International Journal of Differential Equations
Volume 2010 (2010), Article ID 193893, 18 pages
doi:10.1155/2010/193893
Research Article

Riesz Potentials for Korteweg-de Vries Solitons and Sturm-Liouville Problems

Department of Mathematics, The University of Texas-Pan American, Edinburg, TX 78539-2999, USA

Received 9 August 2009; Accepted 9 November 2009

Academic Editor: Mark M. Meerschaert

Copyright © 2010 Vladimir Varlamov. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

Abstract

Riesz potentials (also called Riesz fractional derivatives) and their Hilbert transforms are computed for the Korteweg-de Vries soliton. They are expressed in terms of the full-range Hurwitz Zeta functions 𝜁 + ( 𝑠 , 𝑎 ) and 𝜁 ( 𝑠 , 𝑎 ) . It is proved that these Riesz potentials and their Hilbert transforms are linearly independent solutions of a Sturm-Liouville problem. Various new properties are established for this family of functions. The fact that the Wronskian of the system is positive leads to a new inequality for the Hurwitz Zeta functions.

1. Introduction

In recent years the theory of fractional derivatives and integrals called Fractional Calculus has been steadily gaining importance for applications. Ordinary and partial differential equations of fractional order have been widely used for modeling various processes in physics, chemistry, and engineering (see, e.g., [13] and the references therein). Recent theoretical developments shed new light on the interpretation and properties of fractional derivatives. Having written the latter in the form of Stieltjes integrals, Podlubny [4] found new physical and geometric interpretation of these structures relating them to inhomogeneity of time. Extension of the classical maximum principle to the case of a time-fractional diffusion equation appeared in the recent work of Luchko [5]. In the present paper we are concerned with Riesz fractional derivatives (also called Riesz potentials; see [6, page 88], and [7, page 117]) that are defined as fractional powers of the Laplacian 𝐷 𝛼 = ( Δ ) 𝛼 / 2 with 𝛼 . They are well known for their role in investigating the solvability of nonlinear partial differential equations, and the Korteweg-de Vries equation (KdV henceforth) in particular (see, e.g., [711] and the references therein). In the current work, Riesz potentials of KdV solitons are computed and their relation to ordinary differential equations is established.

We continue the study of Riesz fractional derivatives of solutions to Korteweg-de-Vries-type equations started in [12]. After appropriate rescaling, KdV can be written in the form 𝑢 𝑡 + 𝑢 𝑥 𝑥 𝑥 𝑢 + 3 2 𝑥 = 0 , 𝑥 , 𝑡 > 0 . ( 1 . 1 ) It is well known that the fundamental solution of the Cauchy problem for the linearized KdV is expressed in terms of the Airy function of the first kind 𝐴 𝑖 ( 𝑥 ) and its Hilbert transform (conjugate) in terms of the Scorer function 𝐺 𝑖 ( 𝑥 ) . The papers [1214] were devoted to the study of fractional properties of the Airy functions and their conjugates and to the establishing of related properties for KdV-type equations.

Although there exists extensive literature on solitons, as far as we know, a study of their fractional properties is still missing. A preliminary investigation of Riesz potentials for a KdV soliton was carried out in [15]. In this paper the emphasis was put on the issue of whether solitons inherit fractional properties of fundamental solutions. Riesz potentials of a soliton, 𝑢 𝛼 ( 𝑋 ) = 𝐷 𝛼 𝑢 0 ( 𝑋 ) , where 𝑢 0 ( 𝑋 ) = 2 s e c h 2 𝑋 , 𝑋 = 𝑥 4 𝑡 , and 𝐷 𝛼 = ( 𝜕 2 𝑥 ) 𝛼 / 2 , and their Hilbert transforms, 𝑣 𝛼 ( 𝑋 ) = 𝐻 𝑢 𝛼 ( 𝑋 ) , were obtained in terms of the Hurwitz Zeta function of a complex argument, 𝜁 ( 𝑠 , 𝑧 ) with 𝑠 = 2 + 𝛼 and 𝑧 = 1 / 2 + 𝑖 𝑋 / 𝜋 . It was proved in [15] that the zero mean properties hold for both 𝑢 𝛼 ( 𝑋 ) and 𝑣 𝛼 ( 𝑋 ) with 𝛼 > 0 . This confirmed the predictions based on the properties of fundamental solutions of the linearized Cauchy problems.

The goal of the current paper is to go further and to study Riesz potentials of solitons as solutions of differential equations. We intend to show that these functions and their Hilbert transforms form linearly independent systems of solutions for a second-order ordinary differential equation in a self-adjoint form. This fact may be helpful in understanding the issue of using these structures as intrinsic mode functions in signal processing (see [16, 17] and the references therein), that is, in using Riesz potentials for expansions. In this context it is interesting to point out that the graphs of the functions 𝑢 𝛼 ( 𝑋 ) reveal a striking similarity to those of the Airy wavelets generated by the function 𝐴 𝑖 ( 𝑥 ) 𝐴 𝑖 ( 𝑥 ) (see [18, page 34], and Figure 3 below).

For the analysis to follow; we employ the full-range Hurwitz Zeta functions: 𝜁 + ( 𝑠 , 𝑎 ) = 𝜁 ( 𝑠 , 𝑎 ) + 𝜁 ( 𝑠 , 1 𝑎 ) and 𝜁 ( 𝑠 , 𝑎 ) = 𝜁 ( 𝑠 , 𝑎 ) 𝜁 ( 𝑠 , 1 𝑎 ) (symmetric and antisymmetric combinations of 𝜁 ( 𝑠 , 𝑎 ) and 𝜁 ( 𝑠 , 1 𝑎 ) ), recently introduced in [19] for 𝑎 . We prove that the functions 𝑤 𝛼 ( 𝑋 ) = 𝑢 𝛼 ( 𝑋 ) + 𝑖 𝑣 𝛼 ( 𝑋 ) , 𝛼 > 1 are solutions of the Sturm-Liouville problem 𝑑 𝑃 𝑑 𝑋 𝛼 ( 𝑋 ) 𝑑 𝑤 𝑑 𝑋 + 𝑄 𝛼 ( 𝑋 ) 𝑤 = 𝜆 𝜌 𝛼 ( 𝑋 ) 𝑤 , 𝑋 , ( 1 . 2 ) l i m 𝑋 ± 𝑤 ( 𝑋 ) = 0 , ( 1 . 3 ) for 𝜆 = 1 . Here 𝑃 𝛼 ( 𝑋 ) > 0 , 𝜌 𝛼 ( 𝑋 ) > 0 , and 𝑄 𝛼 ( 𝑋 ) is a real function. The essential point consists in proving that the Wronskian of 𝑢 𝛼 ( 𝑋 ) and 𝑣 𝛼 ( 𝑋 ) is positive for all 𝛼 > 1 and 𝑥 . It allows one to prove that 𝑃 𝛼 ( 𝑋 ) and 𝜌 𝛼 ( 𝑋 ) are positive and to estimate the number of zeros of 𝑢 𝛼 ( 𝑋 ) and 𝑣 𝛼 ( 𝑋 ) on any bounded interval.

