1 Introduction and main results
The setting for this paper is the Euclidean n-space \(\mathbb{R}^{n}\). We use \(S^{n-1}\) and \(V(K)\) to denote the unit sphere and the n-dimensional volume of a body K, respectively. For the standard unit ball B, we write \(V(B)=\omega _{n}\).
If
K is a nonempty compact convex set in
\(\mathbb{R}^{n}\), then the support function of
K,
\(h_{K}=h(K,\cdot ): \mathbb{R}^{n}\rightarrow \mathbb{R}\), is defined by (see [
1])
$$ h(K,x)= \max \{x\cdot y: y\in K\} $$
for
\(x\in \mathbb{R}^{n}\), where
\(x\cdot y\) is the standard inner product of
x and
y. If
K is a compact convex set with nonempty interiors in
\(\mathbb{R}^{n}\), then
K is called a convex body. Let
\(\mathcal{K}^{n}\) denote the set of convex bodies in
\(\mathbb{R}^{n}\).
The radial function
\(\rho _{K}=\rho (K,\cdot ): \mathbb{R}^{n}\setminus \{0\}\rightarrow [0,\infty )\) of a compact star-shaped (about the origin) set
\(K\subset \mathbb{R}^{n}\) is defined by (see [
1])
$$ \rho (K,x)=\max \{\lambda \geq 0: \lambda x\in K\},\quad x\in \mathbb{R}^{n}\setminus \{0\}. $$
If
\(\rho _{K}\) is continuous, then
K will be called a star body (about the origin). Let
\(\mathcal{S}^{n}_{o}\) denote the subset of star bodies containing the origin in
\(\mathbb{R}^{n}\). Two star bodies
K and
L are dilates (of one another) if
\(\rho _{K}(u)/\rho _{L}(u)\) is independent of
\(u\in S^{n-1}\).
The research of width-integrals has a long history. The width-integrals were first considered by Blaschke (see [
2]) and were further researched by Hadwiger (see [
3]). In 1975, Lutwak [
4] gave the
ith width-integrals as follows:
For
\(K\in \mathcal{K}^{n}\) and any real
i, the
ith width-integrals
\(B_{i}(K)\) of
K are defined by
$$ B_{i}(K)=\frac{1}{n} \int _{S^{n-1}}b(K,u)^{n-i}\,dS(u). $$
(1.1)
Here
\(b(K,u)\) denotes the half width of
K in the direction
\(u\in S^{n-1}\) which is defined by
\(b(K,u)=\frac{1}{2}h(K,u)+ \frac{1}{2}h(K,-u)\). If there exists a constant
\(\lambda >0\) such that
\(b(K,u)=\lambda b(L,u)\) for all
\(u\in S^{n-1}\), then
K and
L are said to have similar width. Further, Lutwak [
4] established the following Brunn–Minkowski inequality and cyclic inequality for the
ith width-integrals, respectively.
Whereafter, Lutwak [
5] showed that the mixed width-integral
\(B(K_{1},\ldots,K_{n})\) of
\(K_{1},\ldots, K_{n}\in \mathcal{K}^{n}\) was defined by
$$ B(K_{1},\ldots,K_{n})=\frac{1}{n} \int _{S^{n-1}}b(K_{1},u)\cdots b(K_{n},u) \,dS(u). $$
(1.2)
In 2016, based on (
1.2), Feng [
6] introduced the general mixed width-integrals as follows: For
\(K_{1},\ldots,K_{n}\in \mathcal{K} ^{n}\) and
\(\tau \in (-1,1)\), the general mixed width-integral
\(B^{(\tau )}(K_{1},\ldots,K_{n})\) of
\(K_{1}, \ldots, K_{n}\) is given by
$$ B^{(\tau )}(K_{1},\ldots,K_{n})= \frac{1}{n} \int _{S^{n-1}}b^{(\tau )}(K _{1},u)\cdots b^{(\tau )}(K_{n},u)\,dS(u), $$
(1.3)
where
\(b^{\tau }(K,u)=f_{1}(\tau )h(K,u)+f_{2}(\tau )h(K,-u)\) and
$$ f_{1}(\tau )=\frac{(1+\tau )^{2}}{2(1+\tau ^{2})},\qquad f_{2}(\tau )=\frac{(1-\tau )^{2}}{2(1+\tau ^{2})}. $$
(1.4)
Obviously,
$$\begin{aligned}& f_{1}(\tau )+f_{2}(\tau )=1; \\& f_{1}(-\tau )=f_{2}(\tau ),\qquad f_{2}(- \tau )=f_{1}(\tau ). \end{aligned}$$
Combined with (
1.4), the case of
\(\tau =0\) in (
1.3) is just (
1.2). If there exists a constant
\(\lambda >0\) such that
\(b^{\tau }(K,u)=\lambda b^{\tau }(L,u)\) for all
\(u\in S^{n-1}\), then we say convex bodies
K and
L have similar general width.
K and
L have joint constant general width means that
\(b^{(\tau )}(K,u)b^{(\tau )}(L,u)\) is a constant for all
\(u\in S^{n-1}\).
