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<?xml-stylesheet type="text/xsl" href="../assets/xml/rss.xsl" media="all"?><rss version="2.0" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>The Forbes Group (Posts about student_resources)</title><link>http://swan.physics.wsu.edu/forbes/</link><description></description><atom:link href="http://swan.physics.wsu.edu/forbes/categories/cat_student_resources.xml" rel="self" type="application/rss+xml"></atom:link><language>en</language><copyright>Contents © 2023 &lt;a href="mailto:Michael McNeil Forbes &lt;[email protected]&gt;"&gt;Michael McNeil Forbes&lt;/a&gt; </copyright><lastBuildDate>Wed, 15 Mar 2023 01:12:26 GMT</lastBuildDate><generator>Nikola (getnikola.com)</generator><docs>http://blogs.law.harvard.edu/tech/rss</docs><item><title>Prerequisites: Models</title><link>http://swan.physics.wsu.edu/forbes/public/student_resources/prerequisites_models/</link><dc:creator>Michael McNeil Forbes</dc:creator><description>&lt;div class="cell border-box-sizing text_cell rendered"&gt;&lt;div class="prompt input_prompt"&gt;
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&lt;h2 id="Prerequisites:-Models"&gt;Prerequisites: Models&lt;a class="anchor-link" href="http://swan.physics.wsu.edu/forbes/public/student_resources/prerequisites_models/#Prerequisites:-Models"&gt;&lt;/a&gt;&lt;/h2&gt;&lt;p&gt;This post describes various models that are useful for demonstrating interesting physics.&lt;/p&gt;
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&lt;p&gt;&lt;a href="http://swan.physics.wsu.edu/forbes/public/student_resources/prerequisites_models/"&gt;Read more…&lt;/a&gt; (1 min remaining to read)&lt;/p&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;</description><guid>http://swan.physics.wsu.edu/forbes/public/student_resources/prerequisites_models/</guid><pubDate>Tue, 07 Jan 2020 06:58:41 GMT</pubDate></item><item><title>Thermodynamics</title><link>http://swan.physics.wsu.edu/forbes/public/student_resources/thermodynamics/</link><dc:creator>Michael McNeil Forbes</dc:creator><description>&lt;div&gt;&lt;div class="cell border-box-sizing text_cell rendered"&gt;&lt;div class="prompt input_prompt"&gt;
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&lt;h2 id="Thermodynamics"&gt;Thermodynamics&lt;a class="anchor-link" href="http://swan.physics.wsu.edu/forbes/public/student_resources/thermodynamics/#Thermodynamics"&gt;&lt;/a&gt;&lt;/h2&gt;
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&lt;p&gt;This post discusses how phase equilibrium is established. In particular, we discuss multi-component saturating systems which spontaneously form droplets at zero temperature. This was specifically motivated by the discussion of the conditions for droplet formation in Bose-Fermi mixtures &lt;a href="https://arxiv.org/abs/1801.00346"&gt;1801.00346&lt;/a&gt; and &lt;a href="https://arxiv.org/abs/1804.03278"&gt;1804.03278&lt;/a&gt;. Specifically, the following conditions in &lt;a href="https://arxiv.org/abs/1804.03278"&gt;1804.03278&lt;/a&gt;:&lt;/p&gt;
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\begin{gather}
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\mathcal{E} &amp;lt; 0, \qquad \mathcal{P} = 0; \tag{i}\\
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\mu_b\pdiff{P}{n_f} = \mu_f\pdiff{P}{n_b}; \tag{ii}\\
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\pdiff{\mu_b}{n_b} &amp;gt; 0 , \qquad
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\pdiff{\mu_f}{n_f} &amp;gt; 0, \qquad
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\pdiff{\mu_b}{n_b}\pdiff{\mu_f}{n_f} &amp;gt; \left(\pdiff{\mu_b}{n_f}\right)^2. \tag{iii}
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\end{gather}&lt;p&gt;&lt;a href="https://arxiv.org/abs/1801.00346"&gt;1801.00346&lt;/a&gt;: &lt;a href="https://arxiv.org/abs/1801.00346"&gt;https://arxiv.org/abs/1801.00346&lt;/a&gt;
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&lt;a href="https://arxiv.org/abs/1804.03278"&gt;1804.03278&lt;/a&gt;: &lt;a href="https://arxiv.org/abs/1804.03278"&gt;https://arxiv.org/abs/1804.03278&lt;/a&gt;&lt;/p&gt;