The fact that this Wronskian is positive also leads to a new inequality for the Hurwitz Zeta functions 𝜁 𝑠 , 𝑧 𝜁 ( 𝑠 + 1 , 𝑧 ) + 𝜁 ( 𝑠 , 𝑧 ) 𝜁 𝑠 + 1 , 𝑧 > 0 , ( 1 . 4 ) where 𝑠 > 1 , 𝑧 = 1 / 2 + 𝑖 𝑋 / 𝜋 , and the bar over the letter denotes complex conjugation. As far as we know, there are no results in the literature on the arguments of the Hurwitz Zeta functions. However, (1.4) provides some information on this issue. Indeed, setting 𝜁 ( 𝑠 , 𝑧 ) = 𝑟 𝑠 𝑒 𝑖 𝜑 𝑠 and 𝜁 ( 𝑠 + 1 , 𝑧 ) = 𝑟 𝑠 + 1 𝑒 𝑖 𝜑 𝑠 + 1 in (1.4) allows one to deduce the relation c o s ( 𝜑 𝑠 + 1 ( 𝑧 ) 𝜑 𝑠 ( 𝑧 ) ) > 0 for 𝑠 > 1 , 𝑧 = 1 / 2 + 𝑖 𝑋 / 𝜋 , and 𝑋 .

The paper is organized as follows. In Section 2, we provide the necessary information on the special functions involved. Section 3 is devoted to the study of Riesz potentials for KdV solitons and their Hilbert transforms. In Section 3.1, the main properties of these functions are summarized. Sturm-Liouville problem (1.2) is derived in Section 3.2. Section 3.3 deals with the properties of the Wronskian 𝑊 [ 𝑢 𝛼 , 𝑣 𝛼 ] . Zeros of the functions 𝑢 𝛼 and 𝑣 𝛼 are studied in Section 3.4. In Section 4, the inequality (1.4) is discussed.

2. Preliminaries

Introduce the Fourier transform of the function 𝑓 by 𝑓 ( 𝜉 ) = { 𝑓 } ( 𝜉 ) = 𝑒 𝑖 𝜉 𝑥 𝑓 ( 𝑥 ) 𝑑 𝑥 , ( 2 . 1 ) and the inverse Fourier transform by 𝑓 ( 𝑥 ) = 1 𝑓 1 ( 𝑥 ) = 2 𝜋 𝑒 𝑖 𝜉 𝑥 𝑓 ( 𝜉 ) 𝑑 𝜉 . ( 2 . 2 )

For real 𝛼 and 𝑥 , define Riesz potentials of a function 𝑓 ( 𝑥 ) by the formula (see [7, page 117]) 𝐷 𝛼 1 𝑓 ( 𝑥 ) = 2 𝜋 | | 𝜉 | | 𝛼 𝑓 ( 𝜉 ) 𝑒 𝑖 𝜉 𝑥 𝑑 𝜉 , ( 2 . 3 ) provided that the integral in the right-hand side exists. Define derivatives of 𝐷 𝛼 𝑥 𝑓 ( 𝑥 ) with respect to 𝛼 by 𝜕 𝑛 𝛼 𝐷 𝛼 𝑥 1 𝑓 ( 𝑥 ) = 2 𝜋 | | 𝜉 | | 𝛼 l n 𝑛 | | 𝜉 | | 𝑓 ( 𝜉 ) 𝑒 𝑖 𝜉 𝑥 𝑑 𝜉 , 𝑛 , ( 2 . 4 ) provided that these integrals exist.

Introduce the Hilbert transform of the function 𝑓 by (see [20, page 120]) 1 𝐻 𝑓 ( 𝑥 ) = 𝜋 𝑃 . 𝑉 . 𝑓 ( 𝑦 ) 𝑦 𝑥 𝑑 𝑦 , ( 2 . 5 ) where 𝑥 and 𝑃 . 𝑉 . denotes the Cauchy principal value of the integral. According to our choice of the Fourier transform ( 𝐻 𝑓 ) ( 𝜉 ) = 𝑖 s g n ( 𝜉 ) 𝑓 ( 𝜉 ) , one can see that 𝐻 2 = 𝐼 on 𝐿 𝑝 ( ) , 𝑝 1 , where 𝐼 is the identity operator. Also, 𝜕 𝑥 = 𝐻 𝐷 and 𝜕 2 𝑥 = 𝐷 2 , where the operator 𝐷 is defined by (2.3).

Next, introduce the Trigamma function by (see [21, page 260, 6.4.1]) 𝜓 𝑑 ( 𝑧 ) = 2 𝑑 𝑧 2 l n Γ ( 𝑧 ) = 0 𝑡 𝑒 𝑧 𝑡 1 𝑒 𝑡 𝑑 𝑡 , ( 𝑧 ) > 0 . ( 2 . 6 ) Notice that (see [21], page 260, 6.4.7) 𝜓 ( 𝑧 ) + 𝜓 𝑑 ( 1 𝑧 ) = 𝜋 𝑑 𝑧 { c o t ( 𝜋 𝑧 ) } . ( 2 . 7 ) Also, the following asymptotic expansion holds: 𝜓 1 ( 𝑧 ) 𝑧 + 1 2 𝑧 2 + 1 6 𝑧 3 1 + 𝑂 𝑧 5 | | | | f o r 𝑧 , a r g 𝑧 < 𝜋 . ( 2 . 8 )

The Hurwitz (generalized) Zeta function is defined by (see [22, page 88]) 𝜁 ( 𝑠 , 𝑎 ) = 𝑛 = 0 1 ( 𝑛 + 𝑎 ) 𝑠 f o r ( 𝑠 ) > 1 , 𝑎 , 𝑎 0 , 1 , 2 , . ( 2 . 9 ) This implies that 𝜕 𝑎 𝜁 ( 𝑠 , 𝑎 ) = 𝑠 𝜁 ( 𝑠 + 1 , 𝑎 ) . ( 2 . 1 0 ) This function has the integral representation 1 𝜁 ( 𝑠 , 𝑎 ) = Γ ( 𝑠 ) 0 𝑥 𝑠 1 𝑒 𝑎 𝑥 1 𝑒 𝑥 𝑑 𝑥 f o r ( 𝑠 ) > 1 , ( 𝑎 ) > 0 , ( 2 . 1 1 ) where Γ ( 𝑥 ) is the Gamma function. In two particular cases, we have (see [22]) that 𝜁 1 𝑠 , 2 = ( 2 𝑠 1 ) 𝜁 ( 𝑠 ) , ( 2 . 1 2 ) 𝜁 ( 2 , 𝑎 ) = 𝜓 ( 𝑎 ) , ( 2 . 1 3 ) where 𝜁 ( 𝑠 ) is the Riemann Zeta function.

