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One conceivable hypothesis on the structure of space in the microcosmos, conceived as a collection of disconnected elements in space (points) which cannot be distinguished by observations. An acceptable formalization of discrete space-time can be given in terms of topological spaces <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/d/d033/d033140/d0331401.png" /> in which the connected component of a point <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/d/d033/d033140/d0331402.png" /> is its closure <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/d/d033/d033140/d0331403.png" />, and, in a Hausdorff space <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/d/d033/d033140/d0331404.png" />, is this point itself (totally disconnected spaces). Examples of <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/d/d033/d033140/d0331405.png" /> include a discrete topological space, a rational straight line, analytic manifolds, and Lie groups over fields with ultra-metric absolute values.
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One conceivable hypothesis on the structure of space in the microcosmos, conceived as a collection of disconnected elements in space (points) which cannot be distinguished by observations. An acceptable formalization of discrete space-time can be given in terms of topological spaces $Y$ in which the connected component of a point $y\in Y$ is its closure $\bar y$, and, in a Hausdorff space $Y$, is this point itself (totally disconnected spaces). Examples of $Y$ include a discrete topological space, a rational straight line, analytic manifolds, and Lie groups over fields with ultra-metric absolute values.
  
The discrete space-time hypothesis was originally developed as a variation of a finite totally-disconnected space, in models of finite geometries on Galois fields V.A. Ambartsumyan and D.D. Ivanenko (1930) were the first to treat it in the framework of field theory (as a cubic lattice in space). In quantum theory the hypothesis of discrete space-time appeared in models in which the coordinate (momentum, etc.) space, like the spectrum of the <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/d/d033/d033140/d0331407.png" />-algebra of corresponding operators, is totally disconnected (e.g. like the spectrum of the <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/d/d033/d033140/d0331408.png" />-algebra of probability measures). It received a serious foundation in the concept of "fundamental lengths" in non-linear generalizations of electrodynamics, mesondynamics and Dirac's spinor theory, in which the constants of field action have the dimension of length, and in quantum field theory, where it is necessary to introduce all kinds of "cut-off" factors. These ideas, later in conjunction with non-local models, served as the base for the formulation of the concept of minimal domains in space in which it appears no longer possible to adopt the quantum-theoretical description of micro-objects in terms of their interaction with a macro-instrument. As a result, the space-time continuum is inacceptable for the parametrization of spatial-evolutionary relations in these domains (e.g. the Hamilton formalism in non-local theories), and their points cannot be distinguished by observation (in spaces <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/d/d033/d033140/d0331409.png" /> this may be represented as the presence of a non-Hausdorff uniform structure). The discrete space-time hypothesis was developed in the conception of the non-linear vacuum. According to this concept — under extreme conditions inside particles, and possibly also in astrophysical and cosmological singularities — the spatial characteristics may manifest themselves as dynamic characteristics of a physical system, in the models of which the spatial elements are provided with non-commutative binary operations.
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The discrete space-time hypothesis was originally developed as a variation of a finite totally-disconnected space, in models of finite geometries on Galois fields V.A. Ambartsumyan and D.D. Ivanenko (1930) were the first to treat it in the framework of field theory (as a cubic lattice in space). In quantum theory the hypothesis of discrete space-time appeared in models in which the coordinate (momentum, etc.) space, like the spectrum of the $C^*$-algebra of corresponding operators, is totally disconnected (e.g. like the spectrum of the $C^*$-algebra of probability measures). It received a serious foundation in the concept of "fundamental lengths" in non-linear generalizations of electrodynamics, mesondynamics and Dirac's spinor theory, in which the constants of field action have the dimension of length, and in quantum field theory, where it is necessary to introduce all kinds of "cut-off" factors. These ideas, later in conjunction with non-local models, served as the base for the formulation of the concept of minimal domains in space in which it appears no longer possible to adopt the quantum-theoretical description of micro-objects in terms of their interaction with a macro-instrument. As a result, the space-time continuum is inacceptable for the parametrization of spatial-evolutionary relations in these domains (e.g. the Hamilton formalism in non-local theories), and their points cannot be distinguished by observation (in spaces $Y$ this may be represented as the presence of a non-Hausdorff uniform structure). The discrete space-time hypothesis was developed in the conception of the non-linear vacuum. According to this concept — under extreme conditions inside particles, and possibly also in astrophysical and cosmological singularities — the spatial characteristics may manifest themselves as dynamic characteristics of a physical system, in the models of which the spatial elements are provided with non-commutative binary operations.
  
 
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====Comments====
 
====Comments====
Another approach to discrete space-time is to consider the set of integral solutions of the Diophantine equation <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/d/d033/d033140/d03314010.png" />, and thus to examine the group of all integral Lorentz transformations [[#References|[a1]]], [[#References|[a2]]]. For this purpose, A. Schild used spin tensors with Gaussian integer components. He proved that the spatial projections of the time-like lines joining a fixed point ( "event" ) to other lattice points are dense, and therefore the direction in which material particles can move form a dense system; that is, a particle can move in "approximately" any direction. The scalar speeds, however, take only discrete values, not far short of the speed of light.
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Another approach to discrete space-time is to consider the set of integral solutions of the Diophantine equation $t^2-x^2-y^2-z^2=1$, and thus to examine the group of all integral Lorentz transformations [[#References|[a1]]], [[#References|[a2]]]. For this purpose, A. Schild used spin tensors with Gaussian integer components. He proved that the spatial projections of the time-like lines joining a fixed point ( "event" ) to other lattice points are dense, and therefore the direction in which material particles can move form a dense system; that is, a particle can move in "approximately" any direction. The scalar speeds, however, take only discrete values, not far short of the speed of light.
  
