"Einstein field equation"의 두 판 사이의 차이
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where R_{\mu \nu}\, is the Ricci curvature tensor, R\, the scalar curvature,, <math>\Lambda</math> is the [[cosmological constant]] | where R_{\mu \nu}\, is the Ricci curvature tensor, R\, the scalar curvature,, <math>\Lambda</math> is the [[cosmological constant]] | ||
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+ | <h5 style="line-height: 2em; margin: 0px;">Einstein-Hilb</h5> | ||
2011년 9월 3일 (토) 07:35 판
introduction
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 scalar curvature,, \(\Lambda\) is the cosmological constant
Einstein-Hilb
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encyclopedia
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- [1]http://en.wikipedia.org/wiki/Einstein_field_equations
- http://en.wikipedia.org/wiki/Riemann_curvature_tensor
- http://en.wikipedia.org/wiki/Ricci_curvature
- http://en.wikipedia.org/wiki/Scalar_curvature[2]
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- Princeton companion to mathematics(Companion_to_Mathematics.pdf)
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