheating. We also discuss the physics of alloys like bronze, and under what conditions two different materials will mix and form a binary mixture, and under what conditions there will be phase separation into 2 distinct concentrations, as happens with oil and water. A small concentration of impurities is always favorable according to entropy, and will always mix. But larger concentrations may "fall apart" and phase separate. Class discussions: Lots about supercooling and superheating. More about nonequilibrium behavior like window glass. Lecture Audio</itunes:subtitle>
      <itunes:summary>Now that we know what order parameters are (see last lecture), we'll use the order parameter of a phase to construct the Landau free energy. The Landau free energy depends on the order parameter, and retains all the symmetries of the physical system. It's amazing how much you can get from symmetry, and we're able to see how it is that a ferromagnet can have what's called a continuous phase transition. That is, starting from zero temperature with a saturated magnetization, upon raising the temperature, the magnetization slowly decreases, until it has smoothly (continuously, in fact) gone to zero. This makes it a continous transition. We also show what a first order (discontinuous) phase transition would look like. First order phase transitions can exhibit supercooling and superheating. We also discuss the physics of alloys like bronze, and under what conditions two different materials will mix and form a binary mixture, and under what conditions there will be phase separation into 2 distinct concentrations, as happens with oil and water. A small concentration of impurities is always favorable according to entropy, and will always mix. But larger concentrations may "fall apart" and phase separate. Class discussions: Lots about supercooling and superheating. More about nonequilibrium behavior like window glass. Lecture Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,23311900</guid>
      <pubDate>Tue, 21 Aug 2007 08:11:54 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://web.ics.purdue.edu/~erica/416/mp3/Lecture20.LandauTheory.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 20:  Landau Theory of Phase Transitions; Oil, Water, and Alloys</title>
      <link>http://odeo.com/episodes/24181102-Lecture-20-Landau-Theory-of-Phase-Transitions-Oil-Water-and-Alloys</link>
      <description>Now that we know what order parameters are (see last lecture), we'll use the order parameter of a phase to construct the Landau free energy. The Landau free energy depends on the order parameter, and retains all the symmetries of the physical system. It's amazing how much you can get from symmetry, and we're able to see how it is that a ferromagnet can have what's called a continuous phase transition. That is, starting from zero temperature with a saturated magnetization, upon raising the temperature, the magnetization slowly decreases, until it has smoothly (continuously, in fact) gone to zero. This makes it a continous transition. We also show what a first order (discontinuous) phase transition would look like. First order phase transitions can exhibit supercooling and superheating. We also discuss the physics of alloys like bronze, and under what conditions two different materials will mix and form a binary mixture, and under what conditions there will be phase separation into 2 ...</description>
      <itunes:subtitle>Now that we know what order parameters are (see last lecture), we'll use the order parameter of a phase to construct the Landau free energy. The Landau free energy depends on the order parameter, and retains all the symmetries of the physical system. It's amazing how much you can get from symmetry, and we're able to see how it is that a ferromagnet can have what's called a continuous phase transition. That is, starting from zero temperature with a saturated magnetization, upon raising the temperature, the magnetization slowly decreases, until it has smoothly (continuously, in fact) gone to zero. This makes it a continous transition. We also show what a first order (discontinuous) phase transition would look like. First order phase transitions can exhibit supercooling and superheating. We also discuss the physics of alloys like bronze, and under what conditions two different materials will mix and form a binary mixture, and under what conditions there will be phase separation into 2 distinct concentrations, as happens with oil and water. A small concentration of impurities is always favorable according to entropy, and will always mix. But larger concentrations may "fall apart" and phase separate. Class discussions: Lots about supercooling and superheating. More about nonequilibrium behavior like window glass. Lecture Audio</itunes:subtitle>
