"Einstein field equation"의 두 판 사이의 차이

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<h5>introduction</h5>
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==introduction</h5>
  
 
* prerequiste : Riemann tensor, the Ricci tensor, and the Ricci scalar
 
* prerequiste : Riemann tensor, the Ricci tensor, and the Ricci scalar
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<h5>history</h5>
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==history</h5>
  
 
* http://www.google.com/search?hl=en&tbs=tl:1&q=
 
* http://www.google.com/search?hl=en&tbs=tl:1&q=
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<h5>related items</h5>
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==related items</h5>
  
 
* [[cosmological constant]]
 
* [[cosmological constant]]

2012년 10월 28일 (일) 13:58 판

==introduction

  • prerequiste : Riemann tensor, the Ricci tensor, and the Ricci scalar
  • relativistic matter 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 \(R_{\mu \nu}\) is the Ricci curvature tensor, \(R\) the Ricci scalar curvature, \(\Lambda\) is the cosmological constant, \(T_{\mu \nu}\) momentum-energy tensor

 

 

steps to solve an Einstein equation
  • consider a metric, for example
    \(ds^2=-dt^2+e^{2b(t,r)}dr^2+R(t,r)d\phi^2\)
    where b, R are unknown functions
  • find the components of the curvature tensor
  • find the components of the Einstein tensor

 

 

Einstein-Hilbert action
  • Einstein-Hilbert action
    \(S= - {1 \over 2\kappa}\int R \sqrt{-g} \, d^4x \\)
    \(\kappa = {8 \pi G \over c^4} \)

 

 

equation of motion

 

 

solutions example : Schwarzschild black hole

 

 

 

solutions example : gravitational wave
  • Einstein
  • eventually led to the graviton idea\

 

 

==history

 

 

==related items

 

 

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