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&lt;p&gt;&lt;a href="http://swan.physics.wsu.edu/forbes/public/student_resources/thermodynamics/"&gt;Read more…&lt;/a&gt; (3 min remaining to read)&lt;/p&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;</description><guid>http://swan.physics.wsu.edu/forbes/public/student_resources/thermodynamics/</guid><pubDate>Fri, 27 Apr 2018 16:31:12 GMT</pubDate></item><item><title>Uncertanties</title><link>http://swan.physics.wsu.edu/forbes/public/student_resources/uncertanties/</link><dc:creator>Michael McNeil Forbes</dc:creator><description>&lt;div class="cell border-box-sizing text_cell rendered"&gt;&lt;div class="prompt input_prompt"&gt;
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&lt;p&gt;&lt;img src="http://swan.physics.wsu.edu/forbes/images/Correlations.svg" alt="Correlation Plot"&gt;&lt;/p&gt;
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&lt;h2 id="Uncertainties"&gt;Uncertainties&lt;a class="anchor-link" href="http://swan.physics.wsu.edu/forbes/public/student_resources/uncertanties/#Uncertainties"&gt;&lt;/a&gt;&lt;/h2&gt;&lt;p&gt;Here we discuss the python &lt;a href="https://pythonhosted.org/uncertainties/"&gt;uncertainties&lt;/a&gt; package and demonstrate some of its features.&lt;/p&gt;
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&lt;p&gt;&lt;a href="http://swan.physics.wsu.edu/forbes/public/student_resources/uncertanties/"&gt;Read more…&lt;/a&gt; (6 min remaining to read)&lt;/p&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;</description><guid>http://swan.physics.wsu.edu/forbes/public/student_resources/uncertanties/</guid><pubDate>Wed, 06 Sep 2017 04:24:57 GMT</pubDate></item><item><title>Galilean Covariance</title><link>http://swan.physics.wsu.edu/forbes/public/student_resources/galilean-covariance/</link><dc:creator>Michael McNeil Forbes</dc:creator><description>&lt;div class="cell border-box-sizing text_cell rendered"&gt;&lt;div class="prompt input_prompt"&gt;
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&lt;p&gt;&lt;img src="https://upload.wikimedia.org/wikipedia/commons/8/85/F%C3%A9lix_Parra_-_Galileo_Demonstrating_the_New_Astronomical_Theories_at_the_University_of_Padua_-_Google_Art_Project.jpg" alt="Galileo"&gt;&lt;/p&gt;
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&lt;h2 id="Galilean-Covariance"&gt;Galilean Covariance&lt;a class="anchor-link" href="http://swan.physics.wsu.edu/forbes/public/student_resources/galilean-covariance/#Galilean-Covariance"&gt;&lt;/a&gt;&lt;/h2&gt;&lt;p&gt;In his &lt;a href="https://en.wikipedia.org/wiki/Dialogue_Concerning_the_Two_Chief_World_Systems"&gt;"Dialogue Concerning the Two Chief World Systems"&lt;/a&gt;, Galileo put forth the notion that the laws of physics are the same in any constantly moving (inertial) reference frame.
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Colloquially this means that if you are on a train, there is no experiment you can do to tell that the train is moving (without looking outside).&lt;/p&gt;
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&lt;p&gt;This post will explain formally what Galilean covariance means, clarify the difference between covariance and invariance, and elucidate the meaning of Galilean covariance in classical and quantum mechanics. In particular, it will explain the following result obtained by simply changing coordinates, which may appear paradoxical at first:&lt;/p&gt;
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&lt;blockquote&gt;
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&lt;p&gt;Consider a modern Lagrangian formulation of a classical object moving without a potential in 1D with coordinates $x$ and $\dot{x}$, and the same object in a moving frame with coordinates $X = x - vt$ and $\dot{X} = \dot{x} - v$. The Lagrangian and conjugate momenta in these frames are:&lt;/p&gt;
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&lt;p&gt;\begin{align}&lt;/p&gt;
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&lt;p&gt;L[x, \dot{x}, t] &amp;amp;= \frac{m\dot{x}^2}{2}, &amp;amp;
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p &amp;amp;\equiv \pdiff{L}{\dot{x}} = m\dot{x},\
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L_v[X, \dot{X}, t] &amp;amp;= \frac{m(\dot{X}+v)^2}{2}, &amp;amp;
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P &amp;amp;\equiv \pdiff{L_v}{\dot{X}} = m(\dot{X}+v) = p.
