Two-dimensional space: Difference between revisions
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Two-dimensional spaces can also be [[curved space|curved]], for example the [[sphere]] and [[hyperbolic plane]], sufficiently small portions of which appear like the flat plane, but on which straight lines which are locally parallel do not stay equidistant from each-other but eventually converge or diverge, respectively. Two-dimensional spaces with a locally Euclidean concept of distance but which can have non-uniform [[Gaussian curvature|curvature]] are called [[differential geometry of surfaces|Riemannian surfaces]].{{efn|Not to be confused with [[Riemann surfaces]].}} |
Two-dimensional spaces can also be [[curved space|curved]], for example the [[sphere]] and [[hyperbolic plane]], sufficiently small portions of which appear like the flat plane, but on which straight lines which are locally parallel do not stay equidistant from each-other but eventually converge or diverge, respectively. Two-dimensional spaces with a locally Euclidean concept of distance but which can have non-uniform [[Gaussian curvature|curvature]] are called [[differential geometry of surfaces|Riemannian surfaces]].{{efn|Not to be confused with [[Riemann surfaces]].}} |
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Besides Riemannian surfaces which look locally like the Euclidean plane, there are [[Lorentzian manifold|Lorentzian]] surfaces which look locally like a two-dimensional slice of relativistic [[spacetime]] with one spatial and one time dimension, |
Besides Riemannian surfaces which look locally like the Euclidean plane, there are [[Lorentzian manifold|Lorentzian]] surfaces which look locally like a two-dimensional slice of relativistic [[spacetime]] with one spatial and one time dimension, constant-curvature examples of which are the flat Lorentzian plane (a two-dimensional subspace of [[Minkowski space]]), and the curved [[de Sitter space|de Sitter]] and [[anti-de Sitter space|anti-de Sitter]] planes. Between Riemannian and Lorentzian surfaces are [[Galilean geometry|Galilean]] surfaces which look locally like a two-dimensional slice of non-relativistic spacetime, including the flat Galilean plane and curved planes which are the [[duality (mathematics)|duals]] of the Euclidean plane and Lorentzian plane. |
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Other types of mathematical planes and surfaces modify or do away with the structures defining the Euclidean plane. For example, the [[affine plane]] has a notion of parallel lines but no notion of distance, and the [[projective plane]] does away with both. A two-dimensional [[metric space]] has some concept of distance but it need not match the Euclidean version. A [[surface (topology)|topological surface]] can be stretched, twisted, or bent without changing its essential properties. An [[algebraic surface]] is a two-dimensional set of solutions of a [[system of polynomial equations]]. |
Other types of mathematical planes and surfaces modify or do away with the structures defining the Euclidean plane. For example, the [[affine plane]] has a notion of parallel lines but no notion of distance, and the [[projective plane]] does away with both. A two-dimensional [[metric space]] has some concept of distance but it need not match the Euclidean version. A [[surface (topology)|topological surface]] can be stretched, twisted, or bent without changing its essential properties. An [[algebraic surface]] is a two-dimensional set of solutions of a [[system of polynomial equations]]. |
Revision as of 22:29, 26 December 2023
A two-dimensional space is a mathematical space with two dimensions, meaning points have two degrees of freedom: their locations can be locally described with two coordinates or they can move in two independent directions. Common two-dimensional spaces are often called planes, or, more generally, surfaces.
The most basic example is the flat Euclidean plane, an idealization of a flat surface in physical space such as a sheet of paper or a chalkboard. On the Euclidean plane, any two points can be joined by a unique straight line along which the distance can be measured. The space is flat because any two lines transversed by a third line perpendicular to both of them are parallel, meaning they never intersect and stay at uniform distance from each-other.
Two-dimensional spaces can also be curved, for example the sphere and hyperbolic plane, sufficiently small portions of which appear like the flat plane, but on which straight lines which are locally parallel do not stay equidistant from each-other but eventually converge or diverge, respectively. Two-dimensional spaces with a locally Euclidean concept of distance but which can have non-uniform curvature are called Riemannian surfaces.[a]
Besides Riemannian surfaces which look locally like the Euclidean plane, there are Lorentzian surfaces which look locally like a two-dimensional slice of relativistic spacetime with one spatial and one time dimension, constant-curvature examples of which are the flat Lorentzian plane (a two-dimensional subspace of Minkowski space), and the curved de Sitter and anti-de Sitter planes. Between Riemannian and Lorentzian surfaces are Galilean surfaces which look locally like a two-dimensional slice of non-relativistic spacetime, including the flat Galilean plane and curved planes which are the duals of the Euclidean plane and Lorentzian plane.
Other types of mathematical planes and surfaces modify or do away with the structures defining the Euclidean plane. For example, the affine plane has a notion of parallel lines but no notion of distance, and the projective plane does away with both. A two-dimensional metric space has some concept of distance but it need not match the Euclidean version. A topological surface can be stretched, twisted, or bent without changing its essential properties. An algebraic surface is a two-dimensional set of solutions of a system of polynomial equations.
Some mathematical spaces have additional arithmetical structure associated with their points. A two-dimensional vector space is an affine plane whose has points called vector with a special designated origin or zero vector, and a notion of adding vectors together or scaling (geometry) them by a number. A two-dimensional vector space can optionally include a Euclidean, Lorentzian, or Galilean concept of distance. The complex plane, hyperbolic number plane, and dual number plane each have points which are considered numbers themselves, and can be added and multiplied. A Riemann surface or Lorentz surface appear locally like the complex plane or hyperbolic number plane, respectively.
Mathematical spaces are often defined or represented using numbers rather than geometric axioms. One of the most fundamental two-dimensional spaces is the real coordinate space, denoted consisting of pairs of real-number coordinates. Sometimes the space represents arbitrary quantities rather than geometric positions, as in the parameter space of a mathematical model or the configuration space of a physical system.
More generally, other types of numbers can be used as coordinates. The complex plane is two-dimensional when considered to be formed from real-number coordinates, but one-dimensional in terms of complex-number coordinates. A two-dimensional complex space – such as the two-dimensional complex coordinate space, the complex projective plane, or a complex surface – has two complex dimensions, which can alternately be represented using four real dimensions. A two-dimensional lattice is an infinite grid of points which can be represented using integer coordinates. Some two-dimensional spaces, such as finite planes, have only a finite set of elements.
Notes
- ^ Not to be confused with Riemann surfaces.
Further reading
- Hartshorne, Robin (2000). Geometry: Euclid and Beyond. Springer. doi:10.1007/978-0-387-22676-7. ISBN 0-387-98650-2.
- Kinsey, Laura Christine (1993). Topology of Surfaces. Springer. doi:10.1007/978-1-4612-0899-0. ISBN 0-387-94102-9.
- Needham, Tristan (2021). Visual Differential Geometry and Forms. Princeton. ISBN 0-691-20370-9.
- Stillwell, John (1992). Geometry of Surfaces. Springer. doi:10.1007/978-1-4612-0929-4. ISBN 0-387-97743-0.
- Yaglom, Isaak Moiseevich (1968) [1963]. Complex Numbers in Geometry. Translated by Primrose, Eric J. F. Academic Press. LCCN 66-26269.