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Fractional Quasi-Bessel Equations

Pavel B. Dubovski 1, Jeffrey A. Slepoi 1
Abstract

In this paper we consider fractional quasi-Bessel equations

i=1mdixαi+piDαiu(x)+(xβν2)u(x)=0\sum_{i=1}^{m}d_{i}x^{\alpha_{i}+p_{i}}D^{\alpha_{i}}u(x)+(x^{\beta}-\nu^{2})u(x)=0

and construct their existence and uniqueness theory in the class of fractional series. Our methodology allows us to obtain new results for a broad class of fractional differential equations including Cauchy-Euler and constant-coefficient equations.

MSC 2010: 26A33, 34A25

Key Words and Phrases: quasi-Bessel equations; fractional calculus; fractional power series; existence; uniqueness; Cauchy-Euler equations; constant-coefficient equations

1 Introduction

We generalize the classical Bessel equation (1.1)

x2u′′+xu+(x2ν2)u=0x^{2}u^{\prime\prime}+xu^{\prime}+(x^{2}-\nu^{2})u=0 (1.1)

to a broad class of equations including multi-term fractional Bessel, Cauchy-Euler equations, and fractional differential equations with constant coefficients. We consider the Caputo

DCαu(t)=1Γ(nα)0tu(n)(x)dx(tx)α+1n,n1α<n,nD_{C}^{\alpha}u(t)=\frac{1}{\Gamma(n-\alpha)}\int_{0}^{t}\frac{u^{(n)}(x)dx}{(t-x)^{\alpha+1-n}},n-1\leq\alpha<n,n\in\mathbb{N} (1.2)

and Riemann-Liouville

DRαu(t)=1Γ(nα)dndtn0tu(x)dx(tx)α+1n,n1α<n,nD_{R}^{\alpha}u(t)=\frac{1}{\Gamma(n-\alpha)}\frac{d^{n}}{dt^{n}}\int_{0}^{t}\frac{u(x)dx}{(t-x)^{\alpha+1-n}},n-1\leq\alpha<n,n\in\mathbb{N} (1.3)

fractional derivatives.

Equation (1.1) is a source for many generalizations and extensions. Numerous results for hyper-Bessel equations and corresponding operators, introduced by Dimovski, are obtained in [1, 4, 10, 12]. Paper [3] introduces another definition for the fractional order Bessel operator, which allows to construct an operational calculus applicable to Bessel equation with fractional derivatives. W. Okrasiński and L. Plociniczak [14] consider a fractional modification of the Bessel equation, and solve it in terms of the power series.

A natural extension of the classical Bessel equation (1.1) in terms of Caputo fractional derivatives

x2αD2αu(x)+xαDαu(x)+(x2αν2)u(x)=0,α(0,1]x^{2\alpha}D^{2\alpha}u(x)+x^{\alpha}D^{\alpha}u(x)+(x^{2\alpha}-\nu^{2})u(x)=0,\alpha\in(0,1] (1.4)

was analyzed by Rodrigues, Viera and Yakubovich [16], where a solution in a form of series for equation (1.4) was identified for a some specific values of ν\nu depending on α\alpha.

The multi-term fractional Bessel equation

i=1m1dixαiDCαiu(x)+(xβν2)u(x)=0,αi>0,β>0\sum_{i=1}^{m_{1}}d_{i}x^{\alpha_{i}}D_{C}^{\alpha_{i}}u(x)+(x^{\beta}-\nu^{2})u(x)=0,\alpha_{i}>0,\beta>0 (1.5)

with existence and uniqueness criteria was presented by the authors in [5] where we constructed solutions in the form of series

u(x)=n=0cnxγ+βn.u(x)=\sum_{n=0}^{\infty}c_{n}x^{\gamma+\beta n}. (1.6)

with coefficients cnc_{n} as

cn=(1)nk=1n(i=1m1diΓ(1+γ+βk)Γ(1+γ+βkαi)ν2).\displaystyle c_{n}=\frac{(-1)^{n}}{\displaystyle\prod_{k=1}^{n}\left(\displaystyle\sum_{i=1}^{m_{1}}\frac{d_{i}\Gamma(1+\gamma+\beta k)}{\Gamma(1+\gamma+\beta k-\alpha_{i})}-\nu^{2}\right)}. (1.7)

The characteristic equation for equation (1.5)

i=1m1diΓ(1+γ)Γ(1+γαi)ν2=0\sum_{i=1}^{m_{1}}\frac{d_{i}\Gamma(1+\gamma)}{\Gamma(1+\gamma-\alpha_{i})}-\nu^{2}=0 (1.8)

must be solvable and all derivatives DαixγD^{\alpha_{i}}x^{\gamma} should exist. Theorem 1 below states that series solution (1.6),(1.7) always exists in real numbers as long as all di>0d_{i}>0 and ν\nu satisfies a certain threshold condition. Our results for equation (1.5) are obtained for a broad class of parameters αi\alpha_{i} and ν\nu. They include some results of ([10], sec. 3.4) and [16]. For example, if we deal with derivatives of integer orders αi\alpha_{i} and ν=0\nu=0 in equation (1.5), then we arrive at the eigenvalue problem, which is solved in [10] and where the fundamental system of solutions (in terms of the hyper-Bessel functions of Delerue) has been determined. Besides fractional Bessel equations (1.5), the quasi-Bessel equations generalize Cauchy-Euler equidimensional equations as well and, thus, we extend further a number of results from the works of Kilbas and Zhukovskaya [9, 18, 19]. After a minor modification, our approach becomes also applicable to the equations with constant coefficients. In works [13], using the methods of [7], the initial value problem is solved for constant-coefficient fractional equations. In [2], the Cauchy problems for some linear constant-coefficient equations with real, including irrational, derivatives, are analyzed and solved. The presented method and its particular version for constant-coefficient equations also allow to treat a class of irrational derivatives. Additional extensive information regarding fractional differential equations can be found in many works on fractional calculus, e.g., in monographs [8, 10, 15, 17].

In this paper we analyze the next generalization of multi-term Bessel equations – the quasi-Bessel fractional equations

i=1mdixαi+piDαiu(x)+(xβν2)u(x)=0,x>0,\sum_{i=1}^{m}d_{i}x^{\alpha_{i}+p_{i}}D^{\alpha_{i}}u(x)+(x^{\beta}-\nu^{2})u(x)=0,\ \ x>0, (1.9)

where αi+\alpha_{i}\in\mathbb{R^{+}} with α1=max1im{αi}\alpha_{1}=\max\limits_{1\leq i\leq m}\{\alpha_{i}\} and p1=0p_{1}=0. Shifting indices pip_{i} (deviations with respect to (1.5)) should be non-negative and satisfy special almost-rational conditions defined in Section 2. If all additional indices pip_{i} are zero, then we arrive at the previously investigated in [5] multi-term fractional Bessel equation (1.5), where the powers of multipliers xx must match the order of derivatives. However, in this research the powers of xx have to match the order of only one derivative – the derivative of the highest order. As we show below, many other equations, including equations with constant coefficients, represent special cases of quasi-Bessel equations and, as just a corollary, we can derive the key points of the theory for fractional constant-coefficient equations.