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\end{align}&lt;/p&gt;
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&lt;blockquote&gt;
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&lt;p&gt;Perhaps surprisingly the conjugate momentum $P$ is the same in the moving frame whereas Galilean invariance implies that one should have a description in terms of $P = m\dot{X} = p - mv$. The later description exists, but requires a somewhat non-intuitive addition to the Lagrangian of a total derivative.&lt;/p&gt;
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&lt;p&gt;&lt;a href="http://swan.physics.wsu.edu/forbes/public/student_resources/galilean-covariance/"&gt;Read more…&lt;/a&gt; (10 min remaining to read)&lt;/p&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;</description><guid>http://swan.physics.wsu.edu/forbes/public/student_resources/galilean-covariance/</guid><pubDate>Tue, 16 May 2017 04:02:42 GMT</pubDate></item><item><title>Kamiak</title><link>http://swan.physics.wsu.edu/forbes/public/student_resources/kamiak/</link><dc:creator>Michael McNeil Forbes</dc:creator><description>&lt;div&gt;&lt;div class="cell border-box-sizing text_cell rendered"&gt;&lt;div class="prompt input_prompt"&gt;
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&lt;a href="https://hpc.wsu.edu/what-is-kamiak/" class="image"&gt;
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&lt;img alt="Kamiak Research Cluster at WSU" src="http://swan.physics.wsu.edu/forbes/images/kamiak-comp.png"&gt;&lt;/a&gt;
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&lt;h2 id="Kamiak-Cluster-at-WSU"&gt;Kamiak Cluster at WSU&lt;a class="anchor-link" href="http://swan.physics.wsu.edu/forbes/public/student_resources/kamiak/#Kamiak-Cluster-at-WSU"&gt;&lt;/a&gt;&lt;/h2&gt;
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&lt;p&gt;Here we document our experience using the Kamiak HPC cluster at WSU.&lt;/p&gt;
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&lt;h3 id="Resources"&gt;Resources&lt;a class="anchor-link" href="http://swan.physics.wsu.edu/forbes/public/student_resources/kamiak/#Resources"&gt;&lt;/a&gt;&lt;/h3&gt;
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&lt;h4 id="Kamiak-Specific"&gt;Kamiak Specific&lt;a class="anchor-link" href="http://swan.physics.wsu.edu/forbes/public/student_resources/kamiak/#Kamiak-Specific"&gt;&lt;/a&gt;&lt;/h4&gt;&lt;ul&gt;
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&lt;li&gt;&lt;a href="https://hpc.wsu.edu/users-guide/"&gt;Kamiak Users Guide&lt;/a&gt;: Read this.&lt;/li&gt;
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&lt;li&gt;&lt;a href="https://hpc.wsu.edu/support/service-requests/"&gt;Service Requests&lt;/a&gt;: Request access to Kamiak here and use this for other service requests (software installation, issues with the cluster, etc.)&lt;/li&gt;
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&lt;li&gt;&lt;a href="https://hpc.wsu.edu/kamiak-hpc/queue-list/"&gt;Queue List&lt;/a&gt;: List of queues.&lt;/li&gt;
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&lt;/ul&gt;
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&lt;h4 id="General"&gt;General&lt;a class="anchor-link" href="http://swan.physics.wsu.edu/forbes/public/student_resources/kamiak/#General"&gt;&lt;/a&gt;&lt;/h4&gt;&lt;ul&gt;
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&lt;li&gt;&lt;a href="https://slurm.schedmd.com"&gt;SLURM&lt;/a&gt;: Main documentation for the current job scheduler.&lt;/li&gt;
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&lt;li&gt;&lt;a href="http://lmod.readthedocs.org"&gt;Lmod&lt;/a&gt;: Environment module system.&lt;/li&gt;
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&lt;li&gt;&lt;a href="https://conda.io/en/latest/"&gt;Conda&lt;/a&gt;: Package manager for python and other software.&lt;/li&gt;
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&lt;p&gt;&lt;a href="http://swan.physics.wsu.edu/forbes/public/student_resources/kamiak/"&gt;Read more…&lt;/a&gt; (27 min remaining to read)&lt;/p&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;</description><guid>http://swan.physics.wsu.edu/forbes/public/student_resources/kamiak/</guid><pubDate>Fri, 21 Oct 2016 19:50:27 GMT</pubDate></item><item><title>Prerequisites</title><link>http://swan.physics.wsu.edu/forbes/public/student_resources/prerequisites/</link><dc:creator>Michael McNeil Forbes</dc:creator><description>&lt;div class="cell border-box-sizing text_cell rendered"&gt;&lt;div class="prompt input_prompt"&gt;
