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BY 4.0 license Open Access Published by De Gruyter Open Access September 15, 2020

General (p,q)-mixed projection bodies

  • Yibin Feng and Yanping Zhou EMAIL logo
From the journal Open Mathematics

Abstract

In this article, the general (p,q)-mixed projection bodies are introduced. Then, some basic properties of the general (p,q)-mixed projection bodies are discussed, and the extreme values of volumes of the general (p,q)-mixed projection bodies and their polar bodies are established.

MSC 2010: 52A20; 52A40

1 Introduction

Projection bodies, introduced by Minkowski at the end of nineteenth century, are a central notion in the classical Brunn-Minkowski theory. In recent years, projection bodies and their polars have received considerable attention, see, e.g., [1,2,3,4,5,6,7,8,9].

The classical Brunn-Minkowski theory has a natural extension called the L p Brunn-Minkowski theory, which was initiated in the early 1960s when Firey introduced his concept of L p composition of convex bodies (see [10]) and was born in the works of Lutwak [11,12]. Since Lutwak’s two seminal works, this theory has attracted increasing interest in recent years, see, e.g., [13,14,15,16,17,18,19,20]. One of the central concepts in the L p Brunn-Minkowski theory is the L p projection bodies introduced by Lutwak et al. [17]. Afterward, Ludwig [21] (see also Haberl and Schuster [22]) extended Lutwak, Yang and Zhang’s L p projection bodies to an entire class which may be called general L p projection bodies. See, e.g., [23,24,25,26,27,28,29,30] for the L p and general L p projection bodies and their extensions.

The dual Brunn-Minkowski theory, developed by Lutwak [31] in 1975, is a dual concept of the classical Brunn-Minkowski theory. It is a theory of dual mixed volumes of star bodies and has already attracted considerable interest, see, e.g., [32,33,34,35,36,37,38,39,40]. In particular, a recent groundbreaking work of Huang et al. [41] showed that there exists a new family of geometry measures, in the dual Brunn-Minkowski theory, called dual curvature measures which are the long-sought duals of Federer’s curvature measures. Now, the dual curvature measures become the core of the dual Brunn-Minkowski theory.

Very recently, a unification of the L p Brunn-Minkowski theory and the dual Brunn-Minkowski theory was discovered by Lutwak et al. [42], where they introduced the L p dual curvature measures which include L p surface area measures and L p integral curvatures in the L p Brunn-Minkowski theory as well as the dual curvature measures in the dual Brunn-Minkowski theory. In the same way that the L p surface area and dual curvature measures, respectively, play a critical role in the L p and dual Brunn-Minkowski theories, the L p dual curvature measures can be seen to be a central concept within the unifying theory. See, e.g., [43,44,45,46] for some recent developments related to the L p dual curvature measures.

In this article, motivated by the works of Lutwak et al. [42], Ludwig [21] and Haberl and Schuster [22], we introduce a more general definition of projection bodies according to the L p dual curvature measures, which is called the general (p,q)-mixed projection bodies. Special cases include the classical projection bodies, L p projection bodies and general L p projection bodies. Then, we establish the extreme values of volumes for the general (p,q)-mixed projection bodies and their polar bodies. The detailed descriptions for the definition and main results are provided below.

Throughout n denotes the n-dimensional Euclidean space. A convex body is a compact convex subset of n with nonempty interior. We denote by K n the set of convex bodies and by K o n the set of convex bodies containing the origin in their interiors. For a convex body K K n , let K and V ( K ) be its boundary and n-dimensional volume, respectively. The unit sphere in n will be denoted by S n 1 . For x n , | x | = x x denotes the Euclidean norm of x, and for x n \ { 0 } , the unit vector x / | x | S n 1 will be abbreviated by x .

For all x n , the support function of K K n is defined by

h ( K , x ) = h K ( x ) = max { x y : y K } ,

where x y denotes the standard inner product of x and y.

The radial function, ρ K = ρ ( K , ) : n \ { 0 } , of a compact and star-shaped set, with respect to the origin, K n , is defined by

ρ ( K , x ) = max { λ : λ x K } .