The structure of this paper is as follows.
In Section 2 we present the fractional series solution for equation (1.9) and derive the steps to obtain it numerically.

In Section 3 we cite the existence theorem from [5], and prove our main existence result (Theorem 2), including the necessary condition claiming that the power of xx must match the highest fractional derivative.

Motivated by [16], Section 4 presents the uniqueness theorem for the initial value problem of equation (1.9).

Section 5 covers the use of the presented methodology to identify a series solution for homogeneous fractional equations with constant coefficients and its further extension into equations with power function factors. As a particular case of the constructed theory we have another derivation of the existence results for fractional differential equations with constant coefficients with multiple derivatives of any order.

Section 6 provides a few numerical examples which support the constructed theory. Numerical method which utilizes substitution [6] is used to cross check the identified series solution in Example 1 and extend it further. Examples 2-4 confirm that our methodology works on previously analytically solved problems with one fractional derivative presented in monograph by Kilbas, Srivastava, and Trujillo [8].

Throughout this paper notation Dαu(x)D^{\alpha}u(x) is used for both, Riemann-Liouville and Caputo, types of fractional derivatives, whereas DCαu(x)D_{C}^{\alpha}u(x) refers to the Caputo derivative, and DRαu(x)D_{R}^{\alpha}u(x) is the Riemann-Liouville derivative.

2 Construction of the fractional series solution

We go beyond equation (1.5) and consider equation (1.9) in the following form:

d1xα1Dα1u(x)+i=2mdixαi+piDαiu(x)+(xβν2)u(x)=0.d_{1}x^{\alpha_{1}}D^{\alpha_{1}}u(x)+\sum_{i=2}^{m}d_{i}x^{\alpha_{i}+p_{i}}D^{\alpha_{i}}u(x)+(x^{\beta}-\nu^{2})u(x)=0. (2.1)

It is worth mentioning its particular cases:

a)\displaystyle a) d1xα1Dα1u(x)+i=2mdixαi+piDαiu(x)+xβu(x)=0,ν=0,\displaystyle d_{1}x^{\alpha_{1}}D^{\alpha_{1}}u(x)+\sum_{i=2}^{m}d_{i}x^{\alpha_{i}+p_{i}}D^{\alpha_{i}}u(x)+x^{\beta}u(x)=0,\ \nu=0,
b)\displaystyle b) d1xα1Dα1u(x)+i=2mdixαi+piDαiu(x)+u(x)=0,β=ν=0.\displaystyle d_{1}x^{\alpha_{1}}D^{\alpha_{1}}u(x)+\sum_{i=2}^{m}d_{i}x^{\alpha_{i}+p_{i}}D^{\alpha_{i}}u(x)+u(x)=0,\ \beta=\nu=0.
Definition 1.

Differential equation (2.1) is called a quasi-Bessel equation provided that α1=max{αi}\alpha_{1}=\max\{\alpha_{i}\} and for all i, 1imi,\,1\leq i\leq m, did_{i}\in\mathbb{R}, αi+=[0,)\alpha_{i}\in\mathbb{R}^{+}=[0,\infty), β+=+\beta\in\mathbb{Q^{+}}=\mathbb{R}^{+}\cap\mathbb{Q}. Shifting indices pip_{i}, 2im2\leq i\leq m, should be non-negative and almost-rational, i.e., for a fixed number r+r\in\mathbb{R^{+}} the deviations pip_{i} must belong to the set

pir+=r+={x:x=rq,q+}.p_{i}\in\mathbb{Q}^{+}_{r}=r\cdot\mathbb{Q^{+}}=\{x:\ x=rq,\ q\in\mathbb{Q^{+}}\}.

This section is applicable to equations with both Caputo and Riemann-Liouville derivatives. The only difference is the condition on acceptable γ\gamma in (1.8) to generate a true solution. For Riemann-Liouville it is γ>1\gamma>-1 and for Caputo – γ>α11\gamma>\lceil\alpha_{1}\rceil-1 to assure existence of derivatives.

Notation. Let nmaxn_{\max} be the integer ceiling for the highest non-integer derivative, i.e., nmax=max{ni}n_{\max}=\max{\{n_{i}\}} and nminn_{\min} be the integer ceiling for the lowest non-integer derivative, i.e., nmin=min{ni}n_{\min}=\min{\{n_{i}\}} where
ni1<αi<ni,ni,i=1,,mn_{i}-1<\alpha_{i}<n_{i},n_{i}\in\mathbb{N},i=1,...,m.

Lemma 1.

(see [5]) For the existence of the series solution for equation (2.1) with Caputo derivatives, it is necessary that solutions of the characteristic equation (1.8), γ>nmax10\gamma>n_{\max}-1\geq 0. ∎

In the multi-term fractional Bessel equation (1.5) it was possible to use s=βs=\beta as a step (increase) in the series solution because it allowed recursively express all cnc_{n} (1.7). In the more general case of equation (2.1), it is not possible since some coefficients cnc_{n} do not get ’balanced out’ and need to be forced to be zero, which leads to a trivial solution. Therefore, we need to find the largest possible step sβs\leq\beta which allows us to balance out (express recursively) all coefficients. Thus, we proceed as follows.

Let us assume that the solution for equation (2.1) is

u(x)=n=0cnxγ+sn,u(x)=\sum_{n=0}^{\infty}c_{n}x^{\gamma+sn}, (2.2)

where γ\gamma satisfies the equation

G(γ)=i=1m1diΓ(1+γ)Γ(1+γαi)ν2=i=1m1diQ(0,αi)ν2=0,G(\gamma)=\sum_{i=1}^{m_{1}}\frac{d_{i}\Gamma(1+\gamma)}{\Gamma(1+\gamma-\alpha_{i})}-\nu^{2}=\sum_{i=1}^{m_{1}}d_{i}Q(0,\alpha_{i})-\nu^{2}=0, (2.3)

where pi=0,i=2,,m1p_{i}=0,i=2,...,m_{1} and

Q(r,p)=Γ(1+γ+r)Γ(1+γ+rp).Q(r,p)=\frac{\Gamma(1+\gamma+r)}{\Gamma(1+\gamma+r-p)}. (2.4)

It is clear that all roots of equation (2.3) belong to a bounded interval.
In addition to p1=0p_{1}=0, several other terms could also have pi=0p_{i}=0. Let us call them the pure Bessel terms. For these terms the power of the factor xαx^{\alpha} matches the order of the derivative Dαu(x)D^{\alpha}u(x). Let m1m_{1} be the number of pure Bessel terms in (2.1). Then, all other terms have strictly positive shifted powers pi>0p_{i}>0 for i=m1+1,,mi=m_{1}+1,...,m.

