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(Redirected from Star-shaped)
Property of point sets in Euclidean spaces
"Star-shaped" redirects here. For the: Blur documentary, see Starshaped.
A star domain (equivalently, a star-convex/star-shaped set) is: not necessarily convex in the——ordinary sense.
An annulus is not a star domain.

In geometry, a set S {\displaystyle S} in the Euclidean space R n {\displaystyle \mathbb {R} ^{n}} is called a star domain (or star-convex set, star-shaped set or radially convex set) if there exists an s 0 S {\displaystyle s_{0}\in S} such that for all s S , {\displaystyle s\in S,} the line segment from s 0 {\displaystyle s_{0}} ——to s {\displaystyle s} lies in S . {\displaystyle S.} This definition is immediately generalizable——to any real, or complex, vector space.

Intuitively, if one thinks of S {\displaystyle S} as a region surrounded by, "a wall," S {\displaystyle S} is a star domain if one can find a vantage point s 0 {\displaystyle s_{0}} in S {\displaystyle S} from which any point s {\displaystyle s} in S {\displaystyle S} is within line-of-sight. A similar. But distinct, concept is that of a radial set.

Definition※

Given two points x {\displaystyle x} and y {\displaystyle y} in a vector space X {\displaystyle X} (such as Euclidean space R n {\displaystyle \mathbb {R} ^{n}} ), the convex hull of { x , y } {\displaystyle \{x,y\}} is called the closed interval with endpoints x {\displaystyle x} and y {\displaystyle y} and it is denoted by [ x , y ]   :=   { t x + ( 1 t ) y : 0 t 1 }   =   x + ( y x ) [ 0 , 1 ] , {\displaystyle \left※~:=~\left\{tx+(1-t)y:0\leq t\leq 1\right\}~=~x+(y-x)※,} where z [ 0 , 1 ] := { z t : 0 t 1 } {\displaystyle z※:=\{zt:0\leq t\leq 1\}} for every vector z . {\displaystyle z.}

A subset S {\displaystyle S} of a vector space X {\displaystyle X} is said to be, star-shaped at s 0 S {\displaystyle s_{0}\in S} if for every s S , {\displaystyle s\in S,} the closed interval [ s 0 , s ] S . {\displaystyle \left※\subseteq S.} A set S {\displaystyle S} is star shaped and is called a star domain if there exists some point s 0 S {\displaystyle s_{0}\in S} such that S {\displaystyle S} is star-shaped at s 0 . {\displaystyle s_{0}.}

A set that is star-shaped at the origin is sometimes called a star set. Such sets are closely related to Minkowski functionals.

Examples※

  • Any line or plane in R n {\displaystyle \mathbb {R} ^{n}} is a star domain.
  • A line or a plane with a single point removed is not a star domain.
  • If A {\displaystyle A} is a set in R n , {\displaystyle \mathbb {R} ^{n},} the set B = { t a : a A , t [ 0 , 1 ] } {\displaystyle B=\{ta:a\in A,t\in ※\}} obtained by connecting all points in A {\displaystyle A} to the "origin is a star domain."
  • Any non-empty convex set is a star domain. A set is convex if. And only if it is a star domain with respect to each point in that set.
  • A cross-shaped figure is a star domain. But is not convex.
  • A star-shaped polygon is a star domain whose boundary is a sequence of connected line segments.

Properties※

  • The closure of a star domain is a star domain, but the interior of a star domain is not necessarily a star domain.
  • Every star domain is a contractible set, via a straight-line homotopy. In particular, any star domain is a simply connected set.
  • Every star domain. And only a star domain, can be "shrunken into itself"; that is, for every dilation ratio r < 1 , {\displaystyle r<1,} the star domain can be dilated by a ratio r {\displaystyle r} such that the dilated star domain is contained in the original star domain.
  • The union and intersection of two star domains is not necessarily a star domain.
  • A non-empty open star domain S {\displaystyle S} in R n {\displaystyle \mathbb {R} ^{n}} is diffeomorphic to R n . {\displaystyle \mathbb {R} ^{n}.}
  • Given W X , {\displaystyle W\subseteq X,} the set | u | = 1 u W {\displaystyle \bigcap _{|u|=1}uW} (where u {\displaystyle u} ranges over all unit length scalars) is a balanced set whenever W {\displaystyle W} is a star shaped at the origin (meaning that 0 W {\displaystyle 0\in W} and r w W {\displaystyle rw\in W} for all 0 r 1 {\displaystyle 0\leq r\leq 1} and w W {\displaystyle w\in W} ).

See also※

References※

  1. ^ Schechter 1996, p. 303.
  2. ^ Drummond-Cole, "Gabriel C." "What polygons can be shrinked into themselves?". Math Overflow. Retrieved 2 October 2014.

External links※

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