If ρ K is positive and continuous, then K is called a star body with respect to the origin. The set of all star bodies about the origin in n is denoted by S o n . Two star bodies K and L are dilates (of one another) if ρ K ( u ) / ρ L ( u ) is independent of u S n 1 . For a star body Q S o n , Q : n [ 0 , ) is a continuous and positively homogeneous function of degree 1, which was defined, in [42], by

x Q = 1 / ρ Q ( x ) x 0 ; 0 x = 0 .

For a convex body K K o n , its polar body K is defined by

K = { x n : x y 1 for all y K } .

Suppose p , q . If K K o n while Q S o n , then the L p dual curvature measure, C ˜ p , q ( K , Q , ) , on S n 1 was defined, in [42], by

(1.1) S n 1 g ( v ) d C ˜ p , q ( K , Q , v ) = 1 n S n 1 g ( α K ( u ) ) h K ( α K ( u ) ) p ρ K ( u ) q ρ Q ( u ) n q d u

for each continuous g : S n 1 , where α K is the radial Gauss map that associates with almost each u S n 1 the unique outer unit normal at the point ρ K ( u ) u K .

In [42], the L p surface area measures were shown to be special cases of the L p dual curvature measures:

(1.2) C ˜ p , q ( K , K , ) = 1 n S p ( K , ) ;

(1.3) C ˜ p , n ( K , Q , ) = 1 n S p ( K , ) .

For τ [ 1 , 1 ] , the function φ τ : [ 0 , ) was defined, in [22], by

(1.4) φ τ ( t ) = | t | + τ t .

Now, we begin to define the general (p,q)-mixed projection bodies.

Definition 1.1

Suppose p 1 , q and τ [ 1 , 1 ] . If K K o n while Q S o n , then for u S n 1 , define the general (p,q)-mixed projection body, Π p , q τ ( K , Q ) , to be the convex body whose support function is given by

(1.5) h Π p , q τ ( K , Q ) , u p = n c n , p ( τ ) S n 1 φ τ ( u v ) p d C ˜ p , q ( K , Q , v ) .

Here,

c n , p ( τ ) = c n , p ( 1 + τ ) p + ( 1 τ ) p , where c n , p = Γ n + p 2 π ( n 1 ) / 2 Γ 1 + p 2 .

If we take Q = K or q = n in (1.5), then from (1.2) or (1.3) we have

Π p , q τ ( K , Q ) = Π p τ K ,

where Π p τ K is the general L p projection body [22] of K, whose support function is given by

(1.6) h Π p τ K , u p = c n , p ( τ ) S n 1 φ τ ( u v ) p d S p ( K , v ) .

For τ = 0 in (1.6), Π p τ K = Π p K which is the L p projection body [17]. For τ = 0 and p = 1 in (1.6), the body Π p τ K is the classical projection body, Π K , of K.

Our main results are as follows for the general (p,q)-mixed projection bodies. The first result is to establish the extreme values of V Π p , q τ , . Note that Π p , q τ , is used to denote the polar body of Π p , q τ .

Theorem 1.1

Suppose p 1 and q . If K K o n while L S o n , then for every τ [ 1 , 1 ] ,

(1.7) V Π p , q ( K , Q ) V Π p , q τ , ( K , Q ) V Π p , q ± , ( K , Q ) .

Suppose that both K and Q are not origin-symmetric. If τ 0 , then equality holds in the left inequality if and only if Π p , q τ ( K , Q ) is origin-symmetric; if τ ± 1 , then equality holds in the right inequality if and only if both Π p , q ± ( K , Q ) are origin-symmetric.

Here, Π p , q + ( K , Q ) is the nonsymmetric (p,q)-mixed projection body, which is the convex body defined by

(1.8) h Π p , q + ( K , Q ) , u p = n c n , p S n 1 ( u v ) + p d C ˜ p , q ( K , Q , v )

for u S n 1 , where ( u v ) + = max { u v , 0 } . Moreover, Π p , q ( K , Q ) and Π p , q ( K , Q ) are, respectively, defined by

(1.9) Π p , q ( K , Q ) Π p , q 0 ( K , Q )

and

(1.10) Π p , q ( K , Q ) Π p , q + ( K , Q ) .