By plugging expression (2.2) into equation (2.1), we obtain

n=0\displaystyle\sum_{n=0}^{\infty}\!\!\!\! cn\displaystyle c_{n} (i=1m1dixγ+snQ(ns,αi)+i=m1+1mdixγ+sn+piQ(ns+pi,αi))\displaystyle\!\!\!\!\left(\sum_{i=1}^{m_{1}}d_{i}x^{\gamma+sn}Q(ns,\alpha_{i})+\sum_{i=m_{1}+1}^{m}d_{i}x^{\gamma+sn+p_{i}}Q(ns+p_{i},\alpha_{i})\right)
+\displaystyle+ (xβν2)n=0cnxγ+sn=0,\displaystyle\!\!\!(x^{\beta}-\nu^{2})\sum_{n=0}^{\infty}c_{n}x^{\gamma+sn}=0,

or

n=0cnxγ+sn\displaystyle\sum_{n=0}^{\infty}c_{n}x^{\gamma+sn}\!\! (\displaystyle\Bigg{(}\!\! i=1m1diQ(ns,αi)ν2\displaystyle\displaystyle\sum_{i=1}^{m_{1}}d_{i}Q(ns,\alpha_{i})-\nu^{2} (2.5)
+\displaystyle+ i=m1+1mxpidiQ(ns+pi,αi)+xβ)=0.\displaystyle\!\!\displaystyle\sum_{i=m_{1}+1}^{m}x^{p_{i}}d_{i}Q(ns+p_{i},\alpha_{i})+x^{\beta}\Bigg{)}=0.

If the step ss is such that pis=npi\displaystyle\frac{p_{i}}{s}=n_{p_{i}}\in\mathbb{N} and βs=nβ\displaystyle\frac{\beta}{s}=n_{\beta}\in\mathbb{N} then we obtain

n=0cnxγ+sn(\displaystyle\sum_{n=0}^{\infty}c_{n}x^{\gamma+sn}\Bigg{(} i=1m1\displaystyle\displaystyle\sum_{i=1}^{m_{1}} diQ(ns,αi)ν2\displaystyle d_{i}Q(ns,\alpha_{i})-\nu^{2}
+\displaystyle+ i=m1+1m\displaystyle\displaystyle\sum_{i=m_{1}+1}^{m} xsnpidiQ(ns+pi,αi)+xsnβ)=0.\displaystyle x^{sn_{p_{i}}}d_{i}Q(ns+p_{i},\alpha_{i})+x^{sn_{\beta}}\Bigg{)}=0. (2.6)

Step ss should be such that any powers of xx in quasi-Bessel equation (2.1) are included in the set γ+sn\gamma+sn. We want to find the maximum possible step ss to minimize the number of steps and avoid having unnecessary zero coefficients cnc_{n}. Let us describe how step ss can be identified.

  • From the definition of quasi-Bessel equation (2.1) we have βr+\beta\in\mathbb{Q}_{r}^{+}, pir+p_{i}\in\mathbb{Q}_{r}^{+}. Therefore we first convert them into rational numbers:
    β0=βr=a1b1\displaystyle\beta^{0}=\frac{\beta}{r}=\frac{a_{1}}{b_{1}}; pi0=01=aibi,2im1;pi0=pir=aibi\ \ \displaystyle p_{i}^{0}=\frac{0}{1}=\frac{a_{i}}{b_{i}},2\leq i\leq m_{1};\ \ p_{i}^{0}=\frac{p_{i}}{r}=\frac{a_{i}}{b_{i}}, m1<imm_{1}<i\leq m. If r+r\in\mathbb{Q^{+}}, then r=1r=1.

  • Find the lowest common denominator NLCD=LCD{bi}N_{LCD}=\text{LCD}\{b_{i}\},
    m1<imm_{1}<i\leq m.

  • Calculate the acceptable step and corresponding shifts for β\beta and pip_{i}:

    s0=1NLCD;nβ0=β0s0;npi0=pi0s0,m1<im.s^{0}=\frac{1}{N_{LCD}};\ n_{\beta}^{0}=\frac{\beta^{0}}{s^{0}}\in\mathbb{N};\ n_{p_{i}}^{0}=\frac{p_{i}^{0}}{s^{0}}\in\mathbb{N},\ m_{1}<i\leq m. (2.7)
  • The identified parameters β0,pi0\beta^{0},p_{i}^{0}, m1<imm_{1}<i\leq m in (2.7) can still have common factors. To maximize step ss we need to identify their greatest common factor (NgcfN_{gcf}), adjust step ss and each parameter. Then, finally, we obtain:

    s=s0Ngcf;nβ=nβ0Ngcf;npi=npi0Ngcf,m1<im.s=s^{0}\cdot N_{gcf};\ n_{\beta}=\frac{n_{\beta}^{0}}{N_{gcf}};\ n_{p_{i}}=\frac{n_{p_{i}}^{0}}{N_{gcf}},\ m_{1}<i\leq m. (2.8)

As an example, for equation

2x2.4D2.4u(x)3x1.8D1.5u(x)+xD0.4u(x)+(x3ν2)u(x)=02x^{2.4}D^{2.4}u(x)-3x^{1.8}D^{1.5}u(x)+xD^{0.4}u(x)+(x^{3}-\nu^{2})u(x)=0

we have d1=2d_{1}=2, d2=3d_{2}=-3, d3=1d_{3}=1, α1=2.4\alpha_{1}=2.4, α2=1.8\alpha_{2}=1.8, α3=0.4\alpha_{3}=0.4. Then β=3\beta=3, p2=0.3p_{2}=0.3, p3=0.6p_{3}=0.6, and we obtain b1=1b_{1}=1, b2=10b_{2}=10, b3=5b_{3}=5, their NLCD=10N_{LCD}=10. Thus,

s0=1NLCD=0.1,nβ0=βs0=30,np20=p2s0=3,np30=p3s0=6.s^{0}=\frac{1}{N_{LCD}}=0.1,\ n_{\beta}^{0}=\frac{\beta}{s^{0}}=30,\ n_{p_{2}}^{0}=\frac{p_{2}}{s^{0}}=3,\ n_{p_{3}}^{0}=\frac{p_{3}}{s^{0}}=6.

Since Ngsf=GCF(30,3,6)=3N_{gsf}={\rm GCF}(30,3,6)=3, then, finally,

s=s0Ngsf=0.3,nβ=303=10,np2=1,np3=2.s=s^{0}\cdot N_{gsf}=0.3,\ n_{\beta}=\frac{30}{3}=10,\ n_{p_{2}}=1,\ n_{p_{3}}=2.

Other examples are presented in Sections 5 and 6.

Equation (2) can be re-written to identify more clearly the recursive relationship of the coefficients cnc_{n}:

n=0cnxγ+sn(i=1m1diQ(ns,αi)ν2)+\displaystyle\sum_{n=0}^{\infty}c_{n}x^{\gamma+sn}\left(\sum_{i=1}^{m_{1}}d_{i}Q(ns,\alpha_{i})-\nu^{2}\right)+
i=m1+1m(n=npicnxγ+sndiQ(ns+pi,αi))+n=nβcnxγ+sn=0.\displaystyle\!\!\!\!\sum_{i=m_{1}+1}^{m}\left(\sum_{n=n_{p_{i}}}^{\infty}c_{n}x^{\gamma+sn}d_{i}Q(ns+p_{i},\alpha_{i})\right)+\sum_{n=n_{\beta}}^{\infty}c_{n}x^{\gamma+sn}=0.\>\>\>\>\>\> (2.9)

As long as condition (1.8) for xγx^{\gamma} at n=0n=0 is satisfied, we can make c0c_{0} equal to any number. For simplicity we assume c0=1c_{0}=1. Then, to make equation (2) valid, we need to offset cnc_{n} by the sum of coefficients cnpic_{n}^{p_{i}} and cnβc_{n}^{\beta}

cn=cnβ+i=m1+1mcnpi.c_{n}=c_{n}^{\beta}+\sum_{i=m_{1}+1}^{m}c_{n}^{p_{i}}.

