"Special relativity"의 두 판 사이의 차이

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4번째 줄: 4번째 줄:
 
*  examples<br>
 
*  examples<br>
 
** space-time (ct,x,y,z)
 
** space-time (ct,x,y,z)
**  
+
** electromagnetic field
 
*  
 
*  
  
83번째 줄: 83번째 줄:
 
* http://en.wikipedia.org/wiki/Einstein_field_equations<br>
 
* http://en.wikipedia.org/wiki/Einstein_field_equations<br>
 
* http://en.wikipedia.org/wiki/Solutions_of_the_Einstein_field_equations<br>
 
* http://en.wikipedia.org/wiki/Solutions_of_the_Einstein_field_equations<br>
* http://en.wikipedia.org/wiki/Lorentz_covariant<br>
+
*  <br>http://en.wikipedia.org/wiki/Lorentz_covariant<br>
*  <br>[http://en.wikipedia.org/wiki/Four-vector ]http://en.wikipedia.org/wiki/Four-vector<br>
+
* [http://en.wikipedia.org/wiki/Lorentz_covariant ]http://en.wikipedia.org/wiki/Four-vector<br>
 
* http://en.wikipedia.org/wiki/
 
* http://en.wikipedia.org/wiki/
 
* http://www.scholarpedia.org/
 
* http://www.scholarpedia.org/

2010년 5월 15일 (토) 11:33 판

four-vector 
  • can be transformed by Lorentz transoformation
  • examples
    • space-time (ct,x,y,z)
    • electromagnetic field
  •  

 

 

review of Maxwell's equation

 

 

Lorentz transformation and Maxwell's equation

 

 

 

Vacuum field equation and gravitational field equation
  • gravitational potentail satisfies the following equation
    \(\nabla^2 \Phi = - 4 \pi G \rho\)

 

 

energy-momentum tensor
  • describe the densities and flows of energy and momentum

 

 

 

relativistic Vacuum field equation

 

 

 

relativistic matter field equation
  • Einstein field equation
    \(R_{\mu \nu} - {1 \over 2}g_{\mu \nu}\,R + g_{\mu \nu} \Lambda = {8 \pi G \over c^4} T_{\mu \nu}\)
    where \(\Lambda\) is the cosmological constant

 

 

history

 

 

related items

 

 

encyclopedia

 

 

books

[[4909919|]]

 

 

articles

 

 

question and answers(Math Overflow)

 

 

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