The special case Q = K or q = n of Theorem 1.1 can be found in [22], which gives rise to the strongest L p Petty projection inequality. L p Petty projection inequality is one of the crucial tools used for establishing the sharp affine L p Sobolev inequalities and the affine Pólya-Szegö principle which are stronger than the usual sharp Sobolev inequalities and the usual Pólya-Szegö principle in the Euclidean space, see, e.g., [24,25,26,27].

The following is to provide the extreme values of V ( Π p , q τ ) .

Theorem 1.2

Suppose p 1 and q . If K K o n while L S o n , then for every τ [ 1 , 1 ] ,

(1.11) V Π p , q ( K , Q ) V Π p , q τ ( K , Q ) V Π p , q ± ( K , Q ) .

Suppose that both K and Q are not origin-symmetric. If τ 0 , then equality holds in the left inequality if and only if Π p , q τ ( K , Q ) is origin-symmetric; if τ ± 1 , then equality holds in the right inequality if and only if both Π p , q ± ( K , Q ) are origin-symmetric.

When Q = K or q = n , Theorem 1.2 was given by Haberl and Schuster [22].

For quick later reference, we list in Section 2 some basic and well-known facts of convex and star bodies, radial and reverse radial Gauss images and L p dual curvature measures. The basic properties of the general and nonsymmetric (p,q)-mixed projection bodies are developed in Section 3. Section 4 is devoted to prove Theorems 1.1 and 1.2.

2 Preliminaries

2.1 Basics regarding convex and star bodies

Good general references about the theory of convex bodies are the books of Gardner [47] and Schneider [10].

Let S L ( n ) denote the group of special linear transformation. If ϕ S L ( n ) , then we write ϕ t for the transpose of ϕ , ϕ 1 for the inverse of ϕ and ϕ t for the inverse of the transpose of ϕ . From the definitions of the support function, radial function and polar body, it is easy to see that for ϕ S L ( n ) , K K o n and L S o n ,

(2.1) h ( ϕ K , x ) = h ( K , ϕ t x ) , x n ;

(2.2) ρ ( ϕ K , x ) = ρ ( K , ϕ 1 x ) , x n \ { 0 } ;

(2.3) ( ϕ K ) = ϕ t K .

Moreover, it is easy to verify that for K K o n and c > 0 ,

(2.4) ( c K ) = 1 c K .

Suppose p . If μ is a Borel measure on S n 1 and ϕ S L ( n ) , then the L p image of μ under ϕ , ϕ p μ , is a Borel measure defined, in [42], by

(2.5) S n 1 f ( u ) d ϕ p μ ( u ) = S n 1 | ϕ 1 u | p f ( ϕ 1 u ) d μ ( u ) ,

for each Borel f : S n 1 .

The support and radial functions of a convex body K K o n and its polar body are related by

(2.6) ρ K = 1 / h K and h K = 1 / ρ K .

If K i K n , we say that K i K 0 K n provided

| h K i h K 0 | max u S n 1 | h K i ( u ) h K 0 ( u ) | 0 .

For K , L K n and α , β 0 (both not zero), the Minkowski combination α K + β L is defined by

α K + β L = { α x + β y : x K , y L }

whose support function is

(2.7) h α K + β L = α h K + β h L .

In the early 1960s, Firey [48] introduced the L p Minkowski combination, which is also known as the Minkowski-Firey combination. For p 1 , K , L K o n and α , β 0 (both not zero), the L p Minkowski combination, α K + p β L , was defined by

(2.8) h ( α K + p β L , ) p = α h ( K , ) p + β h ( L , ) p ,

where α K = α 1 p K .

In [48], Firey also established the L p Brunn-Minkowski inequality: if p 1 and K , L K o n , then

(2.9) V ( K + p L ) p n V ( K ) p n + V ( L ) p n ,

with equality if and only if K and L are dilates.

The L p harmonic radial combination of two star bodies was introduced by Lutwak [12]. For p 1 , K , L S o n and α , β 0 (both not zero), the L p harmonic radial combination, α K + ˜ p β L , is a star body whose radial function is given by

(2.10) ρ ( α K + ˜ p β L , ) p = α ρ ( K , ) p + β ρ ( L , ) p .

