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		<title>en&gt;M-le-mot-dit: /* Technical details */ disambiguation error</title>
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		<summary type="html">&lt;p&gt;&lt;span class=&quot;autocomment&quot;&gt;Technical details: &lt;/span&gt; disambiguation error&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;The &amp;#039;&amp;#039;&amp;#039;effective potential&amp;#039;&amp;#039;&amp;#039; (also known as &amp;#039;&amp;#039;&amp;#039;effective potential energy&amp;#039;&amp;#039;&amp;#039;) is a mathematical expression combining multiple (perhaps opposing) effects into a single potential. In [[classical mechanics]] it is defined as the sum of the &amp;#039;opposing&amp;#039; [[centrifugal potential energy]] with the [[potential energy]] of a [[dynamical system]]. It is commonly used in calculating the [[orbit]]s of planets (both [[Newtonian mechanics|Newtonian]] and [[general relativity|relativistic]]) and in semi-classical atomic calculations, and often allows problems to be reduced to fewer [[dimension]]s.&lt;br /&gt;
&lt;br /&gt;
==Definition==&lt;br /&gt;
The effective potential &amp;lt;math&amp;gt;U_\text{eff}&amp;lt;/math&amp;gt; is defined in the following way:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt; U_\text{eff}(\mathbf{r}) = \frac{L^2}{2mr^2} + U(\mathbf{r}) &amp;lt;/math&amp;gt;&lt;br /&gt;
:&amp;#039;&amp;#039;L&amp;#039;&amp;#039; is the [[angular momentum]]&lt;br /&gt;
:&amp;#039;&amp;#039;r&amp;#039;&amp;#039; is the distance between the two masses&lt;br /&gt;
:&amp;#039;&amp;#039;m&amp;#039;&amp;#039; is the [[mass]] of the orbiting body&lt;br /&gt;
:&amp;#039;&amp;#039;U(r)&amp;#039;&amp;#039; is the general form of the [[potential]]&lt;br /&gt;
&lt;br /&gt;
The effective force, then, is the negative [[gradient]] of the effective potential:&lt;br /&gt;
&lt;br /&gt;
&amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
\mathbf{F}_\text{eff} &amp;amp;= -\nabla U_\text{eff}(\mathbf{r}) \\&lt;br /&gt;
                      &amp;amp;= \frac{L^2}{mr^3}\hat{\mathbf{r}} - \nabla U(\mathbf{r})&lt;br /&gt;
\end{align}&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Where &amp;lt;math&amp;gt;\hat{\mathbf{r}}&amp;lt;/math&amp;gt; denotes a unit vector in the radial direction.&lt;br /&gt;
&lt;br /&gt;
==Important properties==&lt;br /&gt;
There are many useful features of the effective potential. &lt;br /&gt;
The condition for a particle of energy &amp;#039;&amp;#039;E&amp;#039;&amp;#039; flying by to be `trapped&amp;#039; and go into an orbit:&lt;br /&gt;
:&amp;lt;math&amp;gt; U_\text{eff} &amp;lt; E &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
To find the radius of a circular orbit, we simply minimize the effective potential with respect to &amp;lt;math&amp;gt;r&amp;lt;/math&amp;gt;, or equivalently set the net force to zero and then solve for &amp;lt;math&amp;gt;r_0&amp;lt;/math&amp;gt;:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \frac{d U_\text{eff}}{dr} = 0 &amp;lt;/math&amp;gt;&lt;br /&gt;
After solving for &amp;lt;math&amp;gt;r_0&amp;lt;/math&amp;gt;, plug this back into &amp;lt;math&amp;gt;U_\text{eff}&amp;lt;/math&amp;gt; to find the maximum value of the effective potential &amp;lt;math&amp;gt;U_\text{eff}^\text{max}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
