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Curvature of a measure : ウィキペディア英語版
Curvature of a measure
In mathematics, the curvature of a measure defined on the Euclidean plane R2 is a quantification of how much the measure's "distribution of mass" is "curved". It is related to notions of curvature in geometry. In the form presented below, the concept was introduced in 1995 by the mathematician Mark S. Melnikov; accordingly, it may be referred to as the Melnikov curvature or Menger-Melnikov curvature. Melnikov and Verdera (1995) established a powerful connection between the curvature of measures and the Cauchy kernel.
==Definition==

Let ''μ'' be a Borel measure on the Euclidean plane R2. Given three (distinct) points ''x'', ''y'' and ''z'' in R2, let ''R''(''x'', ''y'', ''z'') be the radius of the Euclidean circle that joins all three of them, or +∞ if they are collinear. The Menger curvature ''c''(''x'', ''y'', ''z'') is defined to be
:c(x, y, z) = \frac,
with the natural convention that ''c''(''x'', ''y'', ''z'') = 0 if ''x'', ''y'' and ''z'' are collinear. It is also conventional to extend this definition by setting ''c''(''x'', ''y'', ''z'') = 0 if any of the points ''x'', ''y'' and ''z'' coincide. The Menger-Melnikov curvature ''c''2(''μ'') of ''μ'' is defined to be
:c^ (\mu) = \iiint_} c(x, y, z)^ \, \mathrm \mu (x) \mathrm \mu (y) \mathrm \mu (z).
More generally, for ''α'' ≥ 0, define ''c''2''α''(''μ'') by
:c^ (\mu) = \iiint_} c(x, y, z)^ \, \mathrm \mu (x) \mathrm \mu (y) \mathrm \mu (z).
One may also refer to the curvature of ''μ'' at a given point ''x'':
:c^ (\mu; x) = \iint_} c(x, y, z)^ \, \mathrm \mu (y) \mathrm \mu (z),
in which case
:c^ (\mu) = \int_} c^ (\mu; x) \, \mathrm \mu (x).

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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