Coefficient cnc_{n} should compensate previous like terms, the terms which are nβn_{\beta} steps before cnc_{n} together with the terms which are npin_{p_{i}} steps before cnc_{n} from (2).

These coefficients can be expressed as

cnpi=cnnpidpiQ((nnpi)s,αpi)i=1m1diQ(ns,αi)ν2,c_{n}^{p_{i}}=-\frac{c_{n-n_{p_{i}}}\cdot d_{p_{i}}Q\left((n-n_{p_{i}})s,\alpha_{p_{i}}\right)}{\displaystyle\sum_{i=1}^{m_{1}}d_{i}Q(ns,\alpha_{i})-\nu^{2}}, (2.10)

where dpid_{p_{i}} and αpi\alpha_{p_{i}} correspond to pi,m1<imp_{i},m_{1}<i\leq m from the original equation (2.1) and

cnβ=cnnβi=1m1diQ(ns,αi)ν2.c_{n}^{\beta}=-\frac{c_{n-n_{\beta}}}{\displaystyle\sum_{i=1}^{m_{1}}d_{i}Q(ns,\alpha_{i})-\nu^{2}}. (2.11)

These coefficients (2.10) and (2.11) are equal to zero up to the point npin_{p_{i}} for the terms cnpic_{n}^{p_{i}} and up to nβn_{\beta} for cnβc_{n}^{\beta}. Hence, we combine (2.10), (2.11) and obtain the following formula for coefficients cnc_{n}:

cn\displaystyle c_{n}\!\!\!\! =\displaystyle= U(nnβ)cnβ+i=m1+1mU(nnpi)cnpi\displaystyle\!\!U(n-n_{\beta})c_{n}^{\beta}+\sum_{i=m_{1}+1}^{m}U(n-n_{p_{i}})c_{n}^{p_{i}}
=\displaystyle= U(nnβ)cnnβ+i=m1+1mU(nnpi)cnnpidiQ((nnpi)s,αi)i=1m1diQ(ns,αi)ν2,\displaystyle\!\!-\frac{U(n-n_{\beta})c_{n-n_{\beta}}+\displaystyle\sum_{i=m_{1}+1}^{m}U(n-n_{p_{i}})c_{n-n_{p_{i}}}\cdot d_{i}Q((n-n_{p_{i}})s,\alpha_{i})}{\displaystyle\sum_{i=1}^{m_{1}}d_{i}Q(ns,\alpha_{i})-\nu^{2}},

where U(nk)={1 if nk0 if n<kU(n-k)=\begin{cases}1\text{ if }n\geq k\\ 0\text{ if }n<k\end{cases} and Q(r,p),s,npi,nβQ(r,p),s,n_{p_{i}},n_{\beta} are defined in (2.4), (2.8). This algorithm provides the fractional series solution for equation (2.1).

3 Existence theorem

In this section we prove that the constructed fractional series solution and matching power xαx^{\alpha} and the highest derivative (i.e., p1=0p_{1}=0) is the necessary and sufficient condition to obtain the series solution (2.2) where coefficients are defined in (2). Based on the formulas in the previous section it looks like the described logic provides a solution to equation (2.1) if at least one pi=0,i=1,,mp_{i}=0,i=1,...,m (not necessarily p1=0p_{1}=0). However, this is not the case as shown in Theorem 2 below.

Let nm0=max1im0{ni}n_{m_{0}}=\displaystyle\max_{1\leq i\leq m_{0}}{\{n_{i}\}} where ni1<αi<ni,ni,i=1,,m0n_{i}-1<\alpha_{i}<n_{i},\ n_{i}\in\mathbb{N},i=1,...,m_{0}. Here m0m1m_{0}\leq m_{1} is the number of fractional derivatives and m1m0m_{1}-m_{0} is the number of integer derivatives with pi=0p_{i}=0 in equation (2.1) or the number of integer derivatives in multi-term fractional Bessel equation (1.5).

Theorem 1.

[5]. There exists a series solution (1.6),(1.7) for fractional equation (1.5) with Caputo derivatives with all di>0d_{i}>0 in any domain x[0,b],b+x\in[0,b],b\in\mathbb{R_{+}} if ν\nu satisfies the inequality

ν2=νmin2Γ(nm0)i=1m1diΓ(nmaxαi).\nu^{2}=\nu^{2}_{\min}\geq\Gamma(n_{m_{0}})\sum_{i=1}^{m_{1}}\frac{d_{i}}{\Gamma(n_{\max}-\alpha_{i})}. (3.1)

If ν=0\nu=0 and βnm01\beta\geq n_{m_{0}}-1 then at least one solution in the form of series can always be found.
If αmax=max1im1{αi}\displaystyle\alpha_{\max}^{*}=\max_{1\leq i\leq m_{1}}\{\alpha_{i}\} (the highest value of αi\alpha_{i} with pi=0p_{i}=0) is fractional and νmin>0\nu_{\min}>0, then the series solution is unique.
If αmax\alpha_{\max}^{*} is integer and νmin>0\nu_{\min}>0, then the series solution is unique provided that nm0αmax1n_{m_{0}}\geq\alpha_{\max}^{*}-1.
If nm0<αmax1n_{m_{0}}<\alpha_{\max}^{*}-1, then there may be several series solutions. ∎

Remark 1.

If there exists nn such that γ+sn\gamma+sn is another root of (1.8) with step ss defined in (2.8), then γ\gamma does not generate solution (2.2) for equation (2.1) because in this case the series is divergent.

It usually happens when ν=0\nu=0 and only p1=0p_{1}=0. Then the difference between γ\gamma roots is exactly one. If step ss is a fraction of one, smaller γ\gamma root at some step falls onto a bigger γ\gamma root and the series blows up.

For example, equation

x1.5D1.5u(x)+x0.7D0.5u(x)+(x1.20)u(x)=0x^{1.5}D^{1.5}u(x)+x^{0.7}D^{0.5}u(x)+(x^{1.2}-0)u(x)=0

has characteristic equation

Γ(1+γ)Γ(1+γ1.5)=0.\frac{\Gamma(1+\gamma)}{\Gamma(1+\gamma-1.5)}=0.

Hence, β=65,p2=15,r=1\displaystyle\beta=\frac{6}{5},p_{2}=\frac{1}{5},r=1. NLCD=5,s=15,nβ=6,np2=1N_{LCD}=5,s=\displaystyle\frac{1}{5},n_{\beta}=6,n_{p_{2}}=1. Roots are γ1=0.5,γ2=0.5\gamma_{1}=-0.5,\gamma_{2}=0.5. Therefore γ2=γ1+5s\gamma_{2}=\gamma_{1}+5s, which means that for n=5n=5

Q(5s,α1)=Γ(1+γ1+5s)Γ(1+γ1+5sα1)=Γ(10.5+1)Γ(10.5+11.5)=Γ(0.5)Γ(0)=0,Q(5s,\alpha_{1})=\frac{\Gamma(1+\gamma_{1}+5s)}{\Gamma(1+\gamma_{1}+5s-\alpha_{1})}=\frac{\Gamma(1-0.5+1)}{\Gamma(1-0.5+1-1.5)}=\frac{\Gamma(-0.5)}{\Gamma(0)}=0,

which is in the denominator of c5c_{5} in (2) and makes c5=c_{5}=\infty, therefore γ1\gamma_{1} does not generate solution in the form of proposed series.