      <itunes:summary>Now that we know what order parameters are (see last lecture), we'll use the order parameter of a phase to construct the Landau free energy. The Landau free energy depends on the order parameter, and retains all the symmetries of the physical system. It's amazing how much you can get from symmetry, and we're able to see how it is that a ferromagnet can have what's called a continuous phase transition. That is, starting from zero temperature with a saturated magnetization, upon raising the temperature, the magnetization slowly decreases, until it has smoothly (continuously, in fact) gone to zero. This makes it a continous transition. We also show what a first order (discontinuous) phase transition would look like. First order phase transitions can exhibit supercooling and superheating. We also discuss the physics of alloys like bronze, and under what conditions two different materials will mix and form a binary mixture, and under what conditions there will be phase separation into 2 distinct concentrations, as happens with oil and water. A small concentration of impurities is always favorable according to entropy, and will always mix. But larger concentrations may "fall apart" and phase separate. Class discussions: Lots about supercooling and superheating. More about nonequilibrium behavior like window glass. Lecture Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,24181102</guid>
      <pubDate>Tue, 21 Aug 2007 08:11:54 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://web.ics.purdue.edu/~erica/416/mp3/Lecture20.LandauTheory.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 19:  Symmetries, Order Parameters, and the Failure of Reductionism</title>
      <link>http://odeo.com/episodes/23311903-Lecture-19-Symmetries-Order-Parameters-and-the-Failure-of-Reductionism</link>
      <description>We finish the van der Waals equation of state, and use it to illustrate the liquid-gas phase transition. It turns out that at low pressure, the van der Waals equation of state has a wiggle where (dp/pV)0. Since this would cause an explosion, the system instead undergoes phase separation so that part of the container has liquid, and part has gas in it. More is different: We discuss the failure of reductionism. Reductionism is the idea that you will learn everything about an object by breaking it into its smallest bits -- like atoms, then electrons and protons, then quarks, then strings. But large collections of particles (like liquids, gases, and solids) have many properties which aren't really due to their constituents per se, but rather are due to larger organizing principles, and the symmetry of the associated phase. Example: All solids are hard, even though they're made out of different substances. So the property "hardness" is not actually caused by the particular form of the po...</description>
      <itunes:subtitle>We finish the van der Waals equation of state, and use it to illustrate the liquid-gas phase transition. It turns out that at low pressure, the van der Waals equation of state has a wiggle where (dp/pV)0. Since this would cause an explosion, the system instead undergoes phase separation so that part of the container has liquid, and part has gas in it. More is different: We discuss the failure of reductionism. Reductionism is the idea that you will learn everything about an object by breaking it into its smallest bits -- like atoms, then electrons and protons, then quarks, then strings. But large collections of particles (like liquids, gases, and solids) have many properties which aren't really due to their constituents per se, but rather are due to larger organizing principles, and the symmetry of the associated phase. Example: All solids are hard, even though they're made out of different substances. So the property "hardness" is not actually caused by the particular form of the potentials for the particular atoms in that solid. Rather, it's due to the symmetry of the regular crystalline structure the atoms take, and is independent of the type of atom. To illustrate, we discuss several phases of matter, and identify the corresponding "order parameter", which is a measurable quantity that captures the symmetry of the phase. Visual Aids: Rotini pasta to demonstrate twisted nematic phases. Specimens from my rock collection: quartz, amethyst, hematite, and others to see how all crystals are similar, despite being made from different atoms. The "sameness" manifests itself in the basic property of a solid: being hard. The "differenc" manifests itself in color, and in the shape of the crystals, which reveal the underlying quantum mechanics of how the chemical bonds form from atom to atom. Plus, the return of the squishy crystal to illustrate phonons. 0 Lecture Audio</itunes:subtitle>
