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mean width : ウィキペディア英語版
mean width
In geometry, the mean width is a measure of dimension length of the "size" of a body; see Hadwiger's theorem for more about the available measures of bodies. In n dimensions, one has to consider (n-1)-dimensional hyperplanes perpendicular to a given direction \hat in S^, where S^n is the n-sphere (the surface of a (n+1)-dimensional sphere).
The "width" of a body in a given direction \hat is the distance between the closest pair of such planes, such that the body is entirely in between the two hyper planes (the planes only intersect
with the boundary of the body). The mean width is the average of this "width" over all \hat in S^.
More formally, define a compact body B as being equivalent to set of points in its interior plus the points on the boundary (here, points denote elements of \mathbb^n). The support function of body B is defined as
: h_B(n)=\max\
where n is a direction and \langle,\rangle denotes the usual inner product on \mathbb^n. The mean width is then
: b(B)=\frac} h_B(\hat)+h_B(-\hat),
where S_ is the (n-1)-dimensional volume of S^.
Note, that the mean width can be defined for any body (that is compact), but it is most
useful for convex bodies (that is bodies, whose corresponding set is a convex set).
==Mean widths of convex bodies in low dimensions==


抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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