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	<title>what is london penetration depth | Winner Science</title>
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		<title>London equations: explanation of flux penetration</title>
		<link>https://winnerscience.com/london-equations-explanation-of-flux-penetration/</link>
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		<dc:creator><![CDATA[amsh]]></dc:creator>
		<pubDate>Sun, 23 Oct 2011 13:09:56 +0000</pubDate>
				<category><![CDATA[Superconductivity]]></category>
		<category><![CDATA[definition london penetration depth]]></category>
		<category><![CDATA[explanation of meissner effect using london equations]]></category>
		<category><![CDATA[flux penetration and london equations]]></category>
		<category><![CDATA[importance helmholtz theorem]]></category>
		<category><![CDATA[london penetration depth]]></category>
		<category><![CDATA[london penetration depth dependence on temperature]]></category>
		<category><![CDATA[meissner effect and london equations]]></category>
		<category><![CDATA[relation london penetration depth with temperature]]></category>
		<category><![CDATA[significance of gradient]]></category>
		<category><![CDATA[what is london penetration depth]]></category>
		<guid isPermaLink="false">https://winnerscience.com/?p=2475</guid>

					<description><![CDATA[<p>As we have already derived the London equations in last article. Now let us explain the flux penetration (Meissner effect) from London equations: To explain Meissner effect from London equations consider the differential form of Ampere’s circuital law: del x B = µoJs where B is magnetic flux density and</p>
<p>The post <a href="https://winnerscience.com/london-equations-explanation-of-flux-penetration/">London equations: explanation of flux penetration</a> first appeared on <a href="https://winnerscience.com">Winner Science</a>.</p>]]></description>
										<content:encoded><![CDATA[<p style="text-align: justify;">As we have already derived the <a title="London equations" href="https://winnerscience.com/superconductivity/london-equations-in-superconductors-derivation-and-discussion/">London equations</a> in last article. Now let us</p>
<p style="text-align: justify;"><strong>explain the flux penetration (Meissner effect) from London equations:</strong></p>
<p style="text-align: justify;">To explain Meissner effect from London equations consider the differential form of Ampere’s circuital law:</p>
<p style="text-align: justify;">del x B = µ<sub>o</sub>J<sub>s</sub></p>
<p style="text-align: justify;">where B is magnetic flux density and J<sub>s</sub> is current density</p>
<p style="text-align: justify;">Take curl on both sides of above equation</p>
<p style="text-align: justify;">del x (del x B) = µ<sub>o </sub>(del x J<sub>s</sub>)                                                     (5)</p>
<p style="text-align: justify;">As del x (del  x B)= del(del.B) &#8211; del<sup>2</sup>B</p>
<p style="text-align: justify;">Put above equation and <a title="London second equation (equation 4 is derived in last article)" href="https://winnerscience.com/superconductivity/london-equations-in-superconductors-derivation-and-discussion/">London second equation (equation 4 is derived in last article)</a> in equation (5), we get</p>
<p style="text-align: justify;">del(del.B) &#8211; del<sup>2</sup>B = -[( µ<sub>o</sub> n<sub>s</sub>e<sup>2</sup>(B)/m]</p>
<p style="text-align: justify;">But del.B = 0 (Maxwell’s second equation or Gauss law for magnetism)</p>
<p style="text-align: justify;">Therefore above equation becomes</p>
<p style="text-align: justify;">del<sup>2</sup>B = [( µ<sub>o</sub> n<sub>s</sub>e<sup>2</sup>(B)/m]                                                            (6)</p>
<p style="text-align: justify;">del<sup>2</sup>B = B/λ<sub>l</sub><sup>2 </sup>(7)</p>
<p style="text-align: justify;">where λ<sub>l</sub><sup>2</sup> = m/ µ<sub>o</sub> n<sub>s</sub>e<sup>2</sup></p>
<p style="text-align: justify;">or λ<sub>l</sub> = (m/ µ<sub>o</sub> n<sub>s</sub>e<sup>2</sup>)<sup>1/2</sup></p>
<p style="text-align: justify;">where λ<sub>l</sub> is known as London’s penetration depth and it has units of length.</p>
<p style="text-align: justify;">The solution of differential equation (7) is</p>
<p style="text-align: justify;">B = B(0)e<sup>-x/ λ</sup><sub>l</sub> (8)</p>
<p style="text-align: justify;">Where B(0) is the field at the surface and x is the depth inside the superconductor.<span id="more-2475"></span></p>
<p style="text-align: justify;">The equation (8) shows that a uniform magnetic field equal to zero can not exist in a superconductor, which is <a title="Meissner effect" href="https://winnerscience.com/superconductivity/superconductors-critical-temperature-critical-magnetic-field-and-meissner-effect/">Meissner effect</a>. In the pure superconducting state the only field allowed in the exponentially decreasing field as the flux penetrated from external surface and it is given by equation (8) (Refer figure).</p>
<p style="text-align: justify;"><a rel="attachment wp-att-2476" href="https://winnerscience.com/superconductivity/london-equations-explanation-of-flux-penetration/attachment/fig-london-penetration-depth/"><img decoding="async" class="aligncenter size-full wp-image-2476" title="Fig-London penetration depth" src="https://winnerscience.com/wp-content/uploads/2011/10/Fig-London-penetration-depth.png" alt="" width="250" height="175" /></a>Suppose x = λ<sub>l</sub></p>
<p style="text-align: justify;">Then equation (8) becomes</p>
<p style="text-align: justify;">B = B(0)/e</p>
<p style="text-align: justify;"><strong>Definition of London penetration depth</strong>: The London penetration depth is the distance inside the surface of a superconductor at which the magnetic field reduces to 1/e times its value at the surface.</p>
<p style="text-align: justify;">The London penetration depth depends strongly on the temperature and becomes much larger as T approaches <a title="critical temperature" href="https://winnerscience.com/superconductivity/superconductors-critical-temperature-critical-magnetic-field-and-meissner-effect/">critical temperature</a> Tc. The relation is</p>
<p style="text-align: justify;">λ<sub>l</sub>(T)/ λ<sub>l</sub>(0)= [1 – T/T<sub>c</sub>)<sup>4</sup>]<sup>-1/2</sup></p>
<p style="text-align: justify;">where λ<sub>l</sub>(T) and λ<sub>l</sub>(0) are the London penetration depths at temperature T kelvin and 0 k respectively.</p>
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