      <itunes:summary>We finish the van der Waals equation of state, and use it to illustrate the liquid-gas phase transition. It turns out that at low pressure, the van der Waals equation of state has a wiggle where (dp/pV)0. Since this would cause an explosion, the system instead undergoes phase separation so that part of the container has liquid, and part has gas in it. More is different: We discuss the failure of reductionism. Reductionism is the idea that you will learn everything about an object by breaking it into its smallest bits -- like atoms, then electrons and protons, then quarks, then strings. But large collections of particles (like liquids, gases, and solids) have many properties which aren't really due to their constituents per se, but rather are due to larger organizing principles, and the symmetry of the associated phase. Example: All solids are hard, even though they're made out of different substances. So the property "hardness" is not actually caused by the particular form of the potentials for the particular atoms in that solid. Rather, it's due to the symmetry of the regular crystalline structure the atoms take, and is independent of the type of atom. To illustrate, we discuss several phases of matter, and identify the corresponding "order parameter", which is a measurable quantity that captures the symmetry of the phase. Visual Aids: Rotini pasta to demonstrate twisted nematic phases. Specimens from my rock collection: quartz, amethyst, hematite, and others to see how all crystals are similar, despite being made from different atoms. The "sameness" manifests itself in the basic property of a solid: being hard. The "differenc" manifests itself in color, and in the shape of the crystals, which reveal the underlying quantum mechanics of how the chemical bonds form from atom to atom. Plus, the return of the squishy crystal to illustrate phonons. 0 Lecture Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,23311903</guid>
      <pubDate>Tue, 21 Aug 2007 08:10:59 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://feeds.feedburner.com/~r/Physics416/~5/146537827/Lecture19.Symmetry.Reductionism.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 19:  Symmetries, Order Parameters, and the Failure of Reductionism</title>
      <link>http://odeo.com/episodes/24181103-Lecture-19-Symmetries-Order-Parameters-and-the-Failure-of-Reductionism</link>
      <description>We finish the van der Waals equation of state, and use it to illustrate the liquid-gas phase transition. It turns out that at low pressure, the van der Waals equation of state has a wiggle where (dp/pV)0. Since this would cause an explosion, the system instead undergoes phase separation so that part of the container has liquid, and part has gas in it. More is different: We discuss the failure of reductionism. Reductionism is the idea that you will learn everything about an object by breaking it into its smallest bits -- like atoms, then electrons and protons, then quarks, then strings. But large collections of particles (like liquids, gases, and solids) have many properties which aren't really due to their constituents per se, but rather are due to larger organizing principles, and the symmetry of the associated phase. Example: All solids are hard, even though they're made out of different substances. So the property "hardness" is not actually caused by the particular form of the po...</description>
      <itunes:subtitle>We finish the van der Waals equation of state, and use it to illustrate the liquid-gas phase transition. It turns out that at low pressure, the van der Waals equation of state has a wiggle where (dp/pV)0. Since this would cause an explosion, the system instead undergoes phase separation so that part of the container has liquid, and part has gas in it. More is different: We discuss the failure of reductionism. Reductionism is the idea that you will learn everything about an object by breaking it into its smallest bits -- like atoms, then electrons and protons, then quarks, then strings. But large collections of particles (like liquids, gases, and solids) have many properties which aren't really due to their constituents per se, but rather are due to larger organizing principles, and the symmetry of the associated phase. Example: All solids are hard, even though they're made out of different substances. So the property "hardness" is not actually caused by the particular form of the potentials for the particular atoms in that solid. Rather, it's due to the symmetry of the regular crystalline structure the atoms take, and is independent of the type of atom. To illustrate, we discuss several phases of matter, and identify the corresponding "order parameter", which is a measurable quantity that captures the symmetry of the phase. Visual Aids: Rotini pasta to demonstrate twisted nematic phases. Specimens from my rock collection: quartz, amethyst, hematite, and others to see how all crystals are similar, despite being made from different atoms. The "sameness" manifests itself in the basic property of a solid: being hard. The "differenc" manifests itself in color, and in the shape of the crystals, which reveal the underlying quantum mechanics of how the chemical bonds form from atom to atom. Plus, the return of the squishy crystal to illustrate phonons. 0 Lecture Audio</itunes:subtitle>
