To install click the Add extension button. That's it.

The source code for the WIKI 2 extension is being checked by specialists of the Mozilla Foundation, Google, and Apple. You could also do it yourself at any point in time.

4,5
Kelly Slayton
Congratulations on this excellent venture… what a great idea!
Alexander Grigorievskiy
I use WIKI 2 every day and almost forgot how the original Wikipedia looks like.
Live Statistics
English Articles
Improved in 24 Hours
Added in 24 Hours
Languages
Recent
Show all languages
What we do. Every page goes through several hundred of perfecting techniques; in live mode. Quite the same Wikipedia. Just better.
.
Leo
Newton
Brights
Milds

Nonmetricity tensor

From Wikipedia, the free encyclopedia

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

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

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

where is the coordinate basis of vector fields of the tangent bundle, in the case of having a 4-dimensional manifold.

Relation to connection

We say that a connection is compatible with the metric when its associated covariant derivative of the metric tensor (call it , for example) is zero, i.e.

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 implies that the modulus of a vector defined on the tangent bundle to a certain point of the manifold, changes when it is evaluated along the direction (flow) of another arbitrary vector.

References

  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.

External links


This page was last edited on 24 July 2023, at 09:07
Basis of this page is in Wikipedia. Text is available under the CC BY-SA 3.0 Unported License. Non-text media are available under their specified licenses. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc. WIKI 2 is an independent company and has no affiliation with Wikimedia Foundation.