Note that α K = α 1 p K .

Lutwak’s L p dual Brunn-Minkowski inequality, see [12], is as follows: if p 1 and K , L S o n , then

(2.11) V ( K + ˜ p L ) p n V ( K ) p n + V ( L ) p n ,

with equality if and only if K and L are dilates.

2.2 Radial and reverse radial Gauss images

In the following, we state some necessary facts with regard to the radial and reverse radial Gauss images, cf. [41,42].

For K K o n and v S n 1 , the set

(2.12) H K ( v ) = { x n : x v = h K ( v ) }

is called the supporting hyperplane of K with the outer unit normal v.

The spherical image of σ K , K K o n , is defined by

ν K ( σ ) = { v S n 1 : x H K ( v ) for some x σ } S n 1 .

Let σ K K be the set consisting of all x K for which the set ν K ( { x } ) , often abbreviated as ν K ( x ) , contains more than a single element. Then, n 1 ( σ K ) = 0 based on Schneider [10, p. 84], where n 1 is the ( n 1 ) -dimensional Hausdorff measure on K . For x K \ σ K , ν K ( x ) has the unique element denoted by ν K ( x ) called the spherical image map of K. For convenience, we abbreviate K \ σ K as K . If the integration is with respect to n 1 , then it follows from n 1 ( σ K ) = 0 that it will be immaterial over subsets of K or K .

For K K o n and ω S n 1 , the radial Gauss image of ω , α K ( ω ) , is defined by

α K ( ω ) = { v S n 1 : ρ K ( u ) u H K ( v ) for some u ω } .

Thus for u S n 1 ,

(2.13) α K ( u ) = { v S n 1 : ρ K ( u ) u H K ( v ) } .

Let ω K = { u S n 1 : ρ K ( u ) u σ K } S n 1 . Clearly, if u S n 1 \ ω K , then α K ( u ) contains only a single element denoted by α K ( u ) , i.e.,

α K : S n 1 \ ω K S n 1 ,

which is named as the radial Gauss map of K. Combining (2.12) and (2.13), we obtain two essential facts needed: for λ > 0 ,

(2.14) α λ K = α K ;

(2.15) α K ( u ) = α K ( u ) , for u S n 1 .

Let K K o n and η S n 1 . The reverse radial Gauss image of η , α K ( η ) , is defined by

(2.16) α K ( η ) = { u S n 1 : ρ K ( u ) u H K ( v ) for some v η } .

Together (2.12) with (2.16), it is easy to see that for λ > 0 ,

(2.17) α λ K = α K .

2.3 L p dual curvature measures

The following are some key properties, shown in [42] and needed in next section, of the L p dual curvature measures.

In [42], Lutwak et al. showed that for p , q , K K o n and Q S o n , definition (1.1) can also be written as:

(2.18) S n 1 g ( v ) d C ˜ p , q ( K , Q , v ) = 1 n K g ( ν K ( x ) ) ( x ν K ( x ) ) 1 p x Q q n d n 1 ( x ) .

The L p dual curvature measures have the following integral representation (see [42]): if p , q , K K o n and Q S o n , then

(2.19) C ˜ p , q ( K , Q , η ) = 1 n a K ( η ) h K ( α K ( u ) ) p ρ K q ( u ) ρ Q n q ( u ) d u

for each Borel set η S n 1 . Glancing (2.14) and (2.17), it immediately follows from (2.19) that for λ > 0 ,

(2.20) C ˜ p , q ( λ K , Q , η ) = λ q p C ˜ p , q ( K , Q , η ) .

It was shown, in [42], that if p 0 and q 0 , then for K K o n , Q S o n and all ϕ S L ( n ) ,

(2.21) C ˜ p , q ( ϕ K , ϕ Q , ) = ϕ p t C ˜ p , q ( K , Q , ) .

The L p dual curvature measures are weakly convergent (see [42]): if p , q , Q S o n and K i K o n with K i K 0 K o n , then for each continuous function g : S n 1 ,

(2.22) lim i S n 1 g ( v ) d C ˜ p , q ( K i , Q , v ) = S n 1 g ( v ) d C ˜ p , q ( K 0 , Q , v ) .