      <itunes:summary>We finish the van der Waals equation of state, and use it to illustrate the liquid-gas phase transition. It turns out that at low pressure, the van der Waals equation of state has a wiggle where (dp/pV)0. Since this would cause an explosion, the system instead undergoes phase separation so that part of the container has liquid, and part has gas in it. More is different: We discuss the failure of reductionism. Reductionism is the idea that you will learn everything about an object by breaking it into its smallest bits -- like atoms, then electrons and protons, then quarks, then strings. But large collections of particles (like liquids, gases, and solids) have many properties which aren't really due to their constituents per se, but rather are due to larger organizing principles, and the symmetry of the associated phase. Example: All solids are hard, even though they're made out of different substances. So the property "hardness" is not actually caused by the particular form of the potentials for the particular atoms in that solid. Rather, it's due to the symmetry of the regular crystalline structure the atoms take, and is independent of the type of atom. To illustrate, we discuss several phases of matter, and identify the corresponding "order parameter", which is a measurable quantity that captures the symmetry of the phase. Visual Aids: Rotini pasta to demonstrate twisted nematic phases. Specimens from my rock collection: quartz, amethyst, hematite, and others to see how all crystals are similar, despite being made from different atoms. The "sameness" manifests itself in the basic property of a solid: being hard. The "differenc" manifests itself in color, and in the shape of the crystals, which reveal the underlying quantum mechanics of how the chemical bonds form from atom to atom. Plus, the return of the squishy crystal to illustrate phonons. 0 Lecture Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,24181103</guid>
      <pubDate>Tue, 21 Aug 2007 08:10:59 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://web.ics.purdue.edu/~erica/416/mp3/Lecture19.Symmetry.Reductionism.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 18:  Van Der Waals and Geckos</title>
      <link>http://odeo.com/episodes/23311905-Lecture-18-Van-Der-Waals-and-Geckos</link>
      <description>We derive the shape of the phase boundary for solid to gas transitions (sublimation), examples being dry ice (CO2) or ice at low pressure. We derive the van der Waals equation of state, which is an improvement on the ideal gas equation pV=nRT. The ideal gas equation is based on two assumptions: 1. Particles occupy zero volume, and 2. Particles do not interact. Allowing for particles to have a finite size, and also allowing for the fact that at close range, gas particles feel van der Waals attractions, we get the new improved van der Waals equation of state for a gas made of sticky but hard molecules. Van der Waals attractions work because at close range, atoms and molecules notice each other's dipole moments. The dipole moments are due to the fact that at any given instant, the electron cloud is not quite centered on the nucleus of the atom (although it will be centered on average). This instantaneous dipole moment causes atoms in the vicinity to arrange their instantaneous dipoles ...</description>
      <itunes:subtitle>We derive the shape of the phase boundary for solid to gas transitions (sublimation), examples being dry ice (CO2) or ice at low pressure. We derive the van der Waals equation of state, which is an improvement on the ideal gas equation pV=nRT. The ideal gas equation is based on two assumptions: 1. Particles occupy zero volume, and 2. Particles do not interact. Allowing for particles to have a finite size, and also allowing for the fact that at close range, gas particles feel van der Waals attractions, we get the new improved van der Waals equation of state for a gas made of sticky but hard molecules. Van der Waals attractions work because at close range, atoms and molecules notice each other's dipole moments. The dipole moments are due to the fact that at any given instant, the electron cloud is not quite centered on the nucleus of the atom (although it will be centered on average). This instantaneous dipole moment causes atoms in the vicinity to arrange their instantaneous dipoles so as to lower their energy, which causes attraction. It turns out that geckos can cling to walls and ceilings because of van der Waals attractions. Gecko feet have tiny hairs that split many times to make many very fine tips, giving the hairs a very large total surface area. The fine hairs are able to form many contacts with any surface, and the surface-to-hair contact is adhesive due to van der Waals forces. One gecko foot can support the weight of an entire human. Video: Sticky gecko feet, and their van der Waals adhesive properties. Lecture Audio</itunes:subtitle>
      <itunes:summary>We derive the shape of the phase boundary for solid to gas transitions (sublimation), examples being dry ice (CO2) or ice at low pressure. We derive the van der Waals equation of state, which is an improvement on the ideal gas equation pV=nRT. The ideal gas equation is based on two assumptions: 1. Particles occupy zero volume, and 2. Particles do not interact. Allowing for particles to have a finite size, and also allowing for the fact that at close range, gas particles feel van der Waals attractions, we get the new improved van der Waals equation of state for a gas made of sticky but hard molecules. Van der Waals attractions work because at close range, atoms and molecules notice each other's dipole moments. The dipole moments are due to the fact that at any given instant, the electron cloud is