Equation (5.8) in Section 5 is also an example of this situation. ∎

Thus, if the characteristic equation (1.8) has several roots, then all roots except for the largest root need to be checked for validity.

Lemma 2.

(Watson’s lemma as a corollary of Sterling approximation for Γ\Gamma-function).

For any α\alpha\in\mathbb{C},

limnΓ(n)nαΓ(n+α)=1.\lim_{n\to\infty}\frac{\Gamma(n)n^{\alpha}}{\Gamma(n+\alpha)}=1. (3.2)

Theorem 2.

Series solution (2.2) with coefficients (2) of fractional quasi-Bessel equation (2.1) with p1=0p_{1}=0, di>0d_{i}>0, 1im11\leq i\leq m_{1}, converges and represents the solution of equation (2.1) provided that the threshold condition (3.1) for ν\nu is satisfied in the equations with Caputo derivatives. No such threshold condition is required for the equations with Riemann-Liouville derivatives.

If p1>0p_{1}>0 but for some i>1i>1 there exists at least one pi=0p_{i}=0, then the series diverges and a series solution in form (2.2) does not exist for equations with both Caputo and Riemann-Liouville derivatives.

Proof.

We evaluate this series starting from the element
cn>maxi{npi,nβ}c_{n}>\displaystyle\max_{i}\{n_{p_{i}},n_{\beta}\}, we get:

|cn|\displaystyle|c_{n}| \displaystyle\leq |cnnβ+i=m1+1mcnnpidiQ((nnpi)s,αi)j=1m1djQ(ns,αj)ν2|\displaystyle\left|\frac{c_{n-n_{\beta}}+\displaystyle\sum_{i=m_{1}+1}^{m}c_{n-n_{p_{i}}}\cdot d_{i}Q((n-n_{p_{i}})s,\alpha_{i})}{\displaystyle\sum_{j=1}^{m_{1}}d_{j}Q(ns,\alpha_{j})-\nu^{2}}\right|
\displaystyle\leq |cnnβj=1m1djQ(ns,αj)ν2|+i=m1+1m|di||cnnpiQ((nnpi)s,αi)j=1m1djQ(ns,αj)ν2|\displaystyle\left|\frac{c_{n-n_{\beta}}}{\displaystyle\sum_{j=1}^{m_{1}}d_{j}Q(ns,\alpha_{j})-\nu^{2}}\right|+\sum_{i=m_{1}+1}^{m}|d_{i}|\left|\frac{c_{n-n_{p_{i}}}\cdot Q((n-n_{p_{i}})s,\alpha_{i})}{\displaystyle\sum_{j=1}^{m_{1}}d_{j}Q(ns,\alpha_{j})-\nu^{2}}\right| (3.3)
\displaystyle\leq |k=0nnβ1j=1m1diQ((k+nβ)s,αj)ν2|\displaystyle\left|\displaystyle\prod_{k=0}^{n-n_{\beta}}\frac{1}{\displaystyle\sum_{j=1}^{m_{1}}d_{i}Q((k+n_{\beta})s,\alpha_{j})-\nu^{2}}\right|
+\displaystyle+ i=m1+1m|di|nnpi|k=0nnpiQ(ks,αi)j=1m1djQ((k+npj)s,αj)ν2|.\displaystyle\sum_{i=m_{1}+1}^{m}|d_{i}|^{n-n_{p_{i}}}\left|\displaystyle\prod_{k=0}^{n-n_{p_{i}}}\frac{Q(ks,\alpha_{i})}{\displaystyle\sum_{j=1}^{m_{1}}d_{j}Q((k+n_{p_{j}})s,\alpha_{j})-\nu^{2}}\right|. (3.4)

Let us evaluate the first term (3.3). Keeping in mind Remark 1, the denominator is not equal to zero except for the roots of the characteristic equation (1.8) and therefore since dj>0d_{j}>0 for 1jm11\leq j\leq m_{1} and infinite increase of Q(k,α)Q(k,\alpha), we can ignore ν2=const\nu^{2}={\rm const} because it does not effect convergence. Based on expression (2.4) for Q(r,p)Q(r,p) and Euler’s formula (3.2) we can conclude

|1j=1m1djQ((k+nβ)s,αj)||1d1Q((k+nβ)s,α1)|\displaystyle\left|\frac{1}{\displaystyle\sum_{j=1}^{m_{1}}d_{j}Q((k+n_{\beta})s,\alpha_{j})}\right|\leq\left|\frac{1}{d_{1}Q((k+n_{\beta})s,\alpha_{1})}\right|
=|Γ(1+γ+(k+nβ)sα1)d1Γ(1+γ+(k+nβ)s)|=O(|1d1(1+γ+(k+nβ)s)α1|)\displaystyle\ \ =\left|\frac{\Gamma(1+\gamma+(k+n_{\beta})s-\alpha_{1})}{d_{1}\Gamma(1+\gamma+(k+n_{\beta})s)}\right|=O\left(\left|\frac{1}{d_{1}(1+\gamma+(k+n_{\beta})s)^{\alpha_{1}}}\right|\right)
O(|1d1((k+nβ)s)α1|),k (since 1+γ=const>0).\displaystyle\ \ \leq O\left(\left|\frac{1}{d_{1}((k+n_{\beta})s)^{\alpha_{1}}}\right|\right),\ k\to\infty\ \text{ (since }1+\gamma={\rm const}>0).

Hence we derive (dj>0, 1jm1;α1>αi, 2im)(d_{j}>0,\ 1\leq j\leq m_{1};\ \ \alpha_{1}>\alpha_{i},\ 2\leq i\leq m):

|k=0nnβ1j=1m1(diQ((k+nβ)s,αj)ν2)|\displaystyle\left|\displaystyle\prod_{k=0}^{n-n_{\beta}}\frac{1}{\displaystyle\sum_{j=1}^{m_{1}}(d_{i}Q((k+n_{\beta})s,\alpha_{j})-\nu^{2})}\right| (3.5)
O([1d1nnβ+1(nβs)((1+nβ)s)((2+nβ)s)((nnβ+nβ)s)]α1)\displaystyle\ \ \ \leq O\left(\left[\frac{1}{d_{1}^{n-n_{\beta}+1}\big{(}n_{\beta}s\big{)}\big{(}(1+n_{\beta})s\big{)}\big{(}(2+n_{\beta})s\big{)}\cdot...\cdot\big{(}(n-n_{\beta}+n_{\beta})s\big{)}}\right]^{\alpha_{1}}\right)
=O([(nβ1)!(d1s)nnβ+1n!]α1)\displaystyle\ \ \ =O\left(\left[\frac{(n_{\beta}-1)!}{(d_{1}s)^{n-n_{\beta}+1}n!}\right]^{\alpha_{1}}\right)

Evaluation of the second term (3.4) is similar:

|Q(ks,αi)|=|Γ(1+γ+ks)Γ(1+γ+ksαi)|=O((1+γ+ks)αi).\displaystyle|Q(ks,\alpha_{i})|=\left|\frac{\Gamma(1+\gamma+ks)}{\Gamma(1+\gamma+ks-\alpha_{i})}\right|=O((1+\gamma+ks)^{\alpha_{i}}).

