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		<id>https://en.formulasearchengine.com/w/index.php?title=Recursively_inseparable_sets&amp;diff=25198</id>
		<title>Recursively inseparable sets</title>
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		<summary type="html">&lt;p&gt;216.40.38.234: /* Definition */ Formatting fix&lt;/p&gt;
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&lt;div&gt;The &#039;&#039;&#039;Buckingham potential&#039;&#039;&#039; is a [[mathematical formula|formula]] proposed by [[Richard Buckingham]] which describes the [[Wolfgang Pauli|Pauli]] [[Exchange interaction|repulsion energy]] and [[van der Waals force|van der Waals energy]] &amp;lt;math&amp;gt;\Phi_{12}(r)&amp;lt;/math&amp;gt; for the interaction of two atoms that are not directly bonded as a function of the [[Atomic spacing|interatomic distance]] &amp;lt;math&amp;gt;r&amp;lt;/math&amp;gt;.&lt;br /&gt;
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:&amp;lt;math&amp;gt;\Phi_{12}(r) = A \exp \left(-Br\right) - \frac{C}{r^6}&amp;lt;/math&amp;gt;&lt;br /&gt;
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Here, &amp;lt;math&amp;gt;A&amp;lt;/math&amp;gt;, &amp;lt;math&amp;gt;B&amp;lt;/math&amp;gt; and &amp;lt;math&amp;gt;C&amp;lt;/math&amp;gt; are constants. The two terms on the right-hand side constitute a repulsion and an attraction, because their first [[derivative]]s with respect to &amp;lt;math&amp;gt;r&amp;lt;/math&amp;gt; are negative and positive, respectively.&lt;br /&gt;
&lt;br /&gt;
Buckingham proposed this as a simplification of the [[Lennard-Jones potential]], in a theoretical study of the [[equation of state]] for [[gas]]eous [[helium]], [[neon]] and [[argon]].&amp;lt;ref&amp;gt;R. A. Buckingham, &#039;&#039;The Classical Equation of State of Gaseous Helium, Neon and Argon&#039;&#039;, Proceedings of the Royal Society of London. Series A, Mathematical and Physical Sciences &#039;&#039;&#039;168&#039;&#039;&#039; pp. 264-283 (1938)]&amp;lt;/ref&amp;gt;&lt;br /&gt;
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As explained in Buckingham&#039;s original paper and, e.g., in section 2.2.5 of Jensen&#039;s text,&amp;lt;ref name=jensen&amp;gt;F. Jensen, &#039;&#039;Introduction to Computational Chemistry&#039;&#039;, 2nd ed., Wiley, 2007,&amp;lt;/ref&amp;gt; the repulsion is due to the interpenetration of the closed [[electron shell]]s. &amp;quot;There is therefore some justification for choosing the repulsive part (of the potential) as an [[exponential function]]&amp;quot;. The Buckingham potential has been used extensively in simulations of [[molecular dynamics]]. &lt;br /&gt;
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Because the exponential term converges to a constant as &amp;lt;math&amp;gt;r&amp;lt;/math&amp;gt;→&amp;lt;math&amp;gt;0&amp;lt;/math&amp;gt;, while the &amp;lt;math&amp;gt;r^{-6}&amp;lt;/math&amp;gt; term diverges, the Buckingham potential &amp;quot;turns over&amp;quot; as &amp;lt;math&amp;gt;r&amp;lt;/math&amp;gt; becomes small. This may be problematic when dealing with a structure with very short interatomic distances, as the nuclei that cross the turn-over will become strongly (and unphysically) bound to one another at a distance of zero.&amp;lt;ref name=jensen/&amp;gt;&lt;br /&gt;
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==References==&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
&lt;br /&gt;
==External links==&lt;br /&gt;
*[http://www.sklogwiki.org/SklogWiki/index.php/Buckingham_potential Buckingham potential] on [http://www.sklogwiki.org/SklogWiki/index.php/Main_Page SklogWiki]&lt;br /&gt;
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{{DEFAULTSORT:Buckingham potential}}&lt;br /&gt;
[[Category:Theoretical chemistry]]&lt;br /&gt;
[[Category:Computational chemistry]]&lt;br /&gt;
[[Category:Thermodynamics]]&lt;br /&gt;
[[Category:Chemical bonding]]&lt;br /&gt;
[[Category:Intermolecular forces]]&lt;br /&gt;
[[Category:Potentials]]&lt;/div&gt;</summary>
		<author><name>216.40.38.234</name></author>
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