The singularity of 𝜁 ( 𝑠 , 𝑎 ) as 𝑠 1 is given by the relation l i m 𝑠 1 1 𝜁 ( 𝑠 , 𝑎 ) Γ 𝑠 1 = ( 𝑎 ) Γ ( 𝑎 ) = 𝜓 ( 𝑎 ) . ( 2 . 1 4 ) The asymptotic expansion of 𝜁 ( 𝑠 , 𝑎 ) for large 𝑎 is (see [23]) 1 𝜁 ( 𝑠 , 𝑎 ) 2 𝑎 𝑠 + 𝑎 1 𝑠 + 1 𝑠 1 Γ ( 𝑠 ) 𝑘 = 1 𝐵 2 𝑘 ( 2 𝑘 ) ! Γ ( 2 𝑘 + 𝑠 1 ) 𝑎 2 𝑘 + 𝑠 1 | | | | , | 𝑎 | < , a r g 𝑎 < 𝜋 , ( 2 . 1 5 ) where 𝐵 𝑛 are the Bernoulli numbers.

Introduce the full-range forms of Hurwitz Zeta functions (see [19]) 𝜁 + ( 𝑠 , 𝑎 ) = 𝑛 = 1 ( 𝑛 + 𝑎 ) 2 𝑠 / 2 𝜁 , ( 2 . 1 6 ) ( 𝑠 , 𝑎 ) = 𝑛 = 0 1 ( 𝑛 + 𝑎 ) 2 𝑠 / 2 1 𝑛 = 1 ( 𝑛 + 𝑎 ) 2 𝑠 / 2 . ( 2 . 1 7 ) Representations (2.16) and (2.17) imply that 𝜁 + ( 𝑠 , 𝑎 ) = 𝜁 ( 𝑠 , 𝑎 ) + 𝜁 ( 𝑠 , 1 𝑎 ) , 𝜁 ( 𝑠 , 𝑎 ) = 𝜁 ( 𝑠 , 𝑎 ) 𝜁 ( 𝑠 , 1 𝑎 ) . ( 2 . 1 8 ) Hence, follow the symmetric and antisymmetric properties of the functions, 𝜁 + ( 𝑠 , 𝑎 ) = 𝜁 + ( 𝑠 , 1 𝑎 ) , 𝜁 ( 𝑠 , 𝑎 ) = 𝜁 ( 𝑠 , 1 𝑎 ) . ( 2 . 1 9 ) It follows from (2.16) that 𝜁 + ( 𝑠 , 𝑎 ) is a periodic function of 𝑎 , with the unit period. It is even with respect to 𝑎 = 0 and 𝑎 = 1 / 2 . The function 𝜁 ( 𝑠 , 𝑎 ) is odd about 𝑎 = 1 / 2 and 𝜁 ( 𝑠 , 1 / 2 ) = 0 . These functions satisfy the functional differential equations 𝜕 𝑎 𝜁 + ( 𝑠 , 𝑎 ) = 𝑠 𝜁 ( 𝑠 + 1 , 𝑎 ) , 𝜕 𝑎 𝜁 ( 𝑠 , 𝑎 ) = 𝑠 𝜁 + ( 𝑠 + 1 , 𝑎 ) . ( 2 . 2 0 )

Consider now that 𝑠 and denote by 𝑎 the complex conjugate of 𝑎 . Then 𝜁 ( 𝑠 , 𝑎 ) = 𝜁 ( 𝑠 , 𝑎 ) . It implies that, for 𝑎 = 𝑎 1 + 𝑖 𝑎 2 , 𝜁 + 2 ( 𝑠 , 𝑎 ) = 2 { 𝜁 ( 𝑠 , 𝑎 ) } = Γ ( 𝑠 ) 0 𝑥 𝑠 1 𝑒 𝑎 1 𝑥 c o s 𝑎 2 𝑥 1 𝑒 𝑥 𝑑 𝑥 . ( 2 . 2 1 ) In a similar way, 𝜁 ( 𝑠 , 𝑎 ) = 2 𝑖 { 𝜁 ( 𝑠 , 𝑎 ) } = 2 𝑖 Γ ( 𝑠 ) 0 𝑥 𝑠 1 𝑒 𝑎 1 𝑥 𝑎 s i n 2 𝑥 1 𝑒 𝑥 𝑑 𝑥 . ( 2 . 2 2 )

Denote by 𝑊 [ 𝑢 , 𝑣 ] the Wronskian of the functions 𝑢 ( 𝑥 ) and 𝑣 ( 𝑥 ) , that is, 𝑊 [ 𝑢 , 𝑣 ] = | 𝑢 𝑢 𝑣 𝑣 | . For reader's convenience, we present here [24, Theorem 5 . 3 ].

Theorem 2.1. Let 𝑝 ( 𝑡 ) > 0 , 𝑞 ( 𝑡 ) be real valued and continuous for 0 𝑡 𝑇 . Let 𝑢 and 𝑣 be real valued solutions of the equation 𝑝 𝑢 + 𝑞 𝑢 = 0 , ( 2 . 2 3 ) satisfying the condition [ ] 𝑝 ( 𝑡 ) 𝑊 𝑢 ( 𝑡 ) , 𝑣 ( 𝑡 ) = 𝐶 0 > 0 . ( 2 . 2 4 ) Let 𝑁 be the number of zeros of 𝑢 ( 𝑡 ) on [ 0 , 𝑇 ] . Then | | | | 𝜋 𝑁 𝐶 0 𝑇 0 𝑑 𝑡 𝑣 𝑝 ( 𝑡 ) 2 ( 𝑡 ) + 𝑢 2 | | | | ( 𝑡 ) 𝜋 . ( 2 . 2 5 )

In conclusion of this section, we would like to quote an interesting result concerning integrals over the real axis (see [25]).