To find the frequency of small oscillations:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \omega = \sqrt{\frac{U_\text{eff}&amp;#039;&amp;#039;}{m}} &amp;lt;/math&amp;gt;&lt;br /&gt;
where the double prime indicates the second derivative of the effective potential with respect to &amp;lt;math&amp;gt;r&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
==Example: gravitational potential==&lt;br /&gt;
&lt;br /&gt;
For example, consider a particle of mass &amp;#039;&amp;#039;m&amp;#039;&amp;#039; orbiting a much heavier object of mass &amp;#039;&amp;#039;M&amp;#039;&amp;#039;.  Assuming Newtonian mechanics can be used, and the motion of the larger mass is negligible, then the conservation of [[energy]] and [[angular momentum]] give two constants &amp;#039;&amp;#039;E&amp;#039;&amp;#039; and &amp;#039;&amp;#039;L&amp;#039;&amp;#039;, with values&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;E = \frac{1}{2}m\left(\dot{r}^2 + r^2\dot{\phi}^2\right) - \frac{GmM}{r},&amp;lt;/math&amp;gt;&lt;br /&gt;
:&amp;lt;math&amp;gt;L = mr^2\dot{\phi} \, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\dot{r}&amp;lt;/math&amp;gt; is the derivative of r with respect to time,&lt;br /&gt;
:&amp;lt;math&amp;gt;\dot{\phi}&amp;lt;/math&amp;gt; is the [[angular velocity]] of mass&amp;amp;nbsp;&amp;#039;&amp;#039;m&amp;#039;&amp;#039;,&lt;br /&gt;
:&amp;#039;&amp;#039;G&amp;#039;&amp;#039; is the [[gravitational constant]],&lt;br /&gt;
:&amp;#039;&amp;#039;E&amp;#039;&amp;#039; is the total energy, and&lt;br /&gt;
&lt;br /&gt;
Only two variables are needed, since the motion occurs in a plane.  Substituting the second expression into the first and rearranging gives&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;m\dot{r}^2 = 2E - \frac{L^2}{mr^2} + \frac{2GmM}{r} = 2E - \frac{1}{r^2}\left(\frac{L^2}{m} - 2GmMr\right),&amp;lt;/math&amp;gt;&lt;br /&gt;
:&amp;lt;math&amp;gt;\frac{1}{2}m\dot{r}^2 = E - U_\text{eff}(r),&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;U_\text{eff}(r) = \frac{L^2}{2mr^2} - \frac{GmM}{r} &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
is the effective potential.&amp;lt;ref group=&amp;quot;Note&amp;quot;&amp;gt;A similar derivation may be found in Jos&amp;amp;eacute; &amp;amp; Saletan, &amp;#039;&amp;#039;Classical Dynamics: A Contemporary Approach&amp;#039;&amp;#039;, pgs. 31&amp;amp;ndash;33&amp;lt;/ref&amp;gt; As is evident from the above equation, the original two variable problem has been reduced to a one variable problem.  For many applications the effective potential can be treated exactly like the potential energy of a one-dimensional system: for instance, an energy diagram using the effective potential determines turning points and locations of stable and unstable [[Mechanical equilibrium|equilibria]]. A similar method may be used in other applications, for instance determining orbits in a general relativistic [[Schwarzschild metric]]. &lt;br /&gt;
&lt;br /&gt;
Effective potentials are widely used in various fields of condensed matter, like e.g. the Gauss-core potential (Likos 2002, Baeurle 2004) and the screened [[Coulomb potential]] (Likos 2001).&lt;br /&gt;
&lt;br /&gt;
==Notes==&lt;br /&gt;
