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&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{Electromagnetism|cTopic=Magnetostatics}}&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Magnetostatics&amp;#039;&amp;#039;&amp;#039; is the study of [[magnetic field]]s in systems where the [[electric currents|currents]] are steady (not changing with time). It is the magnetic analogue of [[electrostatic]]s, where the [[electric charge|charges]] are stationary. The magnetization need not be static; the equations of magnetostatics can be used to predict fast [[Magnetization reversal|magnetic switching]] events that occur on time scales of nanoseconds or less.&amp;lt;ref name=Hiebert&amp;gt;{{harvnb|Hiebert|Ballentine|Freeman|2002}}&amp;lt;/ref&amp;gt; Magnetostatics is even a good approximation when the currents are not static &amp;amp;mdash; as long as the currents do not alternate rapidly. Magnetostatics is widely used in applications of [[micromagnetics]] such as models of [[magnetic recording]] devices.&lt;br /&gt;
&lt;br /&gt;
==Applications==&lt;br /&gt;
===Magnetostatics as a special case of Maxwell&amp;#039;s equations===&lt;br /&gt;
Starting from [[Maxwell&amp;#039;s equations]] and assuming that charges are either fixed or move as a steady current &amp;lt;math&amp;gt;\scriptstyle\vec{J}&amp;lt;/math&amp;gt;, the equations separate into two equations for the [[electric field]] (see [[electrostatics]]) and two for the [[magnetic field]].&amp;lt;ref name=Feynman&amp;gt;{{harvnb|Feynman|Leighton|Sands|2006}}&amp;lt;/ref&amp;gt; The fields are independent of time and each other. The magnetostatic equations, in both differential and integral forms, are shown in the table below.&lt;br /&gt;
&lt;br /&gt;
{| class=&amp;quot;wikitable&amp;quot;&lt;br /&gt;
|- style=&amp;quot;background-color: #aaddcc;&amp;quot;&lt;br /&gt;
! Name&lt;br /&gt;
! [[Partial differential equation|Partial differential]] form&lt;br /&gt;
! [[Integral]] form&lt;br /&gt;
|-&lt;br /&gt;
| [[Gauss&amp;#039;s law for magnetism]]:&lt;br /&gt;
| &amp;lt;math&amp;gt;\vec{\nabla} \cdot \vec{B} = 0&amp;lt;/math&amp;gt;    &lt;br /&gt;
| &amp;lt;math&amp;gt;\oint_S \vec{B} \cdot \mathrm{d}\vec{S} = 0&amp;lt;/math&amp;gt;&lt;br /&gt;
|-&lt;br /&gt;
| [[Ampère&amp;#039;s law]]:&lt;br /&gt;
| &amp;lt;math&amp;gt;\vec{\nabla} \times \vec{H} = \vec{J}&amp;lt;/math&amp;gt;&lt;br /&gt;
| &amp;lt;math&amp;gt;\oint_C \vec{H} \cdot \mathrm{d}\vec{l} = I_{\mathrm{enc}}&amp;lt;/math&amp;gt;&lt;br /&gt;
|}&lt;br /&gt;
The first integral is over a surface &amp;lt;math&amp;gt;S&amp;lt;/math&amp;gt; with oriented surface element &amp;lt;math&amp;gt;\scriptstyle d\vec{S}&amp;lt;/math&amp;gt;. The second is a line integral around a closed loop &amp;lt;math&amp;gt;C&amp;lt;/math&amp;gt; with line element &amp;lt;math&amp;gt;\scriptstyle\vec{l}&amp;lt;/math&amp;gt;. The current going through the loop is &amp;lt;math&amp;gt;\scriptstyle I_\text{enc}&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
The quality of this approximation may be guessed by comparing the above equations with the full version of [[Maxwell&amp;#039;s equations]] and considering the importance of the terms that have been removed. Of particular significance is the comparison of the &amp;lt;math&amp;gt;\scriptstyle \vec{J}&amp;lt;/math&amp;gt; term against the &amp;lt;math&amp;gt;\scriptstyle \partial \vec{D} / \partial t&amp;lt;/math&amp;gt; term. If the &amp;lt;math&amp;gt;\scriptstyle \vec{J}&amp;lt;/math&amp;gt; term is substantially larger, then the smaller term may be ignored without significant loss of accuracy.&lt;br /&gt;