 
====References====
 
====References====
 
<table><TR><TD valign="top">[a1]</TD> <TD valign="top"> A. Schild, "Discrete space-time and integral Lorentz transformations" ''Canad. J. Math.'' , '''1''' (1949) pp. 29–47 {{MR|0029310}} {{ZBL|0038.40402}} </TD></TR><TR><TD valign="top">[a2]</TD> <TD valign="top"> H.S.M. Coxeter, G.J. Whitrow, "World structure and non-Euclidean honeycombs" ''Proc. Royal Soc. London'' , '''A201''' (1950) pp. 417–437 {{MR|0041576}} {{ZBL|0041.47202}} </TD></TR><TR><TD valign="top">[a3]</TD> <TD valign="top"> T.D. Lee, ''Physics Lett.'' , '''122B''' (1983) pp. 217</TD></TR></table>
 
<table><TR><TD valign="top">[a1]</TD> <TD valign="top"> A. Schild, "Discrete space-time and integral Lorentz transformations" ''Canad. J. Math.'' , '''1''' (1949) pp. 29–47 {{MR|0029310}} {{ZBL|0038.40402}} </TD></TR><TR><TD valign="top">[a2]</TD> <TD valign="top"> H.S.M. Coxeter, G.J. Whitrow, "World structure and non-Euclidean honeycombs" ''Proc. Royal Soc. London'' , '''A201''' (1950) pp. 417–437 {{MR|0041576}} {{ZBL|0041.47202}} </TD></TR><TR><TD valign="top">[a3]</TD> <TD valign="top"> T.D. Lee, ''Physics Lett.'' , '''122B''' (1983) pp. 217</TD></TR></table>

Latest revision as of 16:58, 2 July 2014

One conceivable hypothesis on the structure of space in the microcosmos, conceived as a collection of disconnected elements in space (points) which cannot be distinguished by observations. An acceptable formalization of discrete space-time can be given in terms of topological spaces $Y$ in which the connected component of a point $y\in Y$ is its closure $\bar y$, and, in a Hausdorff space $Y$, is this point itself (totally disconnected spaces). Examples of $Y$ include a discrete topological space, a rational straight line, analytic manifolds, and Lie groups over fields with ultra-metric absolute values.

The discrete space-time hypothesis was originally developed as a variation of a finite totally-disconnected space, in models of finite geometries on Galois fields V.A. Ambartsumyan and D.D. Ivanenko (1930) were the first to treat it in the framework of field theory (as a cubic lattice in space). In quantum theory the hypothesis of discrete space-time appeared in models in which the coordinate (momentum, etc.) space, like the spectrum of the $C^*$-algebra of corresponding operators, is totally disconnected (e.g. like the spectrum of the $C^*$-algebra of probability measures). It received a serious foundation in the concept of "fundamental lengths" in non-linear generalizations of electrodynamics, mesondynamics and Dirac's spinor theory, in which the constants of field action have the dimension of length, and in quantum field theory, where it is necessary to introduce all kinds of "cut-off" factors. These ideas, later in conjunction with non-local models, served as the base for the formulation of the concept of minimal domains in space in which it appears no longer possible to adopt the quantum-theoretical description of micro-objects in terms of their interaction with a macro-instrument. As a result, the space-time continuum is inacceptable for the parametrization of spatial-evolutionary relations in these domains (e.g. the Hamilton formalism in non-local theories), and their points cannot be distinguished by observation (in spaces $Y$ this may be represented as the presence of a non-Hausdorff uniform structure). The discrete space-time hypothesis was developed in the conception of the non-linear vacuum. According to this concept — under extreme conditions inside particles, and possibly also in astrophysical and cosmological singularities — the spatial characteristics may manifest themselves as dynamic characteristics of a physical system, in the models of which the spatial elements are provided with non-commutative binary operations.

References

[1] A. Sokolov, D. Ivanenko, "Quantum field theory" , Moscow-Leningrad (1952) (In Russian) MR0452326
[2] A.N. Vyal'tsev, "Discrete space-time" , Moscow (1965) (In Russian)
[3] D.I. Blokhintsev, "Space and time in the micro-universe" , Moscow (1970) (In Russian)
[4] M.A. Markov, "The nature of matter" , Moscow (1976) (In Russian)
[5] D. Finkel'stein, Phys. Rev. , 9 : 8 (1974) pp. 2219


Comments

Another approach to discrete space-time is to consider the set of integral solutions of the Diophantine equation $t^2-x^2-y^2-z^2=1$, and thus to examine the group of all integral Lorentz transformations [a1], [a2]. For this purpose, A. Schild used spin tensors with Gaussian integer components. He proved that the spatial projections of the time-like lines joining a fixed point ( "event" ) to other lattice points are dense, and therefore the direction in which material particles can move form a dense system; that is, a particle can move in "approximately" any direction. The scalar speeds, however, take only discrete values, not far short of the speed of light.

References

[a1] A. Schild, "Discrete space-time and integral Lorentz transformations" Canad. J. Math. , 1 (1949) pp. 29–47 MR0029310 Zbl 0038.40402
[a2] H.S.M. Coxeter, G.J. Whitrow, "World structure and non-Euclidean honeycombs" Proc. Royal Soc. London , A201 (1950) pp. 417–437 MR0041576 Zbl 0041.47202
[a3] T.D. Lee, Physics Lett. , 122B (1983) pp. 217
How to Cite This Entry:
Discrete space-time. Encyclopedia of Mathematics. URL: http://encyclopediaofmath.org/index.php?title=Discrete_space-time&oldid=32352
This article was adapted from an original article by G.A. Sardanashvili (originator), which appeared in Encyclopedia of Mathematics - ISBN 1402006098. See original article