not quite centered on the nucleus of the atom (although it will be centered on average). This instantaneous dipole moment causes atoms in the vicinity to arrange their instantaneous dipoles so as to lower their energy, which causes attraction. It turns out that geckos can cling to walls and ceilings because of van der Waals attractions. Gecko feet have tiny hairs that split many times to make many very fine tips, giving the hairs a very large total surface area. The fine hairs are able to form many contacts with any surface, and the surface-to-hair contact is adhesive due to van der Waals forces. One gecko foot can support the weight of an entire human. Video: Sticky gecko feet, and their van der Waals adhesive properties. Lecture Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,23311905</guid>
      <pubDate>Tue, 21 Aug 2007 08:09:12 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://web.ics.purdue.edu/~erica/416/mp3/Lecture18.VdW.Geckos.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 18:  Van Der Waals and Geckos</title>
      <link>http://odeo.com/episodes/24181104-Lecture-18-Van-Der-Waals-and-Geckos</link>
      <description>We derive the shape of the phase boundary for solid to gas transitions (sublimation), examples being dry ice (CO2) or ice at low pressure. We derive the van der Waals equation of state, which is an improvement on the ideal gas equation pV=nRT. The ideal gas equation is based on two assumptions: 1. Particles occupy zero volume, and 2. Particles do not interact. Allowing for particles to have a finite size, and also allowing for the fact that at close range, gas particles feel van der Waals attractions, we get the new improved van der Waals equation of state for a gas made of sticky but hard molecules. Van der Waals attractions work because at close range, atoms and molecules notice each other's dipole moments. The dipole moments are due to the fact that at any given instant, the electron cloud is not quite centered on the nucleus of the atom (although it will be centered on average). This instantaneous dipole moment causes atoms in the vicinity to arrange their instantaneous dipoles ...</description>
      <itunes:subtitle>We derive the shape of the phase boundary for solid to gas transitions (sublimation), examples being dry ice (CO2) or ice at low pressure. We derive the van der Waals equation of state, which is an improvement on the ideal gas equation pV=nRT. The ideal gas equation is based on two assumptions: 1. Particles occupy zero volume, and 2. Particles do not interact. Allowing for particles to have a finite size, and also allowing for the fact that at close range, gas particles feel van der Waals attractions, we get the new improved van der Waals equation of state for a gas made of sticky but hard molecules. Van der Waals attractions work because at close range, atoms and molecules notice each other's dipole moments. The dipole moments are due to the fact that at any given instant, the electron cloud is not quite centered on the nucleus of the atom (although it will be centered on average). This instantaneous dipole moment causes atoms in the vicinity to arrange their instantaneous dipoles so as to lower their energy, which causes attraction. It turns out that geckos can cling to walls and ceilings because of van der Waals attractions. Gecko feet have tiny hairs that split many times to make many very fine tips, giving the hairs a very large total surface area. The fine hairs are able to form many contacts with any surface, and the surface-to-hair contact is adhesive due to van der Waals forces. One gecko foot can support the weight of an entire human. Video: Sticky gecko feet, and their van der Waals adhesive properties. Lecture Audio</itunes:subtitle>
      <itunes:summary>We derive the shape of the phase boundary for solid to gas transitions (sublimation), examples being dry ice (CO2) or ice at low pressure. We derive the van der Waals equation of state, which is an improvement on the ideal gas equation pV=nRT. The ideal gas equation is based on two assumptions: 1. Particles occupy zero volume, and 2. Particles do not interact. Allowing for particles to have a finite size, and also allowing for the fact that at close range, gas particles feel van der Waals attractions, we get the new improved van der Waals equation of state for a gas made of sticky but hard molecules. Van der Waals attractions work because at close range, atoms and molecules notice each other's dipole moments. The dipole moments are due to the fact that at any given instant, the electron cloud is not quite centered on the nucleus of the atom (although it will be centered on average). This instantaneous dipole moment causes atoms in the vicinity to arrange their instantaneous dipoles so as to lower their energy, which causes attraction. It turns out that geckos can cling to walls and ceilings because of van der Waals attractions. Gecko feet have tiny hairs that split many times to make many very fine tips, giving the hairs a very large total surface area. The fine hairs are able to form many contacts with any surface, and the surface-to-hair contact is adhesive due to van der Waals forces. One gecko foot can support the weight of an entire human. Video: Sticky gecko feet, and their van der Waals adhesive properties. Lecture Audio</itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2007-08-21,24181104</guid>