&amp;lt;references group=&amp;quot;Note&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
{{Reflist}}&lt;br /&gt;
&lt;br /&gt;
* {{Cite book|last1=Jos&amp;amp;eacute;|first1=JV|last2=Saletan|first2=EJ|year=1998|title=Classical Dynamics: A Contemporary Approach|edition=1st|publisher=Cambridge University Press|isbn=0-521-63636-1|postscript=&amp;lt;!-- Bot inserted parameter. Either remove it; or change its value to &amp;quot;.&amp;quot; for the cite to end in a &amp;quot;.&amp;quot;, as necessary. --&amp;gt;{{inconsistent citations}}}}.&lt;br /&gt;
&lt;br /&gt;
* {{cite journal&lt;br /&gt;
    |url = http://jcp.aip.org/jcpsa6/v117/i4/p1869_s1?isAuthorized=no&lt;br /&gt;
    |last = Likos et al&lt;br /&gt;
    |first = C.N. &lt;br /&gt;
    |last2 = Rosenfeldt &lt;br /&gt;
    |first2 = S. &lt;br /&gt;
    |last3 = Dingenouts &lt;br /&gt;
    |first3 = N. &lt;br /&gt;
    |last4 = Ballauff &lt;br /&gt;
    |first4 = M. &lt;br /&gt;
    |last5 = Lindner &lt;br /&gt;
    |first5 = P. &lt;br /&gt;
    |last6 = Werner &lt;br /&gt;
    |first6 = N. &lt;br /&gt;
    |last7 = Vögtle &lt;br /&gt;
    |first7 = F.&lt;br /&gt;
    |title =  Gaussian effective interaction between flexible dendrimers of fourth generation: a theoretical and experimental study&lt;br /&gt;
    |journal = J. Chem. Phys.&lt;br /&gt;
    |volume = 117&lt;br /&gt;
    |pages = 1869&amp;amp;ndash;1877&lt;br /&gt;
    |year = 2002&lt;br /&gt;
    |doi = 10.1063/1.1486209|bibcode = 2002JChPh.117.1869L &lt;br /&gt;
    |issue = 4 }}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal&lt;br /&gt;
    |url = http://www.springerlink.com/content/t238g8pk30606027/ &lt;br /&gt;
    |last = Baeurle&lt;br /&gt;
    |first = S.A.&lt;br /&gt;
    |coauthors = Kroener J.&lt;br /&gt;
    |title = Modeling Effective Interactions of Micellar Aggregates of Ionic Surfactants with the Gauss-Core Potential  &lt;br /&gt;
    |journal = J. Math. Chem. &lt;br /&gt;
    |volume = 36&lt;br /&gt;
    |pages = 409&amp;amp;ndash;421 &lt;br /&gt;
    |year = 2004 &lt;br /&gt;
    |doi = 10.1023/B:JOMC.0000044526.22457.bb &lt;br /&gt;
    |issue = 4}}&lt;br /&gt;
&lt;br /&gt;
* {{cite journal&lt;br /&gt;
    |url = http://www.sciencedirect.com/science?_ob=ArticleURL&amp;amp;_udi=B6TVP-439VDH7-1&amp;amp;_user=616165&amp;amp;_coverDate=07%2F31%2F2001&amp;amp;_rdoc=1&amp;amp;_fmt=high&amp;amp;_orig=search&amp;amp;_sort=d&amp;amp;_docanchor=&amp;amp;view=c&amp;amp;_searchStrId=1343199058&amp;amp;_rerunOrigin=scholar.google&amp;amp;_acct=C000032338&amp;amp;_version=1&amp;amp;_urlVersion=0&amp;amp;_userid=616165&amp;amp;md5=09b16d8bfcfeecad13e87c345623bd4e &lt;br /&gt;
    |last = Likos &lt;br /&gt;
    |first = C.N.&lt;br /&gt;
    |title =  Effective interactions in soft condensed matter physics &lt;br /&gt;
    |journal = Physics Reports&lt;br /&gt;
    |volume = 348&lt;br /&gt;
    |pages = 267&amp;amp;ndash;439 &lt;br /&gt;
    |year = 2001&lt;br /&gt;
    |doi = 10.1016/S0370-1573(00)00141-1|bibcode = 2001PhR...348..267L &lt;br /&gt;
    |issue = 4–5 }}&lt;br /&gt;
&lt;br /&gt;
{{DEFAULTSORT:Effective Potential}}&lt;br /&gt;
[[Category:Mechanics]]&lt;/div&gt;</summary>
		<author><name>en&gt;M-le-mot-dit</name></author>
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