Since the largest root γ\gamma is less than some constant, then we can say that
0<1+γcγs=const,cγ0<1+\gamma\leq c_{\gamma}s={\rm const},\ c_{\gamma}\in\mathbb{N}. Therefore,

|k=0nnpiQ(ks,αi)|=O([(1+γ)(1+γ+s)(1+γ+2s)\displaystyle\left|\displaystyle\prod_{k=0}^{n-n_{p_{i}}}Q(ks,\alpha_{i})\right|=O\big{(}\big{[}(1+\gamma)(1+\gamma+s)(1+\gamma+2s)\cdot...
(1+γ+(nnpi)s)]αi)\displaystyle\ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \ \cdot(1+\gamma+(n-n_{p_{i}})s)\big{]}^{\alpha_{i}}\big{)}
O([cγs(cγs+s)(cγs+2s)(cγs+(nnpi)s)]αi)\displaystyle\leq O\big{(}\big{[}c_{\gamma}s(c_{\gamma}s+s)(c_{\gamma}s+2s)\cdot...\cdot(c_{\gamma}s+(n-n_{p_{i}})s)\big{]}^{\alpha_{i}}\big{)}
=O([snnpi+1(cγ+1)(cγ+2)((cγ+nnpi))]αi)\displaystyle=O\left(\left[s^{n-n_{p_{i}}+1}(c_{\gamma}+1)(c_{\gamma}+2)\cdot...\cdot((c_{\gamma}+n-n_{p_{i}}))\right]^{\alpha_{i}}\right)
=O([snnpi+1(cγ+nnpi)!cγ!]αi).\displaystyle=O\left(\left[s^{n-n_{p_{i}}+1}\frac{(c_{\gamma}+n-n_{p_{i}})!}{c_{\gamma}!}\right]^{\alpha_{i}}\right). (3.6)

Similarly to (3.5), we obtain

|k=0nnpj1j=1m1(djQ((k+npj)s,αj)ν2)|=O((npj1)!(d1s)nnpj+1n!)α1.\displaystyle\left|\displaystyle\prod_{k=0}^{n-n_{p_{j}}}\frac{1}{\displaystyle\sum_{j=1}^{m_{1}}(d_{j}Q((k+n_{p_{j}})s,\alpha_{j})-\nu^{2})}\right|=O\left(\frac{(n_{p_{j}}-1)!}{(d_{1}s)^{n-n_{p_{j}}+1}n!}\right)^{\alpha_{1}}.

Given that nβ,npi,dinβ,snβ,dinpi,snpi,m1<im,n_{\beta},n_{p_{i}},d_{i}^{n_{\beta}},s^{n_{\beta}},d_{i}^{n_{p_{i}}},s^{n_{p_{i}}},m_{1}<i\leq m, and cγc_{\gamma} are constants, we can ignore them in the evaluation of convergence.

Expression (3) becomes

O([sn(cγ+nnpi)!]αi)=O([sn(nnpi)!Pcγ]αi), where\displaystyle O\left(\left[s^{n}(c_{\gamma}+n-n_{p_{i}})!\right]^{\alpha_{i}}\right)=O\left(\left[s^{n}(n-n_{p_{i}})!P_{c_{\gamma}}\right]^{\alpha_{i}}\right),\ \text{ where }
Pcγ=(nnpi+1)(nnpi+2)(nnpi+cγ) is a polynomial of degree cγ.\displaystyle P_{c_{\gamma}}=(n-n_{p_{i}}+1)(n-n_{p_{i}}+2)...(n-n_{p_{i}}+c_{\gamma})\text{ is a polynomial of degree $c_{\gamma}$}.
Hence,
O([sn(cγ+nnpi)!]αi)=O([sn(nnpi)!ncγ]αi).\displaystyle O\left(\left[s^{n}(c_{\gamma}+n-n_{p_{i}})!\right]^{\alpha_{i}}\right)=O\left(\left[s^{n}(n-n_{p_{i}})!n^{c_{\gamma}}\right]^{\alpha_{i}}\right). (3.7)

Consequently, we obtain

|cn|\displaystyle|c_{n}| =\displaystyle= O(1((d1s)nn!)α1)+O(i=m1+1m|di|n[sn(nnpi)!ncγ]αi(d1nsnn!)α1)\displaystyle O\left(\frac{1}{((d_{1}s)^{n}n!)^{\alpha_{1}}}\right)+O\left(\sum_{i=m_{1}+1}^{m}|d_{i}|^{n}\frac{[s^{n}(n-n_{p_{i}})!n^{c_{\gamma}}]^{\alpha_{i}}}{(d_{1}^{n}s^{n}n!)^{\alpha_{1}}}\right) (3.8)
\displaystyle\leq O(1(d1nsnn!)α1)+O(i=m1+1m|di|nncγαid1nα1(snn!)α1αi).\displaystyle O\left(\frac{1}{(d_{1}^{n}s^{n}n!)^{\alpha_{1}}}\right)+O\left(\sum_{i=m_{1}+1}^{m}\frac{|d_{i}|^{n}n^{c_{\gamma}\alpha_{i}}}{d_{1}^{n\alpha_{1}}(s^{n}n!)^{\alpha_{1}-\alpha_{i}}}\right).

Since αi<α1,m1<im\alpha_{i}<\alpha_{1},\ m_{1}<i\leq m, then we can conclude that

|cn|xγ+snO(xsn(d1nsnn!)α1)+O(i=m1+1m(xs|di|)nncγαid1nα1(snn!)α1αi),|c_{n}|x^{\gamma+sn}\leq O\left(\frac{x^{sn}}{(d_{1}^{n}s^{n}n!)^{\alpha_{1}}}\right)+O\left(\sum_{i=m_{1}+1}^{m}\frac{(x^{s}|d_{i}|)^{n}n^{c_{\gamma}\alpha_{i}}}{d_{1}^{n\alpha_{1}}(s^{n}n!)^{\alpha_{1}-\alpha_{i}}}\right), (3.9)

Finally, series solution (2.2) for equation (2.1) uniformly converges on each bounded interval x[ϵ,b],ϵ>0x\in[\epsilon,b],\epsilon>0, and the solution is differentiable up to any order for x>0x>0.