&lt;br /&gt;
===Re-introducing Faraday&amp;#039;s law===&lt;br /&gt;
A common technique is to solve a series of magnetostatic problems at incremental time steps and then use these solutions to approximate the term &amp;lt;math&amp;gt;\scriptstyle \partial \vec{B} / \partial t&amp;lt;/math&amp;gt;. Plugging this result into [[Faraday&amp;#039;s law of induction|Faraday&amp;#039;s Law]] finds a value for &amp;lt;math&amp;gt;\scriptstyle \vec{E}&amp;lt;/math&amp;gt; (which had previously been ignored). This method is not a true solution of [[Maxwell&amp;#039;s equations]] but can provide a good approximation for slowly changing fields.{{Citation needed|date=October 2010}}&lt;br /&gt;
&lt;br /&gt;
==Solving for the magnetic field==&lt;br /&gt;
===Current sources===&lt;br /&gt;
&lt;br /&gt;
If all currents in a system are known (&amp;#039;&amp;#039;i.e.,&amp;#039;&amp;#039; if a complete description of &amp;lt;math&amp;gt;\scriptstyle \vec{J}&amp;lt;/math&amp;gt; is available) then &lt;br /&gt;
the magnetic field can be determined from the currents by the [[Biot-Savart law|Biot-Savart equation]]:&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt;\vec{B}= \frac{\mu_{0}}{4\pi}I \int{\frac{\mathrm{d}\vec{l} \times \hat{r}}{r^2}}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
This technique works well for problems where the medium is a [[vacuum]] or [[air]] or some similar material with a [[Permeability (electromagnetism)|relative permeability]] of 1. This includes Air core inductors and Air core transformers. One advantage of this technique is that a complex coil geometry can be integrated in sections, or for a very difficult geometry [[numerical integration]] may be used. Since this equation is primarily used to solve [[linear]] problems, the complete answer will be a sum of the integral of each component section.&lt;br /&gt;
&lt;br /&gt;
For problems where the dominant magnetic material is a highly permeable [[magnetic core]] with relatively small air gaps, a [[magnetic circuit]] approach is useful. When the air gaps are large in comparison to the [[magnetic circuit]] length, [[magnetic fringing|fringing]] becomes significant and usually requires a [[finite element]] calculation. The [[finite element]] calculation uses a modified form of the magnetostatic equations above in order to calculate [[magnetic potential]]. The value of &amp;lt;math&amp;gt;\scriptstyle \vec{B}&amp;lt;/math&amp;gt; can be found from the [[magnetic potential]].&lt;br /&gt;
&lt;br /&gt;
The magnetic field can be derived from the [[Magnetic vector potential|vector potential]]. Since the divergence of the magnetic flux density is always zero,&lt;br /&gt;
::&amp;lt;math&amp;gt; \vec{B} = \nabla \times \vec{A}, &amp;lt;/math&amp;gt;&lt;br /&gt;
and the relation of the vector potential to current is:&lt;br /&gt;
::&amp;lt;math&amp;gt; \vec{A} = \frac{\mu_{0}}{4\pi} \int{ \frac{\vec{J} } {r} dV} &amp;lt;/math&amp;gt;&lt;br /&gt;
where &amp;lt;math&amp;gt;\scriptstyle \vec{J} &amp;lt;/math&amp;gt; is the [[current density]].&lt;br /&gt;
&lt;br /&gt;
===Magnetization===&lt;br /&gt;
&lt;br /&gt;
{{Further2|[[Demagnetizing field]] and [[Micromagnetics]]}}&lt;br /&gt;
