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Coarea formula

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Mathematic formula

In the mathematical field of geometric measure theory, the coarea formula expresses the integral of a function over an open set in Euclidean space in terms of integrals over the level sets of another function. A special case is Fubini's theorem, which says under suitable hypotheses that the integral of a function over the region enclosed by a rectangular box can be written as the iterated integral over the level sets of the coordinate functions. Another special case is integration in spherical coordinates, in which the integral of a function on R is related to the integral of the function over spherical shells: level sets of the radial function. The formula plays a decisive role in the modern study of isoperimetric problems.

For smooth functions the formula is a result in multivariate calculus which follows from a change of variables. More general forms of the formula for Lipschitz functions were first established by Herbert Federer (Federer 1959), and for BV functions by Fleming & Rishel (1960).

A precise statement of the formula is as follows. Suppose that Ω is an open set in R n {\displaystyle \mathbb {R} ^{n}} and u is a real-valued Lipschitz function on Ω. Then, for an L function g,

Ω g ( x ) | u ( x ) | d x = R ( u 1 ( t ) g ( x ) d H n 1 ( x ) ) d t {\displaystyle \int _{\Omega }g(x)|\nabla u(x)|\,dx=\int _{\mathbb {R} }\left(\int _{u^{-1}(t)}g(x)\,dH_{n-1}(x)\right)\,dt}

where Hn−1 is the (n − 1)-dimensional Hausdorff measure. In particular, by taking g to be one, this implies

Ω | u | = H n 1 ( u 1 ( t ) ) d t , {\displaystyle \int _{\Omega }|\nabla u|=\int _{-\infty }^{\infty }H_{n-1}(u^{-1}(t))\,dt,}

and conversely the latter equality implies the former by standard techniques in Lebesgue integration.

More generally, the coarea formula can be applied to Lipschitz functions u defined in Ω R n , {\displaystyle \Omega \subset \mathbb {R} ^{n},} taking on values in R k {\displaystyle \mathbb {R} ^{k}} where k ≤ n. In this case, the following identity holds

Ω g ( x ) | J k u ( x ) | d x = R k ( u 1 ( t ) g ( x ) d H n k ( x ) ) d t {\displaystyle \int _{\Omega }g(x)|J_{k}u(x)|\,dx=\int _{\mathbb {R} ^{k}}\left(\int _{u^{-1}(t)}g(x)\,dH_{n-k}(x)\right)\,dt}

where Jku is the k-dimensional Jacobian of u whose determinant is given by

| J k u ( x ) | = ( det ( J u ( x ) J u ( x ) ) ) 1 / 2 . {\displaystyle |J_{k}u(x)|=\left({\det \left(Ju(x)Ju(x)^{\intercal }\right)}\right)^{1/2}.}

Applications

  • Taking u(x) = |x − x0| gives the formula for integration in spherical coordinates of an integrable function f:
R n f d x = 0 { B ( x 0 ; r ) f d S } d r . {\displaystyle \int _{\mathbb {R} ^{n}}f\,dx=\int _{0}^{\infty }\left\{\int _{\partial B(x_{0};r)}f\,dS\right\}\,dr.}
( R n | u | n n 1 ) n 1 n n 1 ω n 1 n R n | u | {\displaystyle \left(\int _{\mathbb {R} ^{n}}|u|^{\frac {n}{n-1}}\right)^{\frac {n-1}{n}}\leq n^{-1}\omega _{n}^{-{\frac {1}{n}}}\int _{\mathbb {R} ^{n}}|\nabla u|}
where ω n {\displaystyle \omega _{n}} is the volume of the unit ball in R n . {\displaystyle \mathbb {R} ^{n}.}

See also

References

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