Open Access
Issue
Wuhan Univ. J. Nat. Sci.
Volume 28, Number 3, June 2023
Page(s) 217 - 220
DOI https://doi.org/10.1051/wujns/2023283217
Published online 13 July 2023

© Wuhan University 2023

Licence Creative CommonsThis is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

0 Introduction

Over the past two centuries, Steiner symmetrization has frequently been employed as a tool for addressing various issues, such as solving isoperimetric problems related to convex bodies, establishing properties of volume and surface area, and proving certain convex geometric inequalities. In recent years, numerous papers have been published on Steiner symmetrizations, which are essential for examining these related problems, see

e.g. Refs. [1-4]. Steiner symmetrization not only serves as the foundation for geometric analysis but also holds a significant role in other branches of mathematics. The authors of Refs. [2,5] constructed a series of Steiner symmetrizations for a given convex body under a specific directional sequence, where the direction sequence is chosen from a finite set of directions on the unit sphere, and the series of Steiner symmetrizations converge to a ball.

There remain many fundamental unsolved problems concerning Steiner symmetrizations. One of the such questions is whether the sequence of Steiner symmetrizations converges to a ball when the direction sequence, which is used to construct Steiner symmetrizations, is dense on the unit sphere. In this paper, we identify suitable iterative sequences of Steiner symmetrizations that do not converge to a ball with the same volume as the initial convex body. Furthermore, we provide examples of specific cases that do not converge under Steiner symmetrizations. Convergent sequences employed to construct Steiner symmetrization typically depend on geometric functions that decrease monotonically along the sequence, such as volume and chord length. In this paper, our primary focus is on designing a sequence of directions that is non-convergent, meaning that the direction sequences diverge in certain cases.

Furthermore, is it possible for the Steiner symmetrization of a convex body to become non-convergent when the selected direction sequence is dense on the unit sphere Sn-1Mathematical equation? Recently, some researchers have raised the same question and demonstrated that by rearranging the direction sequence, the outcomes of Steiner symmetrizations along any dense direction sequence can either converge or diverge [5]. Additionally, they reveal that any given Steiner symmetrization sequence, whether convergent or not, possesses a non-convergent subsequence [6]. In Refs. [5] and [6], the authors mainly focused on the case of convex bodies in the plane. In this paper, we consider the cases of convex bodies and compact sets in high-dimensional space. We construct a specific sequence of directions in high-dimensional space, which guarantees that the sequence of iterative Steiner symmetrizations of the convex body or compact set is non-convergent under this sequence of directions.

1 Preliminaries

Let KMathematical equation be an nMathematical equation-dimensional convex body in RnMathematical equation. The Steiner symmetrization SuKMathematical equation of KMathematical equation with respect to the hyperplane uMathematical equation is the union of the line segments that are produced by translating the intersections of lines parallel to uMathematical equation and the convex body KMathematical equation, where the midpoints of all the line segments lie on the hyperplane uMathematical equation. For a given convex body KRnMathematical equation, we randomly select a sequence of unit directions uiMathematical equation on the unit sphere and perform iterative Steiner symmetrizations on KMathematical equation. The sequence of Steiner symmetrizations SuiSui-1Su1KMathematical equation can converge to a ball if the chosen sequence of the directions is good enough, see e.g. Ref. [7]. On the other hand, the direction set ΛMathematical equation must be dense and appropriately selected from the unit sphere to allow the sequence of Steiner symmetrizations SuiSui-1Su1KMathematical equation of convex body KMathematical equation to converge to a ball. Conversely, an arbitrarily countable dense sequence of directions might not necessarily result in convergence to the ball. Consequently, the order of directions could be crucial for generating the desired effect. In the subsequent analysis, we examine the non-convergence of Steiner symmetrizations applied to a specific convex body KMathematical equation. If we do not choose the appropriate sequence of directional uiMathematical equation, then the limit of the Steiner symmetrization sequence SuiSui-1Su1KMathematical equation of the convex body KMathematical equation may not be convergent when iMathematical equation.

Two essential lemmas and several basic properties of Steiner symmetrizations are given as the following. Standard references to the fundamental properties of Steiner symmetrization include Refs. [2,5,8].