Theorem 2.2. For any integrable function 𝑓 ( 𝑥 ) and 𝑔 ( 𝑥 ) = 𝑥 𝑐 2 / 𝑥 with 𝑐 = c o n s t , 𝑃 . 𝑉 . 𝑓 ( 𝑔 ( 𝑥 ) ) 𝑑 𝑥 = 𝑃 . 𝑉 . 𝑓 ( 𝑥 ) 𝑑 𝑥 . ( 2 . 2 6 ) Moreover, the above formula holds true if 𝑔 ( 𝑥 ) = 𝑥 𝑗 = 1 𝑏 𝑗 𝑥 𝑐 𝑗 , ( 2 . 2 7 ) where { 𝑏 𝑗 } is any sequence of positive constants, 𝑐 𝑗 are any real constants, and the series is convergent.

3. Fractional Derivatives of A KdV Soliton and Their Conjugates

In this section, we consider Riesz fractional derivatives of a KdV soliton and their Hilbert transforms and establish their properties. We notice that all the graphs were obtained with the Mathematica 6 software.

We take the soliton solution of (1.1) in the form 𝑢 0 ( 𝑋 ) = 2 s e c h 2 𝑋 with 𝑋 = 𝑥 4 𝑡 (see Figure 1) and introduce the function 𝑤 𝛼 ( 𝑋 ) = 𝑢 𝛼 ( 𝑋 ) + 𝑖 𝑣 𝛼 ( 𝑋 ) , ( 3 . 1 ) where 𝑢 𝛼 ( 𝑋 ) = 𝐷 𝛼 𝑢 0 ( 𝑋 ) , 𝑣 𝛼 = 𝐷 𝛼 𝐻 𝑢 0 ( 𝑋 ) . ( 3 . 2 ) Notice that the functions 𝑢 𝛼 ( 𝑋 ) and 𝑣 𝛼 ( 𝑋 ) form a conjugate pair (see [20, page 120]) since 𝑢 𝛼 ( 𝑋 ) = 𝐻 𝑣 𝛼 ( 𝑋 ) , 𝑣 𝛼 ( 𝑋 ) = 𝐻 𝑢 𝛼 ( 𝑋 ) . ( 3 . 3 )

193893.fig.001
Figure 1: Graph of the soliton 𝑢 0 ( 𝑋 ) .

The next statement was proved in [15]. Using the functions (2.16) and (2.17), we rewrite it in a more convenient form.

Theorem 3.1. The functions 𝑢 𝛼 ( 𝑋 ) and 𝑣 𝛼 ( 𝑋 ) have the following representations for 𝛼 > 1 and 𝑋 : 𝑢 𝛼 ( 𝑋 ) = 2 Γ ( 2 + 𝛼 ) 𝜋 2 + 𝛼 𝜁 + 1 2 + 𝛼 , 2 𝑋 + 𝑖 𝜋 𝑣 , ( 3 . 4 ) 𝛼 ( 𝑋 ) = 𝑖 2 Γ ( 2 + 𝛼 ) 𝜋 2 + 𝛼 𝜁 1 2 + 𝛼 , 2 𝑋 + 𝑖 𝜋 , ( 3 . 5 ) where 𝜁 + ( 𝑠 , 𝑎 ) and 𝜁 ( 𝑠 , 𝑎 ) are the full-range Hurwitz Zeta functions (see (2.16) and (2.17)) and Γ ( 𝑠 ) is the Gamma function.

3.1. Properties of the Functions 𝑢 𝛼 and 𝑣 𝛼

In this subsection, we collect the properties of the functions 𝑢 𝛼 and 𝑣 𝛼 . Some of them were established in [15] and some are given for the first time as follows.

Properties of the Functions 𝑢 𝛼 and 𝑣 𝛼
( 1 ) The functions 𝑢 𝛼 ( 𝑋 ) and 𝑣 𝛼 ( 𝑋 ) satisfy the functional differential equations 𝑢 𝛼 ( 𝑋 ) = 𝑣 𝛼 + 1 ( 𝑋 ) , 𝑣 𝛼 ( 𝑋 ) = 𝑢 𝛼 + 1 ( 𝑋 ) , ( 3 . 6 ) where 𝛼 > 1 , 𝑋 , and the prime denotes differentiation with respect to 𝑋 . This follows from (3.3) and the relation 𝑑 / 𝑑 𝑋 = 𝐻 𝐷 . ( 2 ) The functions 𝑢 𝛼 ( 𝑋 ) are even and the functions 𝑣 𝛼 ( 𝑋 ) are odd on (see [15] and Figures 14). ( 3 ) The function 𝑢 𝛼 ( 𝑋 ) is periodic with the period 𝒳 = 𝑖 𝜋 . It follows from the periodicity of 𝜁 + ( 𝑠 , 𝑎 ) with the unit period.(4)For all 𝛼 > 0 (see [15]), 𝑢 𝛼 ( 𝑋 ) 𝑑 𝑋 = 0 , 𝑣 𝛼 ( 𝑋 ) 𝑑 𝑋 = 0 . ( 3 . 7 ) These properties are reflected on the graphs (see Figures 3 and 4).(5)For all 𝛼 > 0 and 𝑛 , 𝜕 𝑛 𝛼 𝑢 𝛼 ( 𝑋 ) 𝑑 𝑋 = 0 , 𝜕 𝑛 𝛼 𝑣 𝛼 ( 𝑋 ) 𝑑 𝑋 = 0 . ( 3 . 8 ) These relations follow from the differentiation of the identities in (3.7).(6)For all 𝛼 > 0 and 𝑐 , 𝑃 . 𝑉 . 𝑢 𝛼 𝑐 𝑋 2 𝑋 𝑑 𝑋 = 0 , 𝑃 . 𝑉 . 𝑣 𝛼 𝑐 𝑋 2 𝑋 𝑑 𝑋 = 0 . ( 3 . 9 )
Moreover, 𝑃 . 𝑉 . 𝑢 𝛼 𝑋 𝑗 = 1 𝑏 𝑗 𝑋 𝑐 𝑗 𝑑 𝑋 = 0 , 𝑃 . 𝑉 . 𝑣 𝛼 𝑋 𝑗 = 1 𝑏 𝑗 𝑋 𝑐 𝑗 𝑑 𝑋 = 0 , ( 3 . 1 0 ) where 𝑏 𝑗 is any sequence of positive constants, 𝑐 𝑗 are any real constants, and the series converges. These relations follow from (3.7) and Theorem 2.2.(7)The functional sequence of Riesz potentials { 𝑢 𝛼 ( 𝑋 ) } converges pointwise to the soliton 𝑢 0 ( 𝑋 ) , and the functional sequence { 𝑣 𝛼 ( 𝑋 ) } converges pointwise to the conjugate soliton 𝑣 0 ( 𝑋 ) for 𝛼 0 + (see [15]). Notice that 𝑢 0 ( 𝑋 ) 𝑑 𝑋 = 4 , 𝑃 . 𝑉 . 𝑣 0 ( 𝑋 ) 𝑑 𝑋 = 0 ( 3 . 1 1 ) (see Figures 1 and 2). Here the conjugate soliton 𝑣 0 ( 𝑋 ) is given by 𝑣 0 ( 𝑋 ) = 2 𝑖 𝜋 2 𝜓 1 2 𝑋 + 𝑖 𝜋 𝜓 1 2 𝑋 𝑖 𝜋 . ( 3 . 1 2 ) Equation (3.12) can be recovered from (3.5) with 𝛼 = 0 thanks to (2.13).

