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		<id>https://en.formulasearchengine.com/index.php?title=Saltwater_intrusion&amp;diff=8036</id>
		<title>Saltwater intrusion</title>
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		<updated>2014-01-07T17:59:05Z</updated>

		<summary type="html">&lt;p&gt;122.164.159.160: /* Groundwater extraction */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;In [[mathematics]] and [[theoretical physics]], the &#039;&#039;&#039;induced metric&#039;&#039;&#039; is the [[metric tensor]] defined on a [[submanifold]] which is calculated from the metric tensor on a larger [[manifold]] into which the submanifold is embedded. It may be calculated using the following formula (written using [[Einstein summation convention]]):&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;g_{ab} = \partial_a X^\mu \partial_b X^\nu  g_{\mu\nu} (X^\alpha) \ &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Here &amp;lt;math&amp;gt;a,b \ &amp;lt;/math&amp;gt; describe the indices of coordinates &amp;lt;math&amp;gt;\xi^a \ &amp;lt;/math&amp;gt; of the submanifold while the functions &amp;lt;math&amp;gt;X^\mu(\xi^a) \ &amp;lt;/math&amp;gt; encode the embedding into the higher-dimensional manifold whose tangent indices are denoted &amp;lt;math&amp;gt;\mu,\nu \ &amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
==Example - Curve on a torus==&lt;br /&gt;
&lt;br /&gt;
Let&lt;br /&gt;
: &amp;lt;math&amp;gt;\begin{align}&lt;br /&gt;
 \Pi\colon \mathcal{C} &amp;amp;\to \mathbb{R}^3 \\&lt;br /&gt;
 \tau &amp;amp;\mapsto \left\{\quad\begin{matrix}x^1=(a+b\cos(n\cdot \tau))\cos(m\cdot \tau)\\x^2=(a+b\cos(n\cdot \tau))\sin(m\cdot \tau)\\x^3=b\sin(n\cdot \tau)\end{matrix}\right.&lt;br /&gt;
\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
be a map from the domain of the curve &amp;lt;math&amp;gt;\mathcal{C}&amp;lt;/math&amp;gt;  with parameter &amp;lt;math&amp;gt;\tau&amp;lt;/math&amp;gt; into the euclidean manifold &amp;lt;math&amp;gt;\mathbb{R}^3&amp;lt;/math&amp;gt;. Here &amp;lt;math&amp;gt;a,b,m,n\in\mathbb{R}&amp;lt;/math&amp;gt; are constants.&lt;br /&gt;
&lt;br /&gt;
Then there is a metric given on &amp;lt;math&amp;gt;\mathbb{R}^3&amp;lt;/math&amp;gt; as&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;g=\sum\limits_{\mu,\nu}g_{\mu\nu}\mathrm{d}x^\mu\otimes \mathrm{d}x^\nu\quad\text{with}\quad&lt;br /&gt;
g_{\mu\nu} = \begin{pmatrix}1 &amp;amp; 0 &amp;amp; 0\\0 &amp;amp; 1 &amp;amp; 0\\0 &amp;amp; 0 &amp;amp; 1\end{pmatrix}&lt;br /&gt;
&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
and we compute&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;g_{\tau\tau}=\sum\limits_{\mu,\nu}\frac{\partial x^\mu}{\partial \tau}\frac{\partial x^\nu}{\partial \tau}\underbrace{g_{\mu\nu}}_{\delta_{\mu\nu}} = \sum\limits_\mu\left(\frac{\partial x^\mu}{\partial \tau}\right)^2=m^2 a^2+2m^2ab\cos(n\cdot \tau)+m^2b^2\cos^2(n\cdot \tau)+b^2n^2&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Therefore &amp;lt;math&amp;gt;g_\mathcal{C}=(m^2 a^2+2m^2ab\cos(n\cdot \tau)+m^2b^2\cos^2(n\cdot \tau)+b^2n^2)\mathrm{d}\tau\otimes \mathrm{d}\tau&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
*[[First fundamental form]]&lt;br /&gt;
&lt;br /&gt;
[[Category:Differential geometry]]&lt;br /&gt;
&lt;br /&gt;
{{physics-stub}}&lt;/div&gt;</summary>
		<author><name>122.164.159.160</name></author>
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