Lemma 1[9] Let p1,p2,Mathematical equation be a sequence of positive prime integers. Then the sum

i = 1 1 p i Mathematical equation(1)

diverges.

Lemma 2   (see Ref. [10], Theorem 2.2)Let {um}Mathematical equation be a sequence in Sn-1Mathematical equation with um-1um=cosαmMathematical equation, where {αm}Mathematical equation is a sequence in (0,π/2)Mathematical equation that satisfies

m = 1 α m 2 < Mathematical equation

Then there exists a sequence of rotations {Rm}Mathematical equation such that for every non-empty compact set KRnMathematical equation, the rotated symmetrization sequence

K m = R m S u m S u 1 K Mathematical equation(2)

converges in Hausdorff distance and in symmetric difference to a compact set LMathematical equation.

2 The Non-Convergence of Steiner Symmetrizations

In this section we will construct several cases where the Steiner symmetrizations do not converge. First, we need to find a column of suitable dense direction sequence on the unit sphere. We perform iterate Steiner symmetrizations of the given convex body in these directions, and finally summarize the results of the symmetrizations. Moreover, we prove the limits of some directional sequences under Steiner symmetrizations that either do not exist, or do not converge to an ellipsoid or to a non-convex body (non-compact set) for some unique convex bodies. Using the examples given in the plane, we can quickly get the high dimensional case through low dimensional recurrence.

2.1 The Non-Convergence of Convex Bodies

2.1.1 Construction of directional sequences

Let p1,p2,Mathematical equation be a sequence of positive prime integers. By Lemma 1, we have the sequence sum

i = 1 1 p i Mathematical equation

diverge. Now for any m1Mathematical equation, denote the counter clockwise angle

θ m = i = 1 m 2 p i Mathematical equation(3)

in R2Mathematical equation, and θmMathematical equation is represented by radian, let umMathematical equation be the unit vector in R2Mathematical equation. When θmMathematical equation, we have each continuous incremental angle 2/pm0Mathematical equation, where the unit vector umMathematical equation is an element in a countable dense subset on the unit circle.

Now we look at the following formula

m = 1 c o s ( 2 p m ) = m = 1 ( 1 - 2 s i n 2 2 2 p m ) m = 1 ( 1 - 2 ( 2 2 p m ) 2 ) m = 1 ( 1 - 1 p m 2 ) Mathematical equation(4)

Applying the Euler product formula [11] to the above formula, we obtain

( m = 1 c o s ( 2 p m ) ) - 1 m = 1 ( 1 1 - 1 p m 2 ) = m = 1 ( 1 + 1 p m 2 + 1 p m 4 + ) = k = 1 1 k 2 = π 2 6 Mathematical equation(5)

Thus,

m = 1 c o s 2 p m 6 π 2 Mathematical equation(6)

2.1.2 Non-convergence of line segments

Let lMathematical equation be a line segment perpendicular to the horizontal axis and centered at the origin with a length of 1. Now make the line segment lMathematical equation Steiner symmetrization under the direction sequence {um}Mathematical equation to get SumMathematical equation. As a result, for every symmetrization done, the previous segment is projected onto a line perpendicular to the {um}Mathematical equation. Thus the length of the subsequent segment is equal to that of the previous segment multiplied by the incremental cosine cos(2/pi)Mathematical equation. Moreover, since the limit of i=1cos(2/pi)Mathematical equation in the formula (6) is constant and greater than zero, and the direction angle θmMathematical equation always circles around the circle in a certain order, the Steiner symmetrization of the line segment lMathematical equation always circulates in the circle, and its length is close to a value greater than zero in a limit.

Therefore, it was concluded that the sequence of line segments

l m = S u m S u 2 S u 1 l Mathematical equation(7)

has no limit.