      <pubDate>Tue, 21 Aug 2007 08:09:12 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="audio/mpeg" url="http://feedproxy.google.com/~r/Physics416/~5/LNvUTby5bj8/Lecture18.VdW.Geckos.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 1:  Accessible States</title>
      <link>http://odeo.com/episodes/1762296-Lecture-1-Accessible-States</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2006-08-22,1762296</guid>
      <pubDate>Tue, 22 Aug 2006 02:47:00 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://128.210.157.22:1013/Boilercast/2006/Fall/PHYS416/0101/PHYS416_2006_08_21_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 17: Introduction to Phase Transitions</title>
      <link>http://odeo.com/episodes/1762295-Lecture-17-Introduction-to-Phase-Transitions</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2006-08-21,1762295</guid>
      <pubDate>Mon, 21 Aug 2006 04:51:28 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://web.ics.purdue.edu/~erica/416/mp3/PHYS416_2005_10_31_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 16: Gibbs Free Energy and Chemical Reactions</title>
      <link>http://odeo.com/episodes/1762294-Lecture-16-Gibbs-Free-Energy-and-Chemical-Reactions</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2006-08-21,1762294</guid>
      <pubDate>Mon, 21 Aug 2006 04:49:19 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://web.ics.purdue.edu/~erica/416/mp3/PHYS416_2005_10_26_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 15: Refrigerators and Path Dependence of Work</title>
      <link>http://odeo.com/episodes/1762293-Lecture-15-Refrigerators-and-Path-Dependence-of-Work</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2006-08-21,1762293</guid>
      <pubDate>Mon, 21 Aug 2006 04:48:40 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://web.ics.purdue.edu/~erica/416/mp3/PHYS416_2005_10_24_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Midterm Review</title>
      <link>http://odeo.com/episodes/1762292-Midterm-Review</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2006-08-21,1762292</guid>
      <pubDate>Mon, 21 Aug 2006 04:48:00 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://web.ics.purdue.edu/~erica/416/mp3/PHYS416_2005_10_17_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 14: Engines</title>
      <link>http://odeo.com/episodes/1762291-Lecture-14-Engines</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2006-08-21,1762291</guid>
      <pubDate>Mon, 21 Aug 2006 04:47:04 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://web.ics.purdue.edu/~erica/416/mp3/PHYS416_2005_10_12_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 13: Bose Condensates</title>
      <link>http://odeo.com/episodes/1762290-Lecture-13-Bose-Condensates</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2006-08-21,1762290</guid>
      <pubDate>Mon, 21 Aug 2006 04:46:31 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://web.ics.purdue.edu/~erica/416/mp3/PHYS416_2005_10_05_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 12: Reversible and Irreversible Expansions</title>
      <link>http://odeo.com/episodes/1762288-Lecture-12-Reversible-and-Irreversible-Expansions</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2006-08-21,1762288</guid>
      <pubDate>Mon, 21 Aug 2006 04:45:06 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://web.ics.purdue.edu/~erica/416/mp3/PHYS416_2005_10_03_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 11: Bose Gas and Ideal Gas</title>
      <link>http://odeo.com/episodes/1762287-Lecture-11-Bose-Gas-and-Ideal-Gas</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2006-08-21,1762287</guid>
      <pubDate>Mon, 21 Aug 2006 04:44:16 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://web.ics.purdue.edu/~erica/416/mp3/PHYS416_2005_09_28_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 10:  Fermi-Dirac Distribution Function</title>
      <link>http://odeo.com/episodes/1762286-Lecture-10-Fermi-Dirac-Distribution-Function</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2006-08-21,1762286</guid>
      <pubDate>Mon, 21 Aug 2006 04:43:48 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://web.ics.purdue.edu/~erica/416/mp3/PHYS416_2005_09_26_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
    <item>
      <title>Lecture 9: Gibbs Factor and Gibbs Sum</title>
      <link>http://odeo.com/episodes/1762284-Lecture-9-Gibbs-Factor-and-Gibbs-Sum</link>
      <description></description>
      <itunes:subtitle></itunes:subtitle>
      <itunes:summary></itunes:summary>
      <guid isPermaLink="false">tag:odeo.com,2006-08-21,1762284</guid>
      <pubDate>Mon, 21 Aug 2006 04:43:10 -0700</pubDate>
      <itunes:explicit>no</itunes:explicit>
      <enclosure type="" url="http://web.ics.purdue.edu/~erica/416/mp3/PHYS416_2005_09_21_1330.mp3"/>
      <itunes:author>Thermal and Statistical Physics</itunes:author>
    </item>
  </channel>
</rss>
