Euclidean topology

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In mathematics, and especially general topology, the Euclidean topology is the natural topology induced on n-dimensional Euclidean space ℝn by the Euclidean metric.

Definition

The Euclidean norm on ℝn is the non-negative function ‖⋅‖:ℝn→ℝ defined by ‖(p1,…,pn)‖:=p12+⋯+pn2.

Like all norms, it induces a canonical metric defined by d(p,q)=‖p−q‖. The metric d:ℝn×ℝn→ℝ induced by the Euclidean norm is called the Euclidean metric or the Euclidean distance and the distance between points p=(p1,…,pn) and q=(q1,…,qn) is d(p,q)=‖p−q‖=(p1−q1)2+(p2−q2)2+⋯+(pi−qi)2+⋯+(pn−qn)2.

In any metric space, the open balls form a base for a topology on that space.[1] The Euclidean topology on ℝn is the topology Template:Em by these balls. In other words, the open sets of the Euclidean topology on ℝn are given by (arbitrary) unions of the open balls Br(p) defined as Br(p):={x∈ℝn:d(p,x)<r}, for all real r>0 and all p∈ℝn, where d is the Euclidean metric.

Properties

When endowed with this topology, the real line ℝ is a T5 space. Given two subsets say A and B of ℝ with A‾∩B=A∩B‾=∅, where A‾ denotes the closure of A, there exist open sets SA and SB with A⊆SA and B⊆SB such that SA∩SB=∅.[2]

See also

References

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