2.1.3 Non-convergence of special convex bodies

Let KMathematical equation be a cylindrical convex body of area εMathematical equation and contain a summation axis. According to the monotonicity of the Steiner symmetrizations on convex bodies, in the Steiner symmetrization sequence

K m = S u m S u 2 S u 1 K Mathematical equation(8)

each element has a corresponding axis of symmetrization lmMathematical equation, so that the diameter of each KmMathematical equation is greater than 6/π2Mathematical equation. The Steiner symmetrization shows that each KmMathematical equation has the same area εMathematical equation as the original convex body KMathematical equation, where εMathematical equation can be arbitrarily small, so that the sequence KmMathematical equation can never converge to a ball. Actually, when ε<9/π3Mathematical equation, the sequence KmMathematical equation does not converge, because the symmetry axis of KmMathematical equation keeps consistently rotating, but does not converge to a very small area of εMathematical equation.

We have shown that some special convex body or compact set do not necessarily converge after Steiner symmetrizations under a countably dense sequence of orientations. In this section, we use specific examples to show that convex bodies are not valid for Steiner symmetrizations under a specific directional sequence when the divergent series (1) are used as the basis to facilitate the calculation. Refs. [10,12] have shown that a more general family of examples can be constructed starting with any decreasing sequence of incremental angles θiMathematical equation provided that i=1θi2Mathematical equation converges and i=1θiMathematical equation diverges. By applying the iterated Steiner symmetrizations in the resulting sequence of directions to a sufficiently eccentric ellipsoid, we will obtain a sequence of ellipsoids whose principal axes rotate forever without converging to a ball.

2.1.4 Another way of expressing non-convergence

First construct a column of sequence θmMathematical equation in (0,π/2)Mathematical equation with

m = 1 θ m = , m = 1 θ m 2 < Mathematical equation(9)

and set γ=m=1cosθmMathematical equation.

For every mN+Mathematical equation, define βm=k=1θkMathematical equation and um=(cosβm,sinβm)Mathematical equation.Here we need to pay attention to β(0,1)Mathematical equation. Indeed, if mMathematical equation is greater than a specific NMathematical equation, then (9) indicates that θm(0,1)Mathematical equation. The above reasoning leads to

c o s θ m = 1 - 2 s i n 2 θ m 2 1 - θ m 2 2 Mathematical equation

and when x(0,1/2)Mathematical equation, we can get

l n ( 1 - x ) - ( 1 + ο ( 1 ) ) x Mathematical equation

Thus

m = 1 l n c o s θ m m = 1 N l n c o s θ m - ( 1 + ο ( 1 ) ) m = N + 1 θ m 2 2 > - Mathematical equation

By the above inequality and γ=em=1lncosθmMathematical equation, we have γ>0Mathematical equation.

Let KMathematical equation be a disk of diameter less than γMathematical equation, and it contains a line segment lMathematical equation perpendicular to the horizontal axis and of length 1. Now the convex body KMathematical equation and the line segment lMathematical equation are made Steiner symmetrical simultaneously, which gives the convex bodies sequence KmMathematical equation and line segments sequence lmMathematical equation. If each Steiner symmetrization SumMathematical equation is projected from the former line segment lm-1Mathematical equation onto the umMathematical equation, then the length of lmMathematical equation is equal to the length of lm-1Mathematical equation multiplied by the cosθmMathematical equation. Since βmMathematical equation is diverged, the line segment lmMathematical equation always rotates around the circle, and thus the length of the line segment lmMathematical equation is monotonically reduced to γMathematical equation. Because KmlmMathematical equation, for each mMathematical equation, there is a KmMathematical equation diameter larger than γMathematical equation. When the sequence KmMathematical equation is convergent, its limiting value must contain a disk of diameter γMathematical equation. In addition, the area of KmMathematical equation is equal to the area of the convex body KMathematical equation, so this is a contradiction of the above situation. In conclusion, the sequence KmMathematical equation does not converge.

2.2 The Non-Convergence of Compact set

Define a compact set KMathematical equation which consists of a line segment lMathematical equation and a ball BrMathematical equation with radius rMathematical equation, select the orientation sequence {um}Mathematical equation in S1Mathematical equation and um-1um=cosθmMathematical equation , γ=m=1cosθmMathematical equation , where the angle of rotation direction sequence θmMathematical equation belongs to (0,π/2)Mathematical equation and satisfies m=1θm2<Mathematical equation. For each non-empty compact set KRnMathematical equation, we can find a rotating sequence {Rm}Mathematical equation such that the Steiner symmetric sequence of KMathematical equation with respect to {Rm}Mathematical equation is