Strongly magnetic materials (&amp;#039;&amp;#039;i.e.,&amp;#039;&amp;#039; [[Ferromagnetic]], [[Ferrimagnetic]] or [[Paramagnetic]]) have a [[magnetization]] that is primarily due to [[spin (physics)|electron spins]]. In such materials the magnetization must be explicitly included using the relation&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \vec{B} = \mu_0(\vec{M}+\vec{H}).&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Except in metals, electric currents can be ignored. Then Ampère&amp;#039;s law is simply&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \nabla\times\vec{H} = 0.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
This has the general solution&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \vec{H} = -\nabla U, &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;U&amp;lt;/math&amp;gt; is a scalar [[potential]]. Substituting this in Gauss&amp;#039;s law gives&lt;br /&gt;
&lt;br /&gt;
:&amp;lt;math&amp;gt; \nabla^2 U = \nabla\cdot\vec{M}.&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
Thus, the divergence of the magnetization, &amp;lt;math&amp;gt;\scriptstyle \nabla\cdot\vec{M},&amp;lt;/math&amp;gt; has a role analogous to the electric charge in electrostatics &amp;lt;ref&amp;gt;{{harvnb|Aharoni|1996}}&amp;lt;/ref&amp;gt; and is often referred to as an effective charge density &amp;lt;math&amp;gt;\rho_M&amp;lt;/math&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
The vector potential method can also be employed with an effective current density&lt;br /&gt;
::&amp;lt;math&amp;gt; \vec{J_M} = \nabla \times \vec{M}. &amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
* [[Darwin Lagrangian]]&lt;br /&gt;
&lt;br /&gt;
==Notes==&lt;br /&gt;
{{Reflist|2}}&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
{{Refbegin}}&lt;br /&gt;
*{{cite book&lt;br /&gt;
|last = Aharoni&lt;br /&gt;
|first = Amikam&lt;br /&gt;
|author-link=Amikam Aharoni&lt;br /&gt;
|title=Introduction to the Theory of Ferromagnetism&lt;br /&gt;
|publisher=[[Clarendon Press]]&lt;br /&gt;
|year = 1996&lt;br /&gt;
|isbn=0-19-851791-2&lt;br /&gt;
|url=http://www.oup.com/us/catalog/general/subject/Physics/ElectricityMagnetism/?view=usa&amp;amp;ci=9780198508090&lt;br /&gt;
}}&lt;br /&gt;
*{{Cite book&lt;br /&gt;
|last1 = Feynman&lt;br /&gt;
|first1 = Richard P.&lt;br /&gt;
|author-link = Richard Feynman&lt;br /&gt;
|first2 = Robert B.&lt;br /&gt;
|last2 = Leighton&lt;br /&gt;
|author2-link = Robert B. Leighton&lt;br /&gt;
|first3 = Matthew&lt;br /&gt;
|last3 = Sands&lt;br /&gt;
|author3-link = Matthew Sands&lt;br /&gt;
|title = [[The Feynman Lectures on Physics]]&lt;br /&gt;
|volume = 2&lt;br /&gt;
|year = 2006&lt;br /&gt;
|isbn = 0-8053-9045-6&lt;br /&gt;
|ref=harv&lt;br /&gt;
}}&lt;br /&gt;
*{{cite article&lt;br /&gt;
|last=Hiebert&lt;br /&gt;
|first=W&lt;br /&gt;
|last2=Ballentine&lt;br /&gt;
|first2=G&lt;br /&gt;
|last3=Freeman&lt;br /&gt;
|first3=M&lt;br /&gt;
|title=Comparison of experimental and numerical micromagnetic dynamics in coherent precessional switching and modal oscillations&lt;br /&gt;
|journal = [[Physical Review B]]&lt;br /&gt;
|volume=65&lt;br /&gt;
|number=14&lt;br /&gt;
|pages=140404&lt;br /&gt;
|year=2002&lt;br /&gt;
|doi=10.1103/PhysRevB.65.140404&lt;br /&gt;
|ref=harv&lt;br /&gt;
}}&lt;br /&gt;
{{Refend}}&lt;br /&gt;
&lt;br /&gt;
[[Category:Electric and magnetic fields in matter]]&lt;br /&gt;
[[Category:Magnetostatics]]&lt;br /&gt;
[[Category:Potentials]]&lt;/div&gt;</summary>
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