Conversely, if p1>0p_{1}>0 but pi=0,i=2,,m1p_{i}=0,i=2,...,m_{1} then in this case

cn\displaystyle c_{n} =\displaystyle= U(nnβ)cnβ+i=m1+1mU(nnpi)cnpi+U(nnp1)cnp1\displaystyle U(n-n_{\beta})c_{n}^{\beta}+\sum_{i=m_{1}+1}^{m}U(n-n_{p_{i}})c_{n}^{p_{i}}+U(n-n_{p_{1}})c_{n}^{p_{1}}
=\displaystyle= U(nnβ)cnnβ+i=m1+1mU(nnpi)cnnpidiQ((nnpi)s,αi)i=2m1diQ(ns,αi)ν2\displaystyle-\frac{U(n-n_{\beta})c_{n-n_{\beta}}+\displaystyle\sum_{i=m_{1}+1}^{m}U(n-n_{p_{i}})c_{n-n_{p_{i}}}\cdot d_{i}Q((n-n_{p_{i}})s,\alpha_{i})}{\displaystyle\sum_{i=2}^{m_{1}}d_{i}Q(ns,\alpha_{i})-\nu^{2}}
U(nnp1)cnnp1Q((nnp1)s,α1)i=2m1diQ(ns,αi)ν2.\displaystyle-\frac{U(n-n_{p_{1}})c_{n-n_{p_{1}}}\cdot Q((n-n_{p_{1}})s,\alpha_{1})}{\displaystyle\sum_{i=2}^{m_{1}}d_{i}Q(ns,\alpha_{i})-\nu^{2}}.

Per expression (2.4) and Euler’s formula (3.2) and assuming that
αm=max2im1{αi}\alpha_{m}=\displaystyle\max_{2\leq i\leq m_{1}}\{\alpha_{i}\} and dmd_{m} corresponds to αm\alpha_{m}, we get as in the first part of the theorem

|cn|\displaystyle|c_{n}| =\displaystyle= O(1(dmnsnn!)αm)+O(i=m1+1mdin(sn(nnpi)!)αincγαidmnαm(snn!)αm)\displaystyle O\left(\frac{1}{(d_{m}^{n}s^{n}n!)^{\alpha_{m}}}\right)+O\left(\sum_{i=m_{1}+1}^{m}\frac{d_{i}^{n}(s^{n}(n-n_{p_{i}})!)^{\alpha_{i}}n^{c_{\gamma}\alpha_{i}}}{d_{m}^{n\alpha_{m}}(s^{n}n!)^{\alpha_{m}}}\right) (3.10)
+\displaystyle+ O(d1nncγα1dmnαm(snn!)αmα1).\displaystyle O\left(\frac{d_{1}^{n}n^{c_{\gamma}\alpha_{1}}}{d_{m}^{n\alpha_{m}}(s^{n}n!)^{\alpha_{m}-\alpha_{1}}}\right).

Since α1>αm\alpha_{1}>\alpha_{m} then the last addend dominates two other terms in (3.10) and is divergent. Hence, |cn||c_{n}|\to\infty as nn\to\infty and the series solution is divergent for any value of x>0x>0 in (2.2).

Thus, condition p1=0p_{1}=0 is necessary for the existence of a series solution. As an additional remark, we should point out that the positivity of coefficients did_{i} is required only for the terms where the order of the derivative is equal to the power of multiplier xx. In this case characteristic equation (1.8) is guaranteed to have real roots. ∎

Remark 2.

For equations with Caputo derivative based on conditions in Theorem 1:

  • If p1=0,ν>0p_{1}=0,\nu>0 and α1\alpha_{1} is fractional then the found series solution is unique up to a constant,

  • It p1=0p_{1}=0 and α1\alpha_{1} is integer equation (2.1) may have multiple solutions.

Remark 3.

Root γ\gamma in the solution, which is calculated in (2.3), depends solely on the terms in equation (2.1) with pi=0p_{i}=0. ∎

Remark 4.

If in addition to p1=0p_{1}=0 any other pi=0p_{i}=0, it only improves convergence since the denominator in the calculations of the coefficients (2) has more terms and cnc_{n} faster converges to zero. ∎

4 Uniqueness for the initial value problem

We can expand Theorem 2 in [5] for multi-term fractional Bessel equation to the fractional quasi-Bessel equation (2.1) with positive coefficients did_{i}.

Theorem 3.

The initial value problem for fractional equation (2.1) with Caputo derivatives with the domain x[0,b]x\in[0,b] and initial conditions u(j)(0)=u0(j),j=0,1,,l1,u^{(j)}(0)=u^{(j)}_{0},j=0,1,...,l-1, where l=α1\displaystyle l=\lceil\alpha_{1}\rceil, has a unique solution for every ν\nu\in\mathbb{R} such that

ν2>b1β+i=1mqi|di|b1ni+pi\nu^{2}>b_{1}^{\beta}+\sum_{i=1}^{m}q_{i}|d_{i}|b_{1}^{n_{i}+p_{i}} (4.1)

where

b1=max{1,b} and qi={1Γ(niαi)(niαi+1),αi<ni1,αi=ni.\displaystyle b_{1}=\max\{1,b\}\text{ and }q_{i}=\begin{cases}\displaystyle\frac{1}{\Gamma(n_{i}-\alpha_{i})(n_{i}-\alpha_{i}+1)}&,\alpha_{i}<n_{i}\\ 1&,\alpha_{i}=n_{i}\end{cases}. (4.2)
Proof.

We denote by ClC^{l} the space of functions uu which are ll times continuously differentiable on [0,b][0,b] with the norm

uCl=k=0lu(k)C=k=0lmaxx[0,b]|u(k)(x)|.||u||_{C^{l}}=\sum_{k=0}^{l}||u^{(k)}||_{C}=\sum_{k=0}^{l}\max_{x\in[0,b]}|u^{(k)}(x)|.

Operator T:ClCT:C^{l}\mapsto C is defined as follows

(Tu)(x)=1ν2[xβu(x)+i=1mdixαi+piDCαiu(x)].(Tu)(x)=\frac{1}{\nu^{2}}\left[x^{\beta}u(x)+\sum_{i=1}^{m}d_{i}x^{\alpha_{i}+p_{i}}D_{C}^{\alpha_{i}}u(x)\right].

Then, we can write general equation in the form u(x)=(Tu)(x)u(x)=(Tu)(x). Taking into account formulas 2.4.24-26 in Corollary 2.3 for Caputo derivative in Chapter 2 from [8] for the interval [0,b][0,b], we have:

DCαiuCkαiuCl, where kαi=bniαiΓ(niαi)(niαi+1), when αi<ni||D_{C}^{\alpha_{i}}u||_{C}\leq k_{\alpha_{i}}||u||_{C^{l}},\text{ where }k_{\alpha_{i}}=\frac{b^{n_{i}-\alpha_{i}}}{\Gamma(n_{i}-\alpha_{i})(n_{i}-\alpha_{i}+1)},\text{ when }\alpha_{i}<n_{i}

and

DCαiuC=uCl, when αi=ni.||D_{C}^{\alpha_{i}}u||_{C}=||u||_{C^{l}},\text{ when }\alpha_{i}=n_{i}.