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Figure 2: Graph of the conjugate soliton 𝑣 0 ( 𝑋 ) .
193893.fig.003
Figure 3: Graph of the fractional derivative 𝑢 3 . 8 ( 𝑋 ) .
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Figure 4: Graph of the conjugate fractional derivative 𝑣 3 . 8 ( 𝑋 ) .

Remark 3.2. The conjugate soliton (3.12) is an algebraic solitary wave for extended KdV: 𝑣 𝑡 + 𝑣 𝑥 𝑥 𝑥 𝑣 + 3 2 𝑣 𝐻 𝑣 𝐻 2 𝑥 = 0 , ( 3 . 1 3 ) obtained by applying the Hilbert transform to (1.1) and setting 𝑣 = 𝐻 𝑢 . The term “algebraic solitary wave” is explained by the fact that 𝑣 0 ( 𝑋 ) has a 1 / 𝑋 decay for large 𝑋 . More precisely (see [15]), 𝑣 0 2 ( 𝑋 ) 𝜋 1 𝑋 1 + 𝑂 𝑋 2 | | 𝑋 | | f o r . ( 3 . 1 4 )

(8)For 𝛼 0 , the functions 𝑢 𝛼 and 𝑣 𝛼 are the elements of 𝐿 2 ( ) . Moreover, they are orthogonal in the principal value sense, namely, for all 𝛼 1 , 𝛼 2 0 ,

𝑃 . 𝑉 . 𝑢 𝛼 1 ( 𝑋 ) 𝑣 𝛼 2 ( 𝑋 ) 𝑑 𝑋 = 0 . ( 3 . 1 5 ) Equations (3.12) and (3.14) imply that 𝑣 0 𝐿 2 ( ) . The fact that 𝑢 𝛼 and 𝑣 𝛼 with 𝛼 > 0 are the elements of 𝐿 2 ( ) follows from their asymptotics obtained in [15], namely, 𝑢 𝛼 ( 𝑋 ) 4 Γ ( 1 + 𝛼 ) 𝜋 2 + 𝛼 [ ] c o s ( 1 + 𝛼 ) a r c t a n ( 2 𝑋 / 𝜋 ) 1 / 4 + ( 𝑋 / 𝜋 ) 2 ( 1 + 𝛼 ) / 2 1 + 𝑂 | | 𝑋 | | 2 + 𝛼 , 𝑣 𝛼 ( 𝑋 ) 4 Γ ( 2 + 𝛼 ) 𝜋 2 + 𝛼 [ ( ] 2 s i n 1 + 𝛼 ) a r c t a n ( 2 𝑋 / 𝜋 ) ( 1 + 𝛼 ) 1 / 4 + ( 𝑋 / 𝜋 ) 2 ( 1 + 𝛼 ) / 2 1 + 𝑂 | | 𝑋 | | 2 + 𝛼 . ( 3 . 1 6 ) Orthogonality of 𝑢 𝛼 and 𝑣 𝛼 follows from the fact that all 𝑢 𝛼 ( 𝑋 ) with 𝛼 0 are even functions and all 𝑣 𝛼 ( 𝑋 ) with 𝛼 0 are odd functions of 𝑋 (see Property  2 and Figures 14).(9)At the point 𝑋 = 0 , one has for all 𝛼 > 1 𝑢 𝛼 ( 0 ) = 4 Γ ( 2 + 𝛼 ) 𝜋 2 + 𝛼 2 𝛼 + 2 𝑣 1 𝜁 ( 2 + 𝛼 ) > 0 , ( 3 . 1 7 ) 𝛼 ( 0 ) = 0 , ( 3 . 1 8 ) where 𝜁 ( 𝑠 ) is the Riemann Zeta function (see [15]).

3.2. Sturm-Liouville Problem

It is convenient to represent 𝑤 𝛼 ( 𝑋 ) in the exponential form, namely, 𝑤 𝛼 ( 𝑋 ) = 𝑅 𝛼 ( 𝑋 ) e x p 𝑖 Θ 𝛼 ( 𝑋 ) , ( 3 . 1 9 ) where 𝑅 𝛼 ( 𝑋 ) = 𝑢 𝛼 ( 𝑋 ) 2 + 𝑣 𝛼 ( 𝑋 ) 2 , Θ 𝛼 Φ ( 𝑋 ) = 𝛼 ( 𝑋 ) , 𝑢 𝛼 Φ ( 𝑋 ) > 0 , 𝛼 ( 𝑋 ) + 𝜋 , 𝑢 𝛼 ( 𝑋 ) < 0 , 𝑣 𝛼 Φ ( 𝑋 ) 0 , 𝛼 ( 𝑋 ) 𝜋 , 𝑢 𝛼 ( 𝑋 ) < 0 , 𝑣 𝛼 Φ ( 𝑋 ) < 0 , 𝛼 ( 𝑣 𝑋 ) = a r c t a n 𝛼 ( 𝑋 ) 𝑢 𝛼 . ( 𝑋 ) ( 3 . 2 0 ) Exponential representation (3.19) allows one to deduce the boundary value problem for the functions 𝑤 𝛼 ( 𝑋 ) . It turns out that for all 𝛼 > 1 the functions 𝑤 𝛼 ( 𝑋 ) solve the equation 𝑑 𝑃 𝑑 𝑋 𝛼 ( 𝑋 ) 𝑑 𝑤 𝑑 𝑋 𝑄 𝛼 ( 𝑋 ) 𝑤 + 𝜌 𝛼 ( 𝑋 ) 𝑤 = 0 , 𝑋 , ( 3 . 2 1 ) where 𝑃 𝛼 ( 𝐶 𝑋 ) = 𝑊 𝑢 𝛼 ( 𝑋 ) , 𝑣 𝛼 𝑄 ( 𝑋 ) , 𝐶 = c o n s t , 𝛼 𝑃 ( 𝑋 ) = 𝛼 ( 𝑋 ) 𝑅 𝛼 ( 𝑋 ) 𝑅 𝛼 , 𝜌 ( 𝑋 ) 𝛼 = Θ ( 𝑋 ) 𝛼 ( 𝑋 ) 2 , Θ ( 3 . 2 2 ) 𝛼 𝑊 𝑢 ( 𝑋 ) = 𝛼 ( 𝑋 ) , 𝑣 𝛼 ( 𝑋 ) 𝑅 2 𝛼 ( . 𝑋 ) ( 3 . 2 3 ) Here 𝑊 [ 𝑢 𝛼 ( 𝑋 ) , 𝑣 𝛼 ( 𝑋 ) ] is the Wronskian of 𝑢 𝛼 ( 𝑋 ) and 𝑣 𝛼 ( 𝑋 ) . Below we shall use a shorter notation 𝑊 𝛼 ( 𝑋 ) = 𝑊 [ 𝑢 𝛼 ( 𝑋 ) , 𝑣 𝛼 ( 𝑋 ) ] .

