Difference between revisions of "Maxwell's Equations"

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== In Free Space ==
 
== In Free Space ==
Gauss' Law:
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<math>\boldsymbol{\nabla \cdot E} = 0 </math>
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These are the Maxwell's Equations we will be using to solve for regions "I" and "II" in our approximation of the Michelson interferometer.
Maxwell's "Baby":
+
 
<math>\boldsymbol{\nabla \cdot B} = 0</math>
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{|align=center
 +
|Gauss' Law:
 +
|Gauss' Law for Magnetism:
 +
|-
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|<math>\boldsymbol{\nabla \cdot E} = 0 </math>  
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|<math>\boldsymbol{\nabla \cdot B} = 0</math>
 +
|-
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|height="20"|&nbsp;||&nbsp;
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|-
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|Faradays's Law:
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|Ampere's Law:
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|-
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|width="400"|<math>\boldsymbol{\nabla \times E} + \frac{\partial \boldsymbol{B}}{\partial t}= 0</math>
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|width="400"|<math>\boldsymbol{\nabla \times B} - \mu_0\epsilon_0\frac{\partial \boldsymbol{E}}{\partial t}= 0 </math>
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|}
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 +
== In the Presence of Charges and Dielectric Media ==
 +
 
 +
{|align=center
 +
|Gauss' Law:
 +
|Gauss' Law for Magnetism:
 +
|-
 +
|<math>\boldsymbol{\nabla \cdot D} = \rho </math>
 +
|<math>\boldsymbol{\nabla \cdot B} = 0</math>  
 +
|-
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|height="20"|&nbsp;||&nbsp;
 +
|-
 +
|Faradays's Law:
 +
|Ampere's Law:
 +
|-
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|width="400"|<math>\boldsymbol{\nabla \times E} + \frac{\partial \boldsymbol{B}}{\partial t}= 0</math>
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|width="400"|<math>\boldsymbol{\nabla \times H} - \frac{\partial \boldsymbol{D}}{\partial t}= \boldsymbol{j} </math>
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|}
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Where <math>\boldsymbol{D} = \epsilon_0 \boldsymbol{E}</math> and <math>\boldsymbol{B} = \mu_0 \boldsymbol{H}</math>.

Latest revision as of 02:52, 6 April 2007

In Free Space

These are the Maxwell's Equations we will be using to solve for regions "I" and "II" in our approximation of the Michelson interferometer.

Gauss' Law: Gauss' Law for Magnetism:
   
Faradays's Law: Ampere's Law:

In the Presence of Charges and Dielectric Media

Gauss' Law: Gauss' Law for Magnetism:
   
Faradays's Law: Ampere's Law:


Where and .