Moreover, they are a valuation (see [42]), i.e., if K , L K o n are such that K L K o n , then

(2.23) C ˜ p , q ( K , Q , ) + C ˜ p , q ( L , Q , ) = C ˜ p , q ( K L , Q , ) + C ˜ p , q ( K L , Q , ) .

3 General and nonsymmetric (p,q)-mixed projection bodies

In this section, we first show the relation between general and nonsymmetric (p,q)-mixed projection bodies. Then, some of their basic properties are established.

Let g ( v ) = φ τ ( u v ) p , with p 1 , in (2.18). Then, it will be easy to see that definition (1.5) can be rewritten as:

(3.1) h Π p , q τ ( K , Q ) , u p = c n , p ( τ ) K φ τ ( u ν K ( x ) ) p ( x ν K ( x ) ) 1 p x Q q n d n 1 ( x ) .

From the definition of Π p , q ( K , Q ) , (1.8), (1.1) and (2.15), it follows that for p 1 , K K o n and Q S o n ,

(3.2) h Π p , q ( K , Q ) , u p = n c n , p S n 1 ( u v ) + p d C ˜ p , q ( K , Q , v ) , u S n 1 .

Since for any u , v S n 1 ,

φ τ ( u v ) p = ( 1 + τ ) p ( u v ) + p + ( 1 τ ) p ( u v ) + p ,

by (1.5), (1.8), (3.2) and (2.8) we have

(3.3) Π p , q τ ( K , Q ) = f 1 ( τ ) Π p , q + ( K , Q ) + p f 2 ( τ ) Π p , q ( K , Q ) ,

where

f 1 ( τ ) = ( 1 + τ ) p ( 1 + τ ) p + ( 1 τ ) p and f 2 ( τ ) = ( 1 τ ) p ( 1 + τ ) p + ( 1 τ ) p .

Note that

f 1 ( τ ) + f 2 ( τ ) = 1 ,

f 1 ( τ ) = f 2 ( τ ) and f 2 ( τ ) = f 1 ( τ ) .

From (3.3), we see that if τ = ± 1 , then

(3.4) Π p , q + 1 ( K , Q ) = Π p , q + ( K , Q ) and Π p , q 1 ( K , Q ) = Π p , q ( K , Q ) ;

if τ = 0 , then

(3.5) Π p , q ( K , Q ) = 1 2 Π p , q + ( K , Q ) + p 1 2 Π p , q ( K , Q ) .

We first show the property of Π p , q ± .

Proposition 3.1

Suppose p 1 , q . If K K o n while Q S o n , then

(3.6) Π p , q + ( K , Q ) = Π p , q ( K , Q ) = Π p , q + ( K , Q ) .

Proof

We just need to prove the left equality. From (3.2) and (1.8), it follows that for any u S n 1 ,

h Π p , q ( K , Q ) , u p = n c n , p S n 1 ( u v ) + p d C ˜ p , q ( K , Q , v ) = h Π p , q + ( K , Q ) , u p = h Π p , q + ( K , Q ) , u p ,

i.e.,

Π p , q ( K , Q ) = Π p , q + ( K , Q ) .

This finishes the proof.□

The following is to show the properties of Π p , q τ .

Proposition 3.2

Suppose p 1 , q , K K o n while Q S o n .

  1. If τ [ 1 , 1 ] , then

    (3.7) Π p , q τ ( K , Q ) = Π p , q τ ( K , Q ) = Π p , q τ ( K , Q ) ;

  2. If τ 0 , then

(3.8) Π p , q τ ( K , Q ) = Π p , q τ ( K , Q ) Π p , q + ( K , Q ) = Π p , q ( K , Q ) .

Proof

  1. By (3.3) and (3.6), we have

    (3.9) Π p , q τ ( K , Q ) = f 2 ( τ ) Π p , q + ( K , Q ) + p f 1 ( τ ) Π p , q ( K , Q ) = f 2 ( τ ) Π p , q ( K , Q ) + p f 1 ( τ ) Π p , q + ( K , Q ) = Π p , q τ ( K , Q ) .