Taking into account the behavior of 𝑤 𝛼 ( 𝑋 ) for large 𝑋 (see [15]), we can restate the obtained results in another form. Indeed, 𝑤 𝛼 ( 𝑋 ) are solutions of the Sturm-Liouville problem 𝑑 𝑃 𝑑 𝑋 𝛼 ( 𝑋 ) 𝑑 𝑤 𝑑 𝑋 + 𝑄 𝛼 ( 𝑋 ) 𝑤 = 𝜆 𝜌 𝛼 ( 𝑋 ) 𝑤 , 𝑋 , ( 3 . 2 4 ) l i m 𝑋 ± 𝑤 ( 𝑋 ) = 0 , ( 3 . 2 5 ) corresponding to 𝜆 = 1 . Without loss of generality, we can choose the constant in (3.22) to be positive. In the next subsection, we shall prove that 𝑊 𝛼 ( 𝑋 ) > 0 . It implies that 𝑃 𝛼 ( 𝑋 ) > 0 and 𝜌 𝛼 ( 𝑋 ) > 0 in (3.22).

It follows from (3.7) that for 𝛼 > 0 the functions 𝑤 𝛼 ( 𝑋 ) also satisfy the zero mean condition 𝑤 𝛼 ( 𝑋 ) 𝑑 𝑋 = 0 . ( 3 . 2 6 ) This reflects the oscillatory behavior of 𝑤 𝛼 ( 𝑋 ) for 𝛼 > 0 (see Figures 3 and 4).

The graph of the arctangent function Φ 𝛼 ( 𝑋 ) is shown in Figure 5. Φ 𝛼 ( 𝑋 ) conveniently serves as a zero counter for both functions: 𝑢 𝛼 ( 𝑋 ) and 𝑣 𝛼 ( 𝑋 ) . It possesses zeros at the points where 𝑣 𝛼 ( 𝑋 ) has zeros and has jumps at the points where 𝑢 𝛼 ( 𝑋 ) has zeros.

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Figure 5: Graph of the arctangent function Φ 3 . 8 ( 𝑋 ) .

Remark 3.3. Observe that a general solution of (3.24) can be written in the form 𝑤 ( 𝑔 ) ( 𝑋 ) = 𝐶 1 𝑢 𝛼 ( 𝑋 ) + 𝐶 2 𝑢 𝛼 ( 𝑋 ) 𝑋 0 𝑊 𝛼 ( 𝑦 ) 𝑢 2 𝛼 ( 𝑦 ) 𝑑 𝑦 , ( 3 . 2 7 ) where 𝐶 1 , 𝐶 2 = c o n s t .

Remark 3.4. We would like to point out that the differential equation given by (3.21) can be factored in the following way (see [26, page 269]): 𝑑 𝑃 𝑑 𝑋 𝛼 ( 𝑋 ) 𝑑 𝑤 𝑑 𝑋 𝑄 𝛼 ( 𝑋 ) 𝑤 + 𝜌 𝛼 𝑊 ( 𝑋 ) 𝑤 = 𝛼 ( 𝑋 ) 𝑢 𝛼 𝑑 ( 𝑋 ) 𝑢 𝑑 𝑋 2 𝛼 ( 𝑋 ) 𝑊 𝛼 𝑑 ( 𝑋 ) 𝑑 𝑋 𝑤 ( 𝑋 ) 𝑢 𝛼 . ( 𝑋 ) ( 3 . 2 8 )

3.3. Wronskian of 𝑢 𝛼 and 𝑣 𝛼

Lemma 3.5. The following properties hold for the Wronskian 𝑊 𝛼 ( 𝑋 ) for 𝛼 > 1 and all 𝑥 : 𝑊 𝛼 ( 𝑋 ) = 𝑊 𝛼 ( 𝑋 ) , 𝑊 𝛼 𝑊 ( 0 ) = 0 , ( 3 . 2 9 ) 𝛼 ( 𝑋 ) > 0 . ( 3 . 3 0 )

