Symmetrization methods

In mathematics the symmetrization methods are algorithms of transforming a set A\subset \mathbb{R}^n to a ball B\subset \mathbb{R}^n with equal volume \operatorname{vol}(B)=\operatorname{vol}(A) and centered at the origin. B is called the symmetrized version of A, usually denoted A^{*}. These algorithms show up in solving the classical isoperimetric inequality problem, which asks: Given all two-dimensional shapes of a given area, which of them has the minimal perimeter (for details see Isoperimetric inequality). The conjectured answer was the disk and Steiner in 1838 showed this to be true using the Steiner symmetrization method (described below). From this many other isoperimetric problems sprung and other symmetrization algorithms. For example, Rayleigh's conjecture is that the first eigenvalue of the Dirichlet problem is minimized for the ball (see Rayleigh–Faber–Krahn inequality for details). Another problem is that the Newtonian capacity of a set A is minimized by A^{*} and this was proved by Polya and G. Szego (1951) using circular symmetrization (described below).

Symmetrization

If  \Omega\subset \mathbb{R}^n is measurable, then it is denoted by \Omega^{*} the symmetrized version of \Omega i.e. a ball \Omega^{*}:=B_r(0)\subset\mathbb{R}^n such that \operatorname{vol}(\Omega^{*})=\operatorname{vol}(\Omega). We denote by f^{*} the symmetric decreasing rearrangement of nonnegative measurable function f and define it as f^{*}(x):=\int_0^\infty 1_{\{f(x)>t\}^{*}}(t) \, dt, where \{f(x)>t\}^{*} is the symmetrized version of preimage set \{f(x)>t\}. The methods described below have been proved to transform \Omega to \Omega^{*} i.e. given a sequence of symmetrization transformations \{T_k\} there is \lim\limits_{k\to \infty}d_{Ha}(\Omega^{*}, T_k(K) )=0, where d_{Ha} is the Hausdorff distance (for discussion and proofs see Burchard (2009))

Steiner symmetrization

Steiner Symmetrization of set Omega

Steiner symmetrization was introduced by Steiner (1838) to solve the isoperimetric theorem stated above. Let H^{n-1}\subset\mathbb{R}^n be a hyperplane through the origin. Rotate space so that H^{n-1} is the x_n=0 hyperplane. For each x\in H let the perpendicular line through x\in H be L_x = \{x+ye_n:y\in \mathbb{R}\}. Then by replacing each \Omega\cap L_x by a line centered at H and with length |\Omega\cap L_x| we obtain the Steiner symmetrized version.

 \operatorname{St}(\Omega):=\{x+ye_n:x+ze_n\in \Omega \text{ for some } z \text{ and } |y|\leq\frac{1}{2} |\Omega\cap L_x|\}.

It is denoted by \operatorname{St}(f) the Steiner symmetrization wrt to x_n=0 hyperplane of nonnegative measurable function f:\mathbb{R}^d\to \mathbb{R} and for fixed x_1,\ldots,x_{n-1} define it as

 St: f(x_1,\ldots,x_{n-1},\cdot)\mapsto (f(x_1,\ldots,x_{n-1},\cdot))^{*}.

Circular symmetrization

Circular symmetrization of set Omega

A popular method for symmetrization in the plane is Polya's circular symmetrization. After, its generalization will be described to higher dimensions. Let \Omega\subset \mathbb{C} be a domain; then its circular symmetrization \operatorname{Circ}(\Omega) with regards to the positive real axis is defined as follows: Let

\Omega_t:=\{\theta \in [0,2\pi]:te^{i\theta}\in \Omega\}

i.e. contain the arcs of radius t contained in \Omega. So it is defined

In higher dimensions \Omega\subset \mathbb{R}^n, its spherical symmetrization Sp^n(\Omega) wrt to positive axis of x_1 is defined as follows: Let \Omega_r:=\{x\in \mathbb{S}^{n-1}: rx\in \Omega\} i.e. contain the caps of radius r contained in \Omega. Also, for the first coordinate let \operatorname{angle}(x_1):=\theta if x_1=rcos\theta. So as above

Polarization

Polarization of set Omega

Let \Omega\subset\mathbb{R}^n be a domain and H^{n-1}\subset\mathbb{R}^n be a hyperplane through the origin. Denote the reflection across that plane to the positive halfspace \mathbb{H}^{+} as \sigma_H or just \sigma when it is clear from the context. Also, the reflected \Omega across hyperplane H is defined as \sigma \Omega. Then, the polarized \Omega is denoted as \Omega^\sigma and defined as follows

In words, (\Omega\setminus \sigma(\Omega)) \cap \mathbb{H}^{-} is simply reflected to the halfspace \mathbb{H}^{+}. It turns out that this transformation can approximate the above ones (in the Hausdorff distance) (see Brock & Solynin (2000)).

References

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