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The Einstein field equations (EFE) may be written in the form:[5][1]
{\displaystyle R_{\mu \nu }-{\tfrac {1}{2}}Rg_{\mu \nu }+\Lambda g_{\mu \nu }={\frac {8\pi G}{c^{4}}}T_{\mu \nu }}{\displaystyle R_{\mu \nu }-{\tfrac {1}{2}}Rg_{\mu \nu }+\Lambda g_{\mu \nu }={\frac {8\pi G}{c^{4}}}T_{\mu \nu }}
EFE on a wall in Leiden
where Rμν is the Ricci curvature tensor, R is the scalar curvature, gμν is the metric tensor, Λ is the cosmological constant, G is Newton's gravitational constant, c is the speed of light in vacuum, and Tμν is the stress–energy tensor.
The EFE is a tensor equation relating a set of symmetric 4 × 4 tensors. Each tensor has 10 independent components. The four Bianchi identities reduce the number of independent equations from 10 to 6, leaving the metric with four gauge fixing degrees of freedom, which correspond to the freedom to choose a coordinate system.
Although the Einstein field equations were initially formulated in the context of a four-dimensional theory, some theorists have explored their consequences in n dimensions.[6] The equations in contexts outside of general relativity are still referred to as the Einstein field equations. The vacuum field equations (obtained when T is identically zero) define Einstein manifolds.
Despite the simple appearance of the equations they are actually quite complicated. Given a specified distribution of matter and energy in the form of a stress–energy tensor, the EFE are understood to be equations for the metric tensor gμν, as both the Ricci tensor and scalar curvature depend on the metric in a complicated nonlinear manner. In fact, when fully written out, the EFE are a system of ten coupled, nonlinear, hyperbolic-elliptic partial differential equations.[7]
One can write the EFE in a more compact form by defining the Einstein tensor
{\displaystyle G_{\mu \nu }=R_{\mu \nu }-{\tfrac {1}{2}}Rg_{\mu \nu },}{\displaystyle G_{\mu \nu }=R_{\mu \nu }-{\tfrac {1}{2}}Rg_{\mu \nu },}
which is a sy
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6 years ago
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Fish
Temporal range: Mid Cambrian–Recent
PreЄЄOSDCPTJKPgN
Giant grouper swimming among schools of other fish
Giant grouper swimming among schools of other fish
Head-on view of a red lionfish
Head-on view of a red lionfish
Scientific classificationEdit this classification
Kingdom: Animalia
Phylum: Chordata
Clade: Olfactores
Subphylum: Vertebrata
Groups included
Jawless fish
†Armoured fish
†Spiny sharks
Cartilaginous fish
Bony fish
Ray-finned fish
Lobe-finned fish
Cladistically included but traditionally excluded taxa
Tetrapods
Fish are gill-bearing aquatic craniate animals that lack limbs with digits. They form a sister group to the tunicates, together forming the olfactores. Included in this definition are the living hagfish, lampreys, and cartilaginous and bony fish as well as various extinct related groups. Tetrapods emerged within lobe-finned fishes, so cladistically they are fish as well. However, traditionally fish are rendered paraphyletic by excluding the tetrapods (i.e., the amphibians, reptiles, birds and mammals which all descended from within the same ancestry). Because in this manner the term "fish" is defined negatively as a paraphyletic group, it is not considered a formal taxonomic grouping in systematic biology, unless it is used in the cladistic sense, including tetrapods.[1][2] The traditional term pisces (also ichthyes) is considered a typological, but not a phylogenetic classification.
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The Einstein field equations (EFE) may be written in the form:[5][1] {\displaystyle R_{\mu \nu }-{\tfrac {1}{2}}Rg_{\mu \nu }+\Lambda g_{\mu \nu }={\frac {8\pi G}{c^{4}}}T_{\mu \nu }}{\displaystyle R_{\mu \nu }-{\tfrac {1}{2}}Rg_{\mu \nu }+\Lambda g_{\mu \nu }={\frac {8\pi G}{c^{4}}}T_{\mu \nu }} EFE on a wall in Leiden where Rμν is the Ricci curvature tensor, R is the scalar curvature, gμν is the metric tensor, Λ is the cosmological constant, G is Newton's gravitational constant, c is the speed of light in vacuum, and Tμν is the stress–energy tensor. The EFE is a tensor equation relating a set of symmetric 4 × 4 tensors. Each tensor has 10 independent components. The four Bianchi identities reduce the number of independent equations from 10 to 6, leaving the metric with four gauge fixing degrees of freedom, which correspond to the freedom to choose a coordinate system. Although the Einstein field equations were initially formulated in the context of a four-dimensional theory, some theorists have explored their consequences in n dimensions.[6] The equations in contexts outside of general relativity are still referred to as the Einstein field equations. The vacuum field equations (obtained when T is identically zero) define Einstein manifolds. Despite the simple appearance of the equations they are actually quite complicated. Given a specified distribution of matter and energy in the form of a stress–energy tensor, the EFE are understood to be equations for the metric tensor gμν, as both the Ricci tensor and scalar curvature depend on the metric in a complicated nonlinear manner. In fact, when fully written out, the EFE are a system of ten coupled, nonlinear, hyperbolic-elliptic partial differential equations.[7] One can write the EFE in a more compact form by defining the Einstein tensor {\displaystyle G_{\mu \nu }=R_{\mu \nu }-{\tfrac {1}{2}}Rg_{\mu \nu },}{\displaystyle G_{\mu \nu }=R_{\mu \nu }-{\tfrac {1}{2}}Rg_{\mu \nu },} which is a sy
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Fish Temporal range: Mid Cambrian–Recent PreЄЄOSDCPTJKPgN Giant grouper swimming among schools of other fish Giant grouper swimming among schools of other fish Head-on view of a red lionfish Head-on view of a red lionfish Scientific classificationEdit this classification Kingdom: Animalia Phylum: Chordata Clade: Olfactores Subphylum: Vertebrata Groups included Jawless fish †Armoured fish †Spiny sharks Cartilaginous fish Bony fish Ray-finned fish Lobe-finned fish Cladistically included but traditionally excluded taxa Tetrapods Fish are gill-bearing aquatic craniate animals that lack limbs with digits. They form a sister group to the tunicates, together forming the olfactores. Included in this definition are the living hagfish, lampreys, and cartilaginous and bony fish as well as various extinct related groups. Tetrapods emerged within lobe-finned fishes, so cladistically they are fish as well. However, traditionally fish are rendered paraphyletic by excluding the tetrapods (i.e., the amphibians, reptiles, birds and mammals which all descended from within the same ancestry). Because in this manner the term "fish" is defined negatively as a paraphyletic group, it is not considered a formal taxonomic grouping in systematic biology, unless it is used in the cladistic sense, including tetrapods.[1][2] The traditional term pisces (also ichthyes) is considered a typological, but not a phylogenetic classification.
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