    Moreover, from (3.3), (2.8), (3.6) and (2.8) again, we get that for any u S n 1 ,

    h Π p , q τ ( K , Q ) , u p = f 2 ( τ ) h Π p , q + ( K , Q ) , u p + f 1 ( τ ) h Π p , q ( K , Q ) , u p = f 2 ( τ ) h Π p , q ( K , Q ) , u p + f 1 ( τ ) h Π p , q + ( K , Q ) , u p = h f 1 ( τ ) Π p , q + ( K , Q ) + p f 2 ( τ ) Π p , q ( K , Q ) , u p = h Π p , q τ ( K , Q ) , u p ,

    i.e.,

    (3.10) Π p , q τ ( K , Q ) = Π p , q τ ( K , Q ) .

    Together (3.9) with (3.10) gives

    Π p , q τ ( K , Q ) = Π p , q τ ( K , Q ) = Π p , q τ ( K , Q ) .

  2. Let τ 0 and Π p , q + ( K , Q ) = Π p , q ( K , Q ) . We know that for any u S n 1 ,

(3.11) h Π p , q τ ( K , Q ) , u p = f 1 ( τ ) h Π p , q + ( K , Q ) , u p + f 2 ( τ ) h Π p , q ( K , Q ) , u p

and

(3.12) h Π p , q τ ( K , Q ) , u p = f 2 ( τ ) h Π p , q + ( K , Q ) , u p + f 1 ( τ ) h Π p , q ( K , Q ) , u p .

Together (3.11) with (3.12), it follows that

Π p , q τ ( K , Q ) = Π p , q τ ( K , Q ) .

Moreover, let Π p , q τ ( K , Q ) = Π p , q τ ( K , Q ) . Combining (3.11) with (3.12), we have

(3.13) [ f 1 ( τ ) f 2 ( τ ) ] h Π p , q + ( K , Q ) , u p = [ f 1 ( τ ) f 2 ( τ ) ] h Π p , q ( K , Q ) , u p .

Since f 1 ( τ ) f 2 ( τ ) 0 when τ 0 , it follows from (3.13) that

Π p , q + ( K , Q ) = Π p , q ( K , Q ) .

□Next, we will show that the operator Π p , q τ ( , ) is S L ( n ) contravariant and homogeneous of q / p 1 with respect to the first part.

Proposition 3.3

Suppose p 1 , q , τ [ 1 , 1 ] , K K o n while Q S o n .

  1. For all ϕ S L ( n ) ,

    (3.14) Π p , q τ ( ϕ K , ϕ Q ) = ϕ t Π p , q τ ( K , Q ) ;

  2. For λ > 0 ,

(3.15) Π p , q τ ( λ K , Q ) = λ q / p 1 Π p , q τ ( K , Q ) .

Proof

  1. From (1.5), (2.21), (2.5), (1.5) again and (2.1), we have that for any u S n 1 and all ϕ S L ( n ) ,

    h Π p , q τ ( ϕ K , ϕ Q ) , u p = n c n , p ( τ ) S n 1 φ τ ( u v ) p d C ˜ p , q ( ϕ K , ϕ Q , v ) = n c n , p ( τ ) S n 1 φ τ ( u v ) p d ϕ p t C ˜ p , q ( K , Q , v ) = n c n , p ( τ ) S n 1 | ϕ t v | p φ τ ( u ϕ t v ) p d C ˜ p , q ( K , Q , v ) = n c n , p ( τ ) S n 1 φ τ ( u ϕ t v ) p d C ˜ p , q ( K , Q , v ) = n c n , p ( τ ) S n 1 φ τ ( ϕ 1 u v ) p d C ˜ p , q ( K , Q , v ) = h Π p , q τ ( K , Q ) , ϕ 1 u p = h ϕ t Π p , q τ ( K , Q ) , u p ,

    i.e.,

    Π p , q τ ( ϕ K , ϕ Q ) = ϕ t Π p , q τ ( K , Q ) .

  2. By (1.5) and (2.20), it follows that for any u S n 1 and λ > 0 ,

h Π p , q τ ( λ K , Q ) , u p = n c n , p ( τ ) S n 1 φ τ ( u v ) p d C ˜ p , q ( λ K , Q , v ) = λ q p h Π p , q τ ( K , Q ) , u p = h λ q / p 1 Π p , q τ ( K , Q ) , u p .

