Difference between revisions of "Ray function"
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− | + | A real-valued function $ F ( x) $ | |
+ | defined on an $ n $- | ||
+ | dimensional space $ \mathbf R ^ {n} $ | ||
+ | and satisfying the following conditions: $ F ( x) $ | ||
+ | is continuous, non-negative and homogeneous (that is, $ F ( \tau x) = \tau F ( x) $ | ||
+ | for any real number $ \tau \geq 0 $). | ||
+ | A ray function $ F ( x) $ | ||
+ | is said to be positive if $ F ( x) > 0 $ | ||
+ | for all $ x \neq 0 $, | ||
+ | and symmetric if $ F ( - x ) = F ( x) $. | ||
+ | A ray function is said to be convex if for any $ x , y \in \mathbf R ^ {n} $, | ||
− | + | $$ | |
+ | F ( x + y ) \leq F ( x) + F ( y) . | ||
+ | $$ | ||
− | + | For any ray function $ F ( x) $ | |
+ | there is a constant $ c = c _ {F} $ | ||
+ | for which | ||
− | + | $$ | |
+ | F ( x) \leq c | x | ,\ x \in \mathbf R ^ {n} . | ||
+ | $$ | ||
− | + | If $ F ( x) $ | |
+ | is positive, then there is also a constant $ \widetilde{c} = \widetilde{c} _ {F} > 0 $ | ||
+ | for which | ||
− | + | $$ | |
+ | F ( x) \geq \widetilde{c} | x | ,\ x \in \mathbf R ^ {n} . | ||
+ | $$ | ||
− | + | The set $ \mathfrak C $ | |
+ | of points $ x \in \mathbf R ^ {n} $ | ||
+ | satisfying the condition | ||
− | < | + | $$ |
+ | F ( x) < 1 | ||
+ | $$ | ||
− | + | is a [[Star body|star body]]. Conversely, for any open star body $ \mathfrak C $ | |
+ | there is a unique ray function $ F _ {\mathfrak C } ( x) $ | ||
+ | for which | ||
+ | |||
+ | $$ | ||
+ | \mathfrak C = \{ {x } : {F _ {\mathfrak C } ( x) < 1 } \} | ||
+ | . | ||
+ | $$ | ||
+ | |||
+ | A star body $ \mathfrak C _ {F} $ | ||
+ | is bounded if and only if its ray function $ F ( x) $ | ||
+ | is positive. If $ F ( x) $ | ||
+ | is a symmetric function, then $ \mathfrak C _ {F} $ | ||
+ | is symmetric about the point 0; the converse is also true. A star body is convex if and only if $ F ( x) $ | ||
+ | is a convex ray function. | ||
====References==== | ====References==== | ||
<table><TR><TD valign="top">[1]</TD> <TD valign="top"> J.W.S. Cassels, "An introduction to the geometry of numbers" , Springer (1959)</TD></TR></table> | <table><TR><TD valign="top">[1]</TD> <TD valign="top"> J.W.S. Cassels, "An introduction to the geometry of numbers" , Springer (1959)</TD></TR></table> | ||
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− | |||
====Comments==== | ====Comments==== |
Latest revision as of 08:10, 6 June 2020
A real-valued function $ F ( x) $
defined on an $ n $-
dimensional space $ \mathbf R ^ {n} $
and satisfying the following conditions: $ F ( x) $
is continuous, non-negative and homogeneous (that is, $ F ( \tau x) = \tau F ( x) $
for any real number $ \tau \geq 0 $).
A ray function $ F ( x) $
is said to be positive if $ F ( x) > 0 $
for all $ x \neq 0 $,
and symmetric if $ F ( - x ) = F ( x) $.
A ray function is said to be convex if for any $ x , y \in \mathbf R ^ {n} $,
$$ F ( x + y ) \leq F ( x) + F ( y) . $$
For any ray function $ F ( x) $ there is a constant $ c = c _ {F} $ for which
$$ F ( x) \leq c | x | ,\ x \in \mathbf R ^ {n} . $$
If $ F ( x) $ is positive, then there is also a constant $ \widetilde{c} = \widetilde{c} _ {F} > 0 $ for which
$$ F ( x) \geq \widetilde{c} | x | ,\ x \in \mathbf R ^ {n} . $$
The set $ \mathfrak C $ of points $ x \in \mathbf R ^ {n} $ satisfying the condition
$$ F ( x) < 1 $$
is a star body. Conversely, for any open star body $ \mathfrak C $ there is a unique ray function $ F _ {\mathfrak C } ( x) $ for which
$$ \mathfrak C = \{ {x } : {F _ {\mathfrak C } ( x) < 1 } \} . $$
A star body $ \mathfrak C _ {F} $ is bounded if and only if its ray function $ F ( x) $ is positive. If $ F ( x) $ is a symmetric function, then $ \mathfrak C _ {F} $ is symmetric about the point 0; the converse is also true. A star body is convex if and only if $ F ( x) $ is a convex ray function.
References
[1] | J.W.S. Cassels, "An introduction to the geometry of numbers" , Springer (1959) |
Comments
Star bodies are usually defined as closed ray sets. A ray function is more commonly called a distance function.
References
[a1] | P.M. Gruber, C.G. Lekkerkerker, "Geometry of numbers" , North-Holland (1987) pp. Sect. (iv) (Updated reprint) |
[a2] | E. Hlawka, "Das inhomogene Problem in der Geometrie der Zahlen" , Proc. Internat. Congress Mathematicians (Amsterdam, 1954) , 3 , Noordhoff (1954) pp. 20–27 ((Also: Selecta, Springer 1990, 178–185.)) |
Ray function. Encyclopedia of Mathematics. URL: http://encyclopediaofmath.org/index.php?title=Ray_function&oldid=48442