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alternate case: coframe
Frame fields in general relativity
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defined on the manifold can be expressed using the frame field and its dual coframe field. Frame fields were introduced into general relativity by Albert EinsteinGauge gravitation theory (1,155 words) [view diff] exact match in snippet view article find links to article
were considered as those of the translation gauge group, and a tetrad (coframe) field was identified with the translation part of an affine connectionSchwarzschild coordinates (4,089 words) [view diff] exact match in snippet view article find links to article
Cartan's exterior calculus method. First, we read off the line element a coframe field, σ 0 = − a ( r ) d t {\displaystyle \sigma ^{0}=-a(r)\,dt} σ 1 =Isotropic coordinates (1,179 words) [view diff] exact match in snippet view article find links to article
Cartan's exterior calculus method. First, we read off the line element a coframe field, σ 0 = − a ( r ) d t {\displaystyle \sigma ^{0}=-a(r)\,dt} σ 1 =Gaussian polar coordinates (365 words) [view diff] exact match in snippet view article find links to article
fluids Schwarzschild coordinates Isotropic coordinates Frame fields in general relativity for more about frame fields and coframe fields. v t e v t eVan Stockum dust (2,067 words) [view diff] exact match in snippet view article find links to article
To prevent misunderstanding, we should emphasize that taking the dual coframe σ 0 = d t + h ( r ) r d φ , σ 1 = 1 f ( r ) d z , σ 2 = 1 f ( r ) d rMaurer–Cartan form (1,992 words) [view diff] exact match in snippet view article find links to article
Kronecker delta. Then Ei is a Maurer–Cartan frame, and θi is a Maurer–Cartan coframe. Since Ei is left-invariant, applying the Maurer–Cartan form to it simplyTeleparallelism (2,612 words) [view diff] exact match in snippet view article find links to article
coefficients) in this global basis. Here ωk is the dual global basis (or coframe) defined by ωi(Xj) = δi j. This is what usually happens in Rn, in any affinePoincaré disk model (4,060 words) [view diff] exact match in snippet view article find links to article
(}1-|\mathbf {x} |^{2}{\Bigr )}{\frac {\partial }{\partial x^{i}}},} with dual coframe of 1-forms θ i = 2 1 − | x | l 2 d x i . {\displaystyle \theta ^{i}={\fracTorsion tensor (4,375 words) [view diff] exact match in snippet view article find links to article
the following manner. Let θ i {\displaystyle \theta ^{i}} be a parallel coframe along γ {\displaystyle \gamma } , and let x i {\displaystyle x^{i}} bePolar coordinate system (6,702 words) [view diff] exact match in snippet view article find links to article
e_{\theta }={\frac {1}{r}}{\frac {\partial }{\partial \theta }},} with dual coframe e r = d r , e θ = r d θ . {\displaystyle e^{r}=dr,\quad e^{\theta }=rd\thetaMathematics of general relativity (7,044 words) [view diff] exact match in snippet view article find links to article
metric tensor takes on a particularly convenient form. When allied with coframe fields, frame fields provide a powerful tool for analysing spacetimes andBorn coordinates (6,357 words) [view diff] exact match in snippet view article find links to article
Lorentzian manifold by a stationary timelike congruence. If we adopt the coframe θ 1 ^ = d z , θ 2 ^ = d r , θ 3 ^ = r d ϕ 1 − ω 2 r 2 {\displaystyle \thetaRindler coordinates (7,773 words) [view diff] exact match in snippet view article find links to article
{\displaystyle c=1} and α = 1 {\displaystyle \alpha =1} , it is natural to take the coframe field d σ 0 = x d t , d σ 1 = d x , d σ 2 = d y , d σ 3 = d z {\displaystyle