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Nonmetricity tensor

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Constant derivative of the metric tensor

In mathematics, the nonmetricity tensor in differential geometry is the covariant derivative of the metric tensor.[1] [2] It is therefore a tensor field of order three. It vanishes for the case of Riemannian geometry and can be used to study non-Riemannian spacetimes.[3]

Definition

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By components, it is defined as follows.[1]

Q μ α β = μ g α β {\displaystyle Q_{\mu \alpha \beta }=\nabla _{\mu }g_{\alpha \beta }} {\displaystyle Q_{\mu \alpha \beta }=\nabla _{\mu }g_{\alpha \beta }}

It measures the rate of change of the components of the metric tensor along the flow of a given vector field, since

μ μ {\displaystyle \nabla _{\mu }\equiv \nabla _{\partial _{\mu }}} {\displaystyle \nabla _{\mu }\equiv \nabla _{\partial _{\mu }}}

where { μ } μ = 0 , 1 , 2 , 3 {\displaystyle \{\partial _{\mu }\}_{\mu =0,1,2,3}} {\displaystyle \{\partial _{\mu }\}_{\mu =0,1,2,3}} is the coordinate basis of vector fields of the tangent bundle, in the case of having a 4-dimensional manifold.

Relation to connection

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We say that a connection Γ {\displaystyle \Gamma } {\displaystyle \Gamma } is compatible with the metric when its associated covariant derivative of the metric tensor (call it Γ {\displaystyle \nabla ^{\Gamma }} {\displaystyle \nabla ^{\Gamma }}, for example) is zero, i.e.

μ Γ g α β = 0. {\displaystyle \nabla _{\mu }^{\Gamma }g_{\alpha \beta }=0.} {\displaystyle \nabla _{\mu }^{\Gamma }g_{\alpha \beta }=0.}

If the connection is also torsion-free (i.e. totally symmetric) then it is known as the Levi-Civita connection, which is the only one without torsion and compatible with the metric tensor. If we see it from a geometrical point of view, a non-vanishing nonmetricity tensor for a metric tensor g {\displaystyle g} {\displaystyle g} implies that the modulus of a vector defined on the tangent bundle to a certain point p {\displaystyle p} {\displaystyle p} of the manifold, changes when it is evaluated along the direction (flow) of another arbitrary vector.

References

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  1. ^ a b Hehl, Friedrich W.; McCrea, J. Dermott; Mielke, Eckehard W.; Ne'eman, Yuval (July 1995). "Metric-affine gauge theory of gravity: field equations, Noether identities, world spinors, and breaking of dilation invariance". Physics Reports . 258 (1–2): 1–171. arXiv:gr-qc/9402012 . Bibcode:1995PhR...258....1H. doi:10.1016/0370-1573(94)00111-F. S2CID 119346282.
  2. ^ Kopeikin, Sergei; Efroimsky, Michael; Kaplan, George (2011), Relativistic Celestial Mechanics of the Solar System , John Wiley & Sons, p. 242, ISBN 9783527408566 .
  3. ^ Puntigam, Roland A.; Lämmerzahl, Claus; Hehl, Friedrich W. (May 1997). "Maxwell's theory on a post-Riemannian spacetime and the equivalence principle". Classical and Quantum Gravity . 14 (5): 1347–1356. arXiv:gr-qc/9607023 . Bibcode:1997CQGra..14.1347P. doi:10.1088/0264-9381/14/5/033. S2CID 44439510.
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