Proof. We start with (3.29). Taking into account relations in (3.3) and the fact that 𝜕 𝑋 = 𝐻 𝐷 , we can write 𝑊 𝛼 ( 𝑋 ) = 𝑢 𝛼 ( 𝑋 ) 𝑣 𝛼 ( 𝑋 ) 𝑣 𝛼 ( 𝑋 ) 𝑢 𝛼 ( 𝑋 ) = 𝑢 𝛼 ( 𝑋 ) 𝑢 𝛼 + 1 ( 𝑋 ) + 𝑣 𝛼 ( 𝑋 ) 𝑣 𝛼 + 1 ( 𝑋 ) . ( 3 . 3 1 ) Since the functions 𝑢 𝛼 ( 𝑋 ) are even and 𝑣 𝛼 ( 𝑋 ) are odd with respect to 𝑋 , 𝑊 𝛼 ( 𝑋 ) is even for 𝑋 . Differentiation of (3.31) with the help of (3.6) and (3.18) yields 𝑊 𝛼 ( 0 ) = 0 . Next, we turn to the proof of (3.30). Since the functions 𝑢 𝛼 ( 𝑋 ) and 𝑣 𝛼 ( 𝑋 ) are linearly independent solutions of the equation (3.24), 𝑊 𝛼 ( 𝑋 ) 0 for all 𝛼 > 1 and 𝑥 . It remains to establish the sign of the Wronskian. In view of (3.17) and (3.18), 𝑊 𝛼 ( 0 ) = 𝑢 𝛼 ( 0 ) 𝑢 𝛼 + 1 ( 0 ) = 1 6 Γ ( 2 + 𝛼 ) Γ ( 3 + 𝛼 ) 𝜋 5 + 2 𝛼 2 2 + 𝛼 2 1 3 + 𝛼 1 𝜁 ( 2 + 𝛼 ) 𝜁 ( 3 + 𝛼 ) > 0 . ( 3 . 3 2 ) By Abel's formula, for all 𝑋 , 𝑊 𝛼 ( 𝑋 ) = 𝑊 𝛼 ( 0 ) e x p 𝑋 0 𝑃 𝛼 ( 𝜂 ) 𝑃 𝛼 , ( 𝜂 ) 𝑑 𝜂 ( 3 . 3 3 ) where the function 𝑃 𝛼 ( 𝑋 ) 𝑃 𝛼 ( 𝑋 ) = 𝑖 ( 𝑠 + 1 ) 𝜋 𝜁 ( 𝑠 , 𝑧 ) 𝜁 + ( 𝑠 + 2 , 𝑧 ) 𝜁 + ( 𝑠 , 𝑧 ) 𝜁 ( 𝑠 + 2 , 𝑧 ) 𝜁 + ( 𝑠 , 𝑧 ) 𝜁 + ( 𝑠 + 1 , 𝑧 ) 𝜁 ( 𝑠 , 𝑧 ) 𝜁 , ( 𝑠 + 1 , 𝑧 ) 𝑠 = 2 + 𝛼 , 𝑧 = 1 / 2 + 𝑖 𝑋 / 𝜋 , ( 3 . 3 4 ) is continuous on . After some simplification, we have that 𝑊 𝛼 ( 𝑋 ) = 𝑊 𝛼 ( 0 ) e x p 𝑠 + 1 𝜋 [ ] [ ] [ ] [ ] 𝜁 ( 𝑠 , 𝑧 ) 𝜁 ( 𝑠 + 2 , 𝑧 ) 𝜁 ( 𝑠 , 𝑧 ) 𝜁 ( 𝑠 + 2 , 𝑧 ) [ ] [ ] [ ] [ ] 𝜁 ( 𝑠 , 𝑧 ) 𝜁 ( 𝑠 + 1 , 𝑧 ) + 𝜁 ( 𝑠 , 𝑧 ) 𝜁 ( 𝑠 + 1 , 𝑧 ) . ( 3 . 3 5 ) This representation yields (3.30). The lemma is proved.

Three-dimensional graph of 𝑊 𝛼 ( 𝑋 ) is given in Figure 6.

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Figure 6: Three-dimensional graph of the Wronskian 𝑊 𝛼 ( 𝑋 ) .

Remark 3.6. What does the positivity of the Wronskian yield for the soliton and its conjugate? For 𝛼 = 0 , (3.30) simplifies to read 𝑊 0 ( 𝑋 ) = 2 s e c h 2 𝑣 ( 𝑋 ) 0 ( 𝑋 ) + t a n h 𝑋 𝑣 0 ( 𝑋 ) > 0 . ( 3 . 3 6 ) We notice that 𝑣 0 ( 𝑋 ) > 0 for 𝑋 > 0 , 𝑣 0 ( 𝑋 ) = 𝑣 0 ( 𝑋 ) for 𝑋 , and 𝑣 0 ( 0 ) = 0 (see Figure 2). Integrating the inequality 𝑣 0 ( 𝑋 ) / 𝑣 0 ( 𝑋 ) + t a n h 𝑋 > 0 over the interval [ 𝜀 , 𝑋 ] for 𝑋 𝜀 > 0 and the inequality 𝑣 0 ( 𝑋 ) / 𝑣 0 ( 𝑋 ) + t a n h 𝑋 < 0 over [ 𝜀 , 𝑋 ] for 𝑋 𝜀 < 0 yields the estimate | | 𝑣 0 | | > | | 𝑣 ( 𝑋 ) 0 | | ( 𝜀 ) c o s h 𝜀 | | 𝑋 | | c o s h 𝑋 f o r 𝜀 > 0 . ( 3 . 3 7 )

3.4. Zeros of the Functions 𝑢 𝛼 ( 𝑋 ) and 𝑣 𝛼 ( 𝑋 )

This subsection is devoted to the estimates of the number of zeros for the functions in question. By a strictly monotone change of variable 𝑦 = 𝑋 𝑏 𝑑 𝜂 𝑃 𝛼 ( 𝜂 ) , 𝑏 = c o n s t , ( 3 . 3 8 ) Equation (3.21) can be reduced to the equation 𝑑 2 𝒲 𝑑 𝑦 2 + 𝑄 𝛼 ( 𝑦 ) 𝒲 = 0 , ( 3 . 3 9 ) where 𝒲 ( 𝑦 ) = 𝑤 ( 𝑋 ( 𝑦 ) ) and 𝑄 𝛼 ( 𝑦 ) = 𝑃 𝛼 ( 𝑋 ( 𝑦 ) ) 𝑄 𝛼 ( 𝑋 ( 𝑦 ) ) . Therefore, any nontrivial solution of (3.39) can have not more than a finite number of zeros on any bounded interval ([24], page 323).

Theorem 3.7. Let 𝑁 𝛼 be the number of zeros of the function 𝑣 𝛼 ( 𝑋 ) on the interval [ 0 , 𝑋 0 ] , where 𝑋 0 < . Then the following inequality holds: 𝐼 𝛼 1 𝑁 𝛼 𝐼 𝛼 + 1 , ( 3 . 4 0 ) where 𝐼 𝛼 = a r c t a n 𝑖 𝜁 2 + 𝛼 , 1 / 2 + 𝑖 𝑋 0 / 𝜋 𝜁 + 2 + 𝛼 , 1 / 2 + 𝑖 𝑋 0 / 𝜋 . ( 3 . 4 1 )

Proof. Since we chose 𝐶 = 1 in (3.22), 𝑃 𝛼 𝑢 ( 𝑋 ) 𝑊 𝛼 ( 𝑋 ) , 𝑣 𝛼 ( 𝑋 ) = 1 . ( 3 . 4 2 ) Therefore, Θ 𝛼 𝑣 ( 𝑋 ) = 𝛼 𝑢 𝛼 𝑢 𝛼 𝑣 𝛼 𝑣 2 𝛼 > 0 . ( 3 . 4 3 ) Therefore, by Theorem 2.1 of Section 2, for the interval [ 0 , 𝑋 0 ] we have the estimate 1 + 𝐼 𝛼 𝑁 𝛼 1 + 𝐼 𝛼 , ( 3 . 4 4 ) where 𝐼 𝛼 = 𝑋 0 0 𝑊 𝛼 ( 𝜂 ) 𝑑 𝜂 𝑣 2 𝛼 ( 𝜂 ) + 𝑢 2 𝛼 = ( 𝜂 ) 𝑋 0 0 Θ 𝛼 ( 𝜂 ) 𝑑 𝜂 = a r c t a n 𝑖 𝜁 2 + 𝛼 , 1 / 2 + 𝑖 𝑋 0 / 𝜋 𝜁 + 2 + 𝛼 , 1 / 2 + 𝑖 𝑋 0 / 𝜋 . ( 3 . 4 5 ) Here we have used the fact that 𝜁 ( 𝑠 , 1 / 2 ) = 0 for 𝑠 > 1 .