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&lt;img src="http://swan.physics.wsu.edu/forbes/images/eli-francis-100644.jpg"&gt;
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&lt;a style='background-color:black;color:white;text-decoration:none;padding:4px 6px;font-family:-apple-system, BlinkMacSystemFont, "San Francisco", "Helvetica Neue", Helvetica, Ubuntu, Roboto, Noto, "Segoe UI", Arial, sans-serif;font-size:12px;font-weight:bold;line-height:1.2;display:inline-block;border-radius:3px;' href="https://unsplash.com/@elifrancis?utm_medium=referral&amp;amp;utm_campaign=photographer-credit&amp;amp;utm_content=creditBadge" target="_blank" rel="noopener noreferrer" title="Download free do whatever you want high-resolution photos from Eli Francis"&gt;&lt;span style="display:inline-block;padding:2px 3px;"&gt;&lt;svg xmlns="http://www.w3.org/2000/svg" style="height:12px;width:auto;position:relative;vertical-align:middle;top:-1px;fill:white;" viewbox="0 0 32 32"&gt;&lt;title&gt;&lt;/title&gt;&lt;path d="M20.8 18.1c0 2.7-2.2 4.8-4.8 4.8s-4.8-2.1-4.8-4.8c0-2.7 2.2-4.8 4.8-4.8 2.7.1 4.8 2.2 4.8 4.8zm11.2-7.4v14.9c0 2.3-1.9 4.3-4.3 4.3h-23.4c-2.4 0-4.3-1.9-4.3-4.3v-15c0-2.3 1.9-4.3 4.3-4.3h3.7l.8-2.3c.4-1.1 1.7-2 2.9-2h8.6c1.2 0 2.5.9 2.9 2l.8 2.4h3.7c2.4 0 4.3 1.9 4.3 4.3zm-8.6 7.5c0-4.1-3.3-7.5-7.5-7.5-4.1 0-7.5 3.4-7.5 7.5s3.3 7.5 7.5 7.5c4.2-.1 7.5-3.4 7.5-7.5z"&gt;&lt;/path&gt;&lt;/svg&gt;&lt;/span&gt;&lt;span style="display:inline-block;padding:2px 3px;"&gt;Eli Francis&lt;/span&gt;&lt;/a&gt;
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&lt;h2 id="Prerequisites"&gt;Prerequisites&lt;a class="anchor-link" href="http://swan.physics.wsu.edu/forbes/public/student_resources/prerequisites/#Prerequisites"&gt;&lt;/a&gt;&lt;/h2&gt;&lt;p&gt;This post describes the prerequisites that I will generally assume you have if you want to work with me. It also contains a list of references where you can learn these prerequisites. Please let me know if you find any additional resources particularly useful so I can add them for the benefit of others. This list is by definition incomplete - you should regard it as a minimum.&lt;/p&gt;
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&lt;p&gt;&lt;a href="mailto:[email protected]"&gt;[email protected]&lt;/a&gt;&lt;/p&gt;
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&lt;p&gt;&lt;a href="http://swan.physics.wsu.edu/forbes/public/student_resources/prerequisites/"&gt;Read more…&lt;/a&gt; (11 min remaining to read)&lt;/p&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;</description><guid>http://swan.physics.wsu.edu/forbes/public/student_resources/prerequisites/</guid><pubDate>Tue, 03 May 2016 22:58:41 GMT</pubDate></item><item><title>Many-body Quantum Mechanics</title><link>http://swan.physics.wsu.edu/forbes/public/student_resources/many-body-quantum-mechanics/</link><dc:creator>Michael McNeil Forbes</dc:creator><description>&lt;div&gt;&lt;div class="cell border-box-sizing text_cell rendered"&gt;&lt;div class="prompt input_prompt"&gt;
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&lt;h2 id="Many-body-Quantum-Mechanics"&gt;Many-body Quantum Mechanics&lt;a class="anchor-link" href="http://swan.physics.wsu.edu/forbes/public/student_resources/many-body-quantum-mechanics/#Many-body-Quantum-Mechanics"&gt;&lt;/a&gt;&lt;/h2&gt;
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&lt;p&gt;In this notebook, we briefly discuss the formalism of many-body theory from the point of view of quantum mechanics.&lt;/p&gt;
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&lt;p&gt;&lt;a href="http://swan.physics.wsu.edu/forbes/public/student_resources/many-body-quantum-mechanics/"&gt;Read more…&lt;/a&gt; (6 min remaining to read)&lt;/p&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;&lt;/div&gt;</description><guid>http://swan.physics.wsu.edu/forbes/public/student_resources/many-body-quantum-mechanics/</guid><pubDate>Wed, 11 Mar 2015 06:13:48 GMT</pubDate></item></channel></rss>
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