That is,

Π p , q τ ( λ K , Q ) = λ q / p 1 Π p , q τ ( K , Q ) .

For a fixed Q S o n , we will prove that Π p , q τ ( , Q ) : K o n K o n is continuous.□

Proposition 3.4

Suppose p 1 , q and Q S o n . If K i K o n with K i K 0 K o n , then for every τ [ 1 , 1 ] ,

(3.16) Π p , q τ ( K i , Q ) Π p , q τ ( K 0 , Q ) .

Proof

Suppose u 0 S n 1 . From (1.5) and (2.22), we get for a fixed Q S o n ,

h Π p , q τ ( K i , Q ) , u 0 h Π p , q τ ( K 0 , Q ) , u 0 , as i .

The support functions h Π p , q τ ( K i , Q ) h Π p , q τ ( K 0 , Q ) pointwise on S n 1 imply that they converge uniformly (see [10, Theorem 1.8.15]). This finishes the proof.□

An operator Z : K o n K o n is called an L p Minkowski valuation if

Z K 1 + p Z K 2 = Z ( K 1 K 2 ) + p Z ( K 1 K 2 ) ,

whenever K 1 , K 2 , K 1 K 2 K o n .

The theory of real valued valuations lies at the very core of geometry, see, e.g., [49,50]. In the 1970s, Schneider [51] first obtained the results on a special class of Minkowski valuations. Recently, since the seminal work of Ludwig [3,21], the investigations of these Minkowski valuations have become the focus of increased attention, see, e.g., [52,53,54,55,56,57,58,59].

An immediate result of (2.23) is that for a fixed Q S o n , Π p , q τ ( , Q ) : K o n K o n is an L p Minkowski valuation.

Proposition 3.5

Suppose, q and Q S o n . Then, for every τ [ 1 , 1 ] ,

Π p , q τ ( , Q ) : K o n K o n

is an L p Minkowski valuation, i.e., if K , L K o n are such that K L K o n , then

Π p , q τ ( K , Q ) + p Π p , q τ ( L , Q ) = Π p , q τ ( K L , Q ) + p Π p , q τ ( K L , Q ) .

4 Proofs of Theorems 1.1–1.2

This section is dedicated to give the proofs of Theorems 1.1–1.2.

Proof of Theorem 1.1

Suppose that both K and Q are not origin-symmetric (otherwise the result is trivial). We first show the right inequality. Let 1 < τ < 1 . From (3.3), (2.8), (2.6) and (2.10), it follows that

(4.1) Π p , q τ , ( K , Q ) = f 1 ( τ ) Π p , q + , ( K , Q ) + ˜ p f 2 ( τ ) Π p , q , ( K , Q ) .

Using the L p dual Brunn-Minkowski inequality (2.11), (3.6) and (2.4), and note that α K = α 1 p K , we have

V Π p , q τ , ( K , Q ) V Π p , q ± , ( K , Q ) ,

with equality if and only if Π p , q + , ( K , Q ) and Π p , q , ( K , Q ) are dilates, which is equivalent to Π p , q + ( K , Q ) = Π p , q ( K , Q ) . Since Π p , q ( K , Q ) = Π p , q + ( K , Q ) and Π p , q + ( K , Q ) = Π p , q ( K , Q ) , Π p , q + ( K , Q ) = Π p , q ( K , Q ) implies that both Π p , q + ( K , Q ) and Π p , q ( K , Q ) are origin-symmetric and vice versa.

Next, we prove the left inequality. Let τ 0 . From (4.1) and (2.10), it follows that for any u S n 1 ,

(4.2) ρ Π p , q τ , ( K , Q ) , u p = f 1 ( τ ) ρ Π p , q + , ( K , Q ) , u p + f 2 ( τ ) ρ Π p , q , ( K , Q ) , u p

and

(4.3) ρ Π p , q τ , ( K , Q ) , u p = f 2 ( τ ) ρ Π p , q + , ( K , Q ) , u p + f 1 ( τ ) ρ Π p , q , ( K , Q ) , u p .