K m = R m S u m S u 1 K Mathematical equation(10)

By Lemma 2, we know that the limit of the sequence (10) must contain a ball BrMathematical equation of radius rMathematical equation and a line segment lMathematical equation of length γMathematical equation. Meanwhile, if we want to make m=1θm2Mathematical equation arbitrarily small, we can make γMathematical equation approach to 1 infinitely by removing several initial terms. Specifically, we can assume that γ>2/πMathematical equation. Let KMathematical equation be the convex hull of the line segment lMathematical equation in the non-convergence convex bodies and the ball BrMathematical equation with center at the origin, where r>0Mathematical equation. If the rotational symmetrization sequence (10) converges, then its limit value must also contain both a ball BrMathematical equation of radius rMathematical equation and a line segment lMathematical equation of length γMathematical equation. So we conclude that the area of any ellipsoid containing the above set is no less than πγr/2Mathematical equation. On the other hand, the area of KmMathematical equation is equal to the area of KMathematical equation, and the upper bound of the area of KMathematical equation is r/(1-4r2)Mathematical equation, then we can obtain a diamond equal to the KMathematical equation area converging to a circle centered on the origin, where the longer diamond is a line segment lMathematical equation of length 1. Because if rMathematical equation is small enough, then its area will be smaller than πγr/2Mathematical equation, by the choice of γMathematical equation , the limit is not an ellipsoid.

So the above example shows that any compact convex set containing a ball BrMathematical equation and a line segment lMathematical equation has an area greater than or equal to γr/2Mathematical equation. Since the area of KMathematical equation is equal to the area of a ball of radius rMathematical equation, namely πr2Mathematical equation, the limiting value of KmMathematical equation is not a compact convex set when πr<γ/2Mathematical equation.

References

  1. Haberl C, Schuster F E. General Formula affine isoperimetric inequalities [J]. Journal of Differential Geometry, 2008, 83(1): 1-26. [Google Scholar]
  2. Lutwak E, Yang D, Zhang G. Orlicz projection bodies [J]. Advances in Mathematics, 2010, 233(1): 220-242. [CrossRef] [MathSciNet] [Google Scholar]
  3. Schaftingen J V. Equivalence between Pólya Szegö and relative capacity inequalities under rearrangement [J]. Archivder Mathematik, 2014, 103(4): 367-379. [CrossRef] [Google Scholar]
  4. Schaftingen J V. Approximation of symmetrizations and symmetry of critical points [J]. Topological Methods in Nonlinear Analysis, 2006, 28(1): 61-85. [MathSciNet] [Google Scholar]
  5. Bianchi G, Klain D A, Lutwak E, et al. A countable set of directions is sufficient for Steiner symmetrization [J]. Advances in Applied Mathematics, 2011, 47(4): 869-873. [CrossRef] [MathSciNet] [Google Scholar]
  6. Burchard A, Fortier F. Random polarizations [J]. Advances in Mathematics, 2013, 234: 550-573. [CrossRef] [MathSciNet] [Google Scholar]
  7. Mani P. Random Steiner symmetrizations [J]. Studia Scientiarum Mathematicarum Hungarica, 1986, 21(3): 373-378. [MathSciNet] [Google Scholar]
  8. Bonnesen T, Fenchel W, Boron L, et al. Theory of Convex Bodies[M]. Berlin: Springer-Verlag, 1934. [Google Scholar]
  9. Apostol T. Introduction to Analytic Number Theory [M]. Berlin: Springer-Verlag, 1976. [Google Scholar]
  10. Bianchi G, Burchard A, Gronchi P, et al. Convergence in shape of Steiner symmetrizations [J]. Indiana University Mathematics Journal, 2012, 61(4): 1695-1710. [CrossRef] [MathSciNet] [Google Scholar]
  11. Hardy G H, Wright E M. An Introduction to the Theory of Numbers [M]. Fifth Edition. New York: The Clarendon Press, 1979. [Google Scholar]
  12. Berenyi H M, Fiddy M A. Application of homometric sets for beam manipulation [J]. Journal of the Optical Society of America A, 1986, 3(3): 373-375. [NASA ADS] [CrossRef] [Google Scholar]

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.