Therefore,

DCαiuCqibniαiuCl,||D_{C}^{\alpha_{i}}u||_{C}\leq q_{i}b^{n_{i}-\alpha_{i}}||u||_{C^{l}},

and we obtain

Tu1Tu2C\displaystyle||Tu_{1}-Tu_{2}||_{C} =\displaystyle= 1ν2xβ(u1(x)u2(x))+i=1mdixαi+piDCαi(u1u2)(x)C\displaystyle\frac{1}{\nu^{2}}||x^{\beta}(u_{1}(x)-u_{2}(x))+\sum_{i=1}^{m}d_{i}x^{\alpha_{i}+p_{i}}D_{C}^{\alpha_{i}}(u_{1}-u_{2})(x)||_{C} (4.3)
\displaystyle\leq 1ν2(b1βu1u2C+i=1m|di|b1αi+piqibniαiu1u2Cl)\displaystyle\frac{1}{\nu^{2}}\left(b_{1}^{\beta}||u_{1}-u_{2}||_{C}+\sum_{i=1}^{m}|d_{i}|b_{1}^{\alpha_{i}+p_{i}}q_{i}b^{n_{i}-\alpha_{i}}||u_{1}-u_{2}||_{C^{l}}\right)
\displaystyle\leq 1ν2(b1β+i=1mqi|di|b1ni+pi)u1u2Cl.\displaystyle\frac{1}{\nu^{2}}\left(b_{1}^{\beta}+\sum_{i=1}^{m}q_{i}|d_{i}|b_{1}^{n_{i}+p_{i}}\right)||u_{1}-u_{2}||_{C^{l}}.

Having condition (4.1) we conclude that TT is a contraction. We apply the Banach fix point theorem to complete the proof. ∎

5 Equations with constant coefficients

Let us consider equation with constant coefficients at each derivative:

i=1mdiDαiu(x)+u(x)=0,α1>αi>0,i=2,,m\sum_{i=1}^{m}d_{i}D^{\alpha_{i}}u(x)+u(x)=0,\alpha_{1}>\alpha_{i}>0,\ i=2,...,m (5.1)

and assume that there exists a real positive number rr such that for all ii, 1im1\leq i\leq m, αir+=r+\alpha_{i}\in\mathbb{Q}_{r}^{+}=r\mathbb{Q^{+}} We multiply each term by xα1x^{\alpha_{1}}. Then we obtain

d1xα1Dα1u(x)+i=2mdixα1Dαiu(x)+(xα10)u(x)=0,d_{1}x^{\alpha_{1}}D^{\alpha_{1}}u(x)+\sum_{i=2}^{m}d_{i}x^{\alpha_{1}}D^{\alpha_{i}}u(x)+(x^{\alpha_{1}}-0)u(x)=0, (5.2)

which is the quasi-Bessel equation (2.1) with ν=0,β=α1\nu=0,\beta=\alpha_{1}. Let us apply the methodology from Section 2. In this case characteristic equation (1.8) becomes

Γ(1+γ)Γ(1+γα1)=0,\frac{\Gamma(1+\gamma)}{\Gamma(1+\gamma-\alpha_{1})}=0, (5.3)

and we arrive at roots γ=α1k,k1\gamma=\alpha_{1}-k,k\geq 1. Since only one term has matching power of xx, then in this case the roots do not depend on the coefficients did_{i}.

If α1\alpha_{1} is integer then (5.3) provides α1\alpha_{1} roots. In the case when α1\alpha_{1} is truly fractional, i.e. α1α1\lceil\alpha_{1}\rceil\neq\alpha_{1}, we can see that all roots γ<α1\gamma<\lceil\alpha_{1}\rceil and therefore characteristic equation does not produce any solutions for constant-coefficient equations with Caputo derivatives unless γ\gamma is a non-negative integer. In this case, the Caputo derivative DCα1xjD_{C}^{\alpha_{1}}x^{j} is equal to zero and solutions can be found without the use of characteristic equation. For example, for the simple equation

DCαu(x)λu(x)=0, 0<α<1,λD^{\alpha}_{C}u(x)-\lambda u(x)=0,\ 0<\alpha<1,\lambda\in\mathbb{R} (5.4)

solution exists [8] as a specific series – the Mittag-Leffler function

u(x)=bEα[λxα]=bn=0λnxnαΓ(1+αn),b=u(0).u(x)=bE_{\alpha}[\lambda x^{\alpha}]=b\sum_{n=0}^{\infty}\frac{\lambda^{n}x^{n\alpha}}{\Gamma(1+\alpha n)},b=u(0)\in\mathbb{R}.

Our formula for coefficients produces identical result with β=α\beta=\alpha,
d1=1λ,c0=bd_{1}=-\frac{1}{\lambda},c_{0}=b,

cn+1=cnλΓ(1+αn)Γ(1+α(n+1)=λn+1Γ(1+α(n+1)).c_{n+1}=\frac{c_{n}\lambda\Gamma(1+\alpha n)}{\Gamma(1+\alpha(n+1)}=\frac{\lambda^{n+1}}{\Gamma(1+\alpha(n+1))}.

In the case of equation (5.2) with Riemann-Liouville derivatives the restriction on γ\gamma is much milder: γ>1\gamma>-1, and, therefore, each root
γ=α1k,k=1,,nmax\gamma=\alpha_{1}-k,k=1,...,n_{\max} generates a solution for equation (5.2) as long as it does not represent a root that becomes another root at some step nn as described in Remark 1. In this case only the solution that corresponds to the largest root γ\gamma exists.

Example. Characteristic equation (5.3) of the equation

d1DR2.1u(x)+d2DR1.4u(x)+d3DR0.7u(x)+u(x)=0, or\displaystyle d_{1}D_{R}^{2.1}u(x)+d_{2}D_{R}^{1.4}u(x)+d_{3}D_{R}^{0.7}u(x)+u(x)=0,\text{ or }
d1x2.1DR2.1u(x)+d2x1.4+0.7DR1.4u(x)+d3x0.7+1.4DR0.7u(x)\displaystyle d_{1}x^{2.1}D_{R}^{2.1}u(x)+d_{2}x^{1.4+0.7}D_{R}^{1.4}u(x)+d_{3}x^{0.7+1.4}D_{R}^{0.7}u(x)
+(x2.10)u(x)=0,\displaystyle+(x^{2.1}-0)u(x)=0,
α1=2.1,p2=0.7,p3=1.4,β=2.1,\displaystyle\alpha_{1}=2.1,\ \ p_{2}=0.7,\ \ p_{3}=1.4,\ \ \beta=2.1,

has three roots: γ1=0.9,γ2=0.1\gamma_{1}=-0.9,\gamma_{2}=0.1 and γ3=1.1\gamma_{3}=1.1. The orders of the derivatives yield step s=0.7s=0.7. Therefore γ2γ1+sn,γ3γ1+sn,γ3γ2+sn\gamma_{2}\neq\gamma_{1}+sn,\gamma_{3}\neq\gamma_{1}+sn,\gamma_{3}\neq\gamma_{2}+sn for any nn\in\mathbb{N}. Consequently, we can construct three different series solutions based on these roots

u1(x)=n=0cnx0.9+sn\displaystyle u_{1}(x)=\sum_{n=0}^{\infty}c_{n}x^{-0.9+sn} (5.5)
u2(x)=n=0cnx0.1+sn\displaystyle u_{2}(x)=\sum_{n=0}^{\infty}c_{n}x^{0.1+sn} (5.6)
u3(x)=n=0cnx1.1+sn.\displaystyle u_{3}(x)=\sum_{n=0}^{\infty}c_{n}x^{1.1+sn}. (5.