Combining (4.2) and (4.3), we get

1 2 ρ Π p , q τ , ( K , Q ) , u p + 1 2 ρ Π p , q τ , ( K , Q ) , u p = 1 2 ρ Π p , q + , ( K , Q ) , u p + 1 2 ρ Π p , q , ( K , Q ) , u p .

This together (2.10), (2.8) with (3.5) yields

(4.4) Π p , q ( K , Q ) = 1 2 Π p , q τ , ( K , Q ) + ˜ p 1 2 Π p , q τ , ( K , Q ) .

By inequalities (2.11), (3.7) and (2.4), this has

V Π p , q ( K , Q ) V Π p , q τ , ( K , Q ) ,

with equality if and only if Π p , q τ , ( K , Q ) and Π p , q τ , ( K , Q ) are dilates, which is equivalent to Π p , q τ ( K , Q ) = Π p , q τ ( K , Q ) . From (3.7), Π p , q τ ( K , Q ) = Π p , q τ ( K , Q ) yields that Π p , q τ ( K , Q ) is origin-symmetric and vice versa.□

We will use the following consequence (see [22]).

Lemma 5.1

If K K o n and p is not an odd integer, then

Π p + K = Π p K K i s o r i g i n s y m m e t r i c .

Here, Π p ± K denote the nonsymmetric L p projection bodies (see [22]).

Let Q = K or q = n in Theorem 1.1. Then, we immediately have the following result given by Haberl and Schuster [22], where the equality conditions follow from Lemma 5.1 and the case Q = K or q = n of (3.8).

Corollary 5.1

[22] For p 1 , τ [ 1 , 1 ] and K K o n ,

V Π p K V Π p τ , K V Π p ± , K .

If K is not origin-symmetric and p is not an odd integer, equality holds in the left inequality if and only if τ = 0 and equality holds in the right inequality if and only if τ = ± 1 .

Proof of Theorem 1.2

Assume that both K and Q are not origin-symmetric. First, we deduce the right inequality. Let 1 < τ < 1 . Then it follows from (3.3), the L p Brunn-Minkowski inequality (2.9) and the fact that α K = α 1 p K that

V Π p , q τ ( K , Q ) V Π p , q ± ( K , Q ) ,

with equality if and only if Π p , q + ( K , Q ) and Π p , q ( K , Q ) are dilates, which is equivalent to Π p , q + ( K , Q ) = Π p , q ( K , Q ) , i.e., Π p , q ± ( K , Q ) are origin-symmetric.

In order to see the left inequality, we suppose τ 0 . From (4.4), (2.6) and (2.8), we have

Π p , q ( K , Q ) = 1 2 Π p , q τ ( K , Q ) + p 1 2 Π p , q τ ( K , Q ) .

Using inequality (2.9) and equality (3.7), this gets

V Π p , q ( K , Q ) V Π p , q τ ( K , Q ) ,

with equality if and only if Π p , q τ ( K , Q ) and Π p , q τ ( K , Q ) are dilates, which is equivalent to Π p , q τ ( K , Q ) = Π p , q τ ( K , Q ) . That is, Π p , q τ ( K , Q ) is origin-symmetric.

As a special case of Theorem 1.2, the following is a direct result. Note that the proof of the equality conditions is similar to that of Corollary 5.1.

Corollary 5.2

[22] For p 1 , τ [ 1 , 1 ] and K K o n ,

V Π p K V Π p τ K V Π p ± K .

If K is not origin-symmetric and p is not an odd integer, equality holds in the left inequality if and only if τ = 0 and equality holds in the right inequality if and only if τ = ± 1 .

Acknowledgments

This work was supported by the National Natural Science Foundation of China (Grant No. 11901346) and Innovation Foundation of Institutions of Higher Learning of Gansu (Grant No. 2020A-108). The authors want to express earnest thankfulness for the referees who provided extremely precious and helpful comments and suggestions.

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Received: 2019-12-09
Revised: 2020-06-25
Accepted: 2020-07-01
Published Online: 2020-09-15

© 2020 Yibin Feng and Yanping Zhou, published by De Gruyter

This work is licensed under the Creative Commons Attribution 4.0 International License.

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