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Difference between revisions of "Quasi-Euclidean space"

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A <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/q/q076/q076490/q0764901.png" />-dimensional space in which each direction given at a point of it can be included in a field the directions of which can be transferred parallelly along any path (that is, a quasi-Euclidean space admits an absolute parallelism). The geodesic lines of a quasi-Euclidean space are partitioned into <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/q/q076/q076490/q0764902.png" /> families of vector lines of fields of absolutely parallel directions, where each such family forms with three others a constant [[Cross ratio|cross ratio]]:
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A $2$-dimensional space in which each direction given at a point of it can be included in a field the directions of which can be transferred parallelly along any path (that is, a quasi-Euclidean space admits an absolute parallelism). The geodesic lines of a quasi-Euclidean space are partitioned into $\infty^1$ families of vector lines of fields of absolutely parallel directions, where each such family forms with three others a constant [[Cross ratio|cross ratio]]:
  
<table class="eq" style="width:100%;"> <tr><td valign="top" style="width:94%;text-align:center;"><img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/q/q076/q076490/q0764903.png" /></td> </tr></table>
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$$\frac{k-k_1}{k_2-k}:\frac{k_3-k_1}{k_2-k_3}=\text{const},$$
  
where <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/q/q076/q076490/q0764904.png" /> is the angular direction coefficient. Each family of geodesics is defined in terms of three constants by a first-order equation:
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where $k=du^2/du^1$ is the angular direction coefficient. Each family of geodesics is defined in terms of three constants by a first-order equation:
  
<table class="eq" style="width:100%;"> <tr><td valign="top" style="width:94%;text-align:center;"><img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/q/q076/q076490/q0764905.png" /></td> </tr></table>
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$$\frac{a_pdu^p}{b_qdu^q}=\text{const}.$$
  
 
====References====
 
====References====

Latest revision as of 15:03, 1 May 2014

A $2$-dimensional space in which each direction given at a point of it can be included in a field the directions of which can be transferred parallelly along any path (that is, a quasi-Euclidean space admits an absolute parallelism). The geodesic lines of a quasi-Euclidean space are partitioned into $\infty^1$ families of vector lines of fields of absolutely parallel directions, where each such family forms with three others a constant cross ratio:

$$\frac{k-k_1}{k_2-k}:\frac{k_3-k_1}{k_2-k_3}=\text{const},$$

where $k=du^2/du^1$ is the angular direction coefficient. Each family of geodesics is defined in terms of three constants by a first-order equation:

$$\frac{a_pdu^p}{b_qdu^q}=\text{const}.$$

References

[1] A.P. Norden, "Spaces with an affine connection" , Nauka , Moscow-Leningrad (1976) (In Russian)


Comments

References

[a1] B.A. [B.A. Rozenfel'd] Rosenfel'd, "A history of non-euclidean geometry" , Springer (1988) (Translated from Russian)
How to Cite This Entry:
Quasi-Euclidean space. Encyclopedia of Mathematics. URL: http://encyclopediaofmath.org/index.php?title=Quasi-Euclidean_space&oldid=17183
This article was adapted from an original article by A.B. Ivanov (originator), which appeared in Encyclopedia of Mathematics - ISBN 1402006098. See original article