Taking
\(K_{1}=\cdots=K_{n-i}=K\),
\(K_{n-i+1}=\cdots=K_{n}=B\) in (
1.3) and allowing
i to be any real, the general
ith width-integrals
\(B_{i}^{(\tau )}(K)\) of
\(K\in \mathcal{K}^{n}\) were given by (see [
6])
$$ B_{i}^{(\tau )}(K)=\frac{1}{n} \int _{S^{n-1}}b^{(\tau )}(K,u)^{n-i}\,dS(u). $$
(1.5)
From (
1.1), (
1.4), and (
1.5), we easily see that if
\(\tau =0\), then
\(B_{i}^{(0)}(K)=B_{i}(K)\).
In 2006, motivated by Lutwak’s
ith width-integrals and together with the notion of radial function, Li, Yuan, and Leng [
7] gave the
ith chord-integrals as follows: For
\(K\in \mathcal{S}_{o}^{n}\) and
i is any real, the
ith chord-integrals
\(C_{i}(K)\) of
K are defined by
$$ C_{i}(K)=\frac{1}{n} \int _{S^{n-1}}c(K,u)^{n-i}\,dS(u). $$
(1.6)
Here
\(c(K,u)\) denotes the half chord of
K in the direction
u and
\(c(K,u)=\frac{1}{2}\rho (K,u)+\frac{1}{2}\rho (K,-u)\). If there exists a constant
\(\lambda >0\) such that
\(c(K,u)=\lambda c(L,u)\) for all
\(u\in \mathcal{S}^{n-1}\), then we say that
K and
L have similar chord.
For the
ith chord-integrals, the authors [
7] proved the following Brunn–Minkowski inequality and cyclic inequality.
The mixed chord-integrals of star bodies were defined by Lu (see [
8]): For
\(K_{1},\ldots,K_{n}\in \mathcal{S}_{o}^{n}\), the mixed chord-integrals
\(C(K_{1},\ldots,K_{n})\) of
\(K_{1}, \ldots, K_{n}\) are defined by
$$ C(K_{1},\ldots,K_{n})=\frac{1}{n} \int _{S^{n-1}}c(K_{1},u)\cdots c(K_{n},u) \,dS(u). $$
Recently, Feng and Wang [
9] gave the general mixed chord-integrals
\(C^{(\tau )}(K_{1},\ldots,K_{n})\) of
\(K_{1},\ldots,K_{n} \in \mathcal{S}_{o}^{n}\) defined by
$$ C^{(\tau )}(K_{1},\ldots,K_{n})= \frac{1}{n} \int _{S^{n-1}}c^{(\tau )}(K _{1},u)\cdots c^{(\tau )}(K_{n},u)\,dS(u), $$
(1.7)
where
\(c^{(\tau )}(K,u)=f_{1}(\tau )\rho (K,u)+f_{2}(\tau )\rho (K,-u)\) and functions
\(f_{1}(\tau )\),
\(f_{2}(\tau )\) satisfy (
1.4). By (
1.4), let
\(\tau =0\) in (
1.7), this is just Lu’s mixed chord-integrals
\(C(K_{1},\ldots,K_{n})\). Star bodies
K and
L are said to have similar general chord mean that there exist constants
\(\lambda , \mu >0\) such that
\(\lambda c^{(\tau )}(K,u)=\mu c^{(\tau )}(L,u)\) for all
\(u\in S^{n-1}\). If the product
\(c^{(\tau )}(K,u)c^{(\tau )}(L,u)\) is constant for all
\(u\in S^{n-1}\), then they are said to have joint constant general chord.
Taking
\(K_{1}=\cdots=K_{n-i}=K\) and
\(K_{n-i+1}=\cdots=K_{n}=B\) in (
1.7) and allowing
i to be any real, the general
ith chord-integral
\(C_{i}^{(\tau )}(K)\) of
\(K\in \mathcal{S}_{o}^{n}\) was given by (see [
9])
$$ C_{i}^{(\tau )}(K)=\frac{1}{n} \int _{S^{n-1}}c^{(\tau )}(K,u)^{n-i}\,dS(u). $$
(1.8)
Obviously, (
1.4), (
1.6), and (
1.8) give
\(C_{i}^{(0)}(K)=C_{i}(K)\).
In this paper, based on Theorems
1.A–
1.B and Theorems
1.C–
1.D, we respectively establish two cyclic Brunn–Minkowski inequalities for general
ith width-integrals and general
ith chord-integrals by using Zhao’s ideas (see [
10] and [
11]). Our works bring the cyclic inequality and Brunn–Minkowski inequality together. Our main results can be stated as follows.
Obviously, if
\(\tau =0\), then inequality (
1.11) yields Theorem
1.A, Corollary
1.2 gives Theorem
1.C, respectively.
Because of
\(\{o\}\in \mathcal{S}_{o}^{n}\), hence let
\(L=\{o\}\) in Theorem
1.2, we may obtain the following.
If
\(\tau =0\), then Corollary
1.3 and Corollary
1.4 respectively give Theorem
1.B and Theorem
1.D.
Our works belong to the asymmetric Brunn–Minkowski theory, which has its starting point in the theory of valuations in connection with isoperimetric and analytic inequalities. As an important research object in convex geometry, asymmetric Brunn–Minkowski theory has gotten rich development, readers can refer to [
12‐
19].
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