Theorem 3.8. The zeros of 𝑢 𝛼 ( 𝑋 ) separate and are separated by those of 𝑣 𝛼 ( 𝑋 ) .

Proof. This follows from Sturm's Separation Theorem (see [24], page 335).

4. Inequality for Hurwitz Zeta Functions

Here we discuss a new inequality for the Hurwitz Zeta functions which follows from Lemma 3.5. The next statement is a corollary of this lemma.

Corollary 4.1. For 𝑠 > 1 and 𝑧 = 1 / 2 + 𝑖 𝑋 / 𝜋 with 𝑋 , the following inequality holds: 𝒦 ( 𝑠 , 𝑧 ) = 𝜁 𝑠 , 𝑧 𝜁 ( 𝑠 + 1 , 𝑧 ) + 𝜁 ( 𝑠 , 𝑧 ) 𝜁 𝑠 + 1 , 𝑧 > 0 . ( 4 . 1 ) This inequality can also be written in another form: 𝒦 ( 𝑠 , 𝑧 ) = { 𝜁 ( 𝑠 , 𝑧 ) } { 𝜁 ( 𝑠 + 1 , 𝑧 ) } + { 𝜁 ( 𝑠 , 𝑧 ) } { 𝜁 ( 𝑠 + 1 , 𝑧 ) } > 0 . ( 4 . 2 )

Proof. Dropping positive terms in front of the full-range Hurwitz Zeta functions in (3.4) and (3.5) and using (3.30) lead to 𝜁 + 𝑠 , 𝑧 𝜁 + ( 𝑠 + 1 , 𝑧 ) 𝜁 ( 𝑠 , 𝑧 ) 𝜁 𝑠 + 1 , 𝑧 𝜁 = 2 𝑠 , 𝑧 𝜁 ( 𝑠 + 1 , 𝑧 ) + 𝜁 ( 𝑠 , 𝑧 ) 𝜁 𝑠 + 1 , 𝑧 [ ] = 4 { 𝜁 ( 𝑠 , 𝑧 ) } { 𝜁 ( 𝑠 + 1 , 𝑧 ) } + { 𝜁 ( 𝑠 , 𝑧 ) } { 𝜁 ( 𝑠 + 1 , 𝑧 ) } > 0 . ( 4 . 3 )

Remark 4.2. Setting 𝜁 ( 𝑠 , 𝑧 ) = 𝑟 𝑠 ( 𝑧 ) 𝑒 𝑖 𝜑 𝑠 ( 𝑧 ) and 𝜁 ( 𝑠 + 1 , 𝑧 ) = 𝑟 𝑠 + 1 𝑒 𝑖 𝜑 𝑠 + 1 ( 𝑧 ) , we can rewrite (4.1) in the form 𝒦 = 2 𝑟 𝑠 𝑟 𝑠 + 1 𝑖 𝜑 e x p 𝑠 + 1 𝜑 𝑠 𝜑 + e x p 𝑖 𝑠 + 1 𝜑 𝑠 = 4 𝑟 𝑠 𝑟 𝑠 + 1 𝜑 c o s 𝑠 + 1 𝜑 𝑠 . ( 4 . 4 ) It shows that, for 𝑧 = 1 / 2 + 𝑖 𝑋 / 𝜋 , 𝑋 , 𝜑 c o s 𝑠 + 1 ( 𝑧 ) 𝜑 𝑠 ( 𝑧 ) > 0 . ( 4 . 5 ) Introduce the scalar product for the complex-valued functions 𝑓 = 𝑓 1 + 𝑖 𝑓 2 and 𝑔 = 𝑔 1 + 𝑖 𝑔 2 by the formula 𝑓 𝑔 = 𝑓 𝑔 = 𝑓 1 𝑓 2 + 𝑓 2 𝑔 2 𝑓 + 𝑖 2 𝑔 1 𝑓 1 𝑔 2 . ( 4 . 6 ) Then for 𝑠 > 1 and 𝑧 = 1 / 2 + 𝑖 𝑋 / 𝜋 , 𝒦 ( 𝑠 , 𝑧 ) = 2 { 𝜁 ( 𝑠 , 𝑧 ) 𝜁 ( 𝑠 + 1 , 𝑧 ) } > 0 . ( 4 . 7 )

Remark 4.3. The proof of (4.1) becomes quite difficult when one approaches it from the point of view of special functions. For example, the use of integral representations (2.21) and (2.22) yields 1 𝒦 = 2 Γ ( 𝑠 ) Γ ( 𝑠 + 1 ) 0 𝑡 𝑠 1 𝜏 𝑠 [ ] c o s 𝑋 / 𝜋 ( 𝑡 𝜏 ) s i n h ( 𝑡 / 2 ) s i n h ( 𝜏 / 2 ) 𝑑 𝑡 𝑑 𝜏 . ( 4 . 8 ) The change of variables 𝜉 = ( 𝑡 𝜏 ) / 2 , 𝜂 = ( 𝑡 + 𝜏 ) / 2 leads to 2 𝒦 = Γ ( 𝑠 ) Γ ( 𝑠 + 1 ) 0 2 𝑋 c o s 𝜋 𝜉 𝑑 𝜉 𝜉 𝜉 ( 𝜉 + 𝜂 ) 𝑠 1 ( 𝜂 𝜉 ) 𝑠 c o s h 𝜂 c o s h 𝜉 𝑑 𝜂 . ( 4 . 9 ) It is not clear at all that the integral (4.9) is positive for all 𝑠 > 1 and 𝑋 . However, (4.1) shows that it is. Multiplication of the series representations (2.16) and (2.17) does not make the proof any easier.

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