Metrical approach to geometry and discrete space-time geometry

Yuri A. Rylov

Institute for Problems in Mechanics, Russian Academy of Sciences,

101-1, Vernadskii Ave., Moscow, 119526, Russia.

email: rylov@ipmnet.ru

Web site: http://rsfq1.physics.sunysb.edu/~rylov/yrylov.htm

or mirror Web site: http://www.ipmnet.ru/~rylov/yrylov.htm

Updated December 8, 2011

Metric approach to geometry admits one to construct a physical geometry, i.e. geometry which is described completely in terms and only in terms of the distance function \rho , or in terms of the world function  \sigma =0.5\rho ^{2}. A discrete geometry is a special case of physical geometry, when there exist an elementary length \lambda _{0} and all distances in the discrete geometry are larger, than the elementary length. A discrete geometry is obtained as a generalization of the proper Euclidean geometry. To produce such a generalization, a logical reloading in the description of the Euclidean geometry is to be produced. It means that the Euclidean  geometry begins to be described in terms of the world function and only in terms of the world function. Such a description contains general geometric relations, which are valid in all physical geometries, and special relations, describing properties of the Euclidean world function. Replacing the Euclidean world function \sigma _{\mathrm{E}} by the world function \sigma _{\mathrm{d}} of the discrete geometry in all general geometric relations and ignoring special relations, one obtains general relations for the discrete geometry. As far as the form of  \sigma _{\mathrm{d}} is supposed to be known, the special relations for the discrete geometry are not needed

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