Menger curvature explained

In mathematics, the Menger curvature of a triple of points in n-dimensional Euclidean space Rn is the reciprocal of the radius of the circle that passes through the three points. It is named after the Austrian-American mathematician Karl Menger.

Definition

Let x, y and z be three points in Rn; for simplicity, assume for the moment that all three points are distinct and do not lie on a single straight line. Let Π ⊆ Rn be the Euclidean plane spanned by x, y and z and let C ⊆ Π be the unique Euclidean circle in Π that passes through x, y and z (the circumcircle of x, y and z). Let R be the radius of C. Then the Menger curvature c(xyz) of x, y and z is defined by

c(x,y,z)=

1{R}.

If the three points are collinear, R can be informally considered to be +∞, and it makes rigorous sense to define c(xyz) = 0. If any of the points x, y and z are coincident, again define c(xyz) = 0.

Using the well-known formula relating the side lengths of a triangle to its area, it follows that

c(x,y,z)=

1{R}
=
4A
|x-y||y-z||z-x|

,

where A denotes the area of the triangle spanned by x, y and z.

Another way of computing Menger curvature is the identity

c(x,y,z)=2\sin\anglexyz
|x-z|
where

\anglexyz

is the angle made at the y-corner of the triangle spanned by x,y,z.

Menger curvature may also be defined on a general metric space. If X is a metric space and x,y, and z are distinct points, let f be an isometry from

\{x,y,z\}

into

R2

. Define the Menger curvature of these points to be

cX(x,y,z)=c(f(x),f(y),f(z)).

Note that f need not be defined on all of X, just on , and the value cX (x,y,z) is independent of the choice of f.

Integral Curvature Rectifiability

Menger curvature can be used to give quantitative conditions for when sets in

Rn

may be rectifiable. For a Borel measure

\mu

on a Euclidean space

Rn

define

cp(\mu)=\int\int\intc(x,y,z)pd\mu(x)d\mu(y)d\mu(z).

E\subseteqRn

is rectifiable if

c2(H1|E)<infty

, where

H1|E

denotes one-dimensional Hausdorff measure restricted to the set

E

.[1]

The basic intuition behind the result is that Menger curvature measures how straight a given triple of points are (the smaller

c(x,y,z)max\{|x-y|,|y-z|,|z-y|\}

is, the closer x,y, and z are to being collinear), and this integral quantity being finite is saying that the set E is flat on most small scales. In particular, if the power in the integral is larger, our set is smoother than just being rectifiable[2]

p>3

,

f:S1Rn

be a homeomorphism and

\Gamma=f(S1)

. Then

f\in

1,1-3
p
C

(S1)

if

cp(H1|\Gamma)<infty

.

0<Hs(E)<infty

where
0<s\leq1
2
, and

c2s(Hs|E)<infty

, then

E

is rectifiable in the sense that there are countably many

C1

curves

\Gammai

such that

Hs(E\backslashcup\Gammai)=0

. The result is not true for
1
2

<s<1

, and

c2s(Hs|E)=infty

for

1<s\leqn

.:[3]

In the opposite direction, there is a result of Peter Jones:[4]

E\subseteq\Gamma\subseteqR2

,

H1(E)>0

, and

\Gamma

is rectifiable. Then there is a positive Radon measure

\mu

supported on

E

satisfying

\muB(x,r)\leqr

for all

x\inE

and

r>0

such that

c2(\mu)<infty

(in particular, this measure is the Frostman measure associated to E). Moreover, if

H1(B(x,r)\cap\Gamma)\leqCr

for some constant C and all

x\in\Gamma

and r>0, then

c2(H1|E)<infty

. This last result follows from the Analyst's Traveling Salesman Theorem.

Analogous results hold in general metric spaces:[5]

See also

External links

References

  1. Leger . J. . 1999 . Menger curvature and rectifiability . . 149 . 3 . 831–869 . math/9905212 . 10.2307/121074 . 121074 . 216176.
  2. Strzelecki . Paweł . Szumańska . Marta . von der Mosel . Heiko . 2010 . Regularizing and self-avoidance effects of integral Menger curvature . . 9 . 1 . 145–187.
  3. Lin . Yong . Mattila . Pertti . 2000 . Menger curvature and C1 regularity of fractals . . 129 . 6 . 1755–1762 . 10.1090/s0002-9939-00-05814-7 . free.
  4. Book: Pajot, H. . 2000 . Analytic Capacity, Rectifiability, Menger Curvature and the Cauchy Integral . Springer . 3-540-00001-1.
  5. Schul . Raanan . 2007 . Ahlfors-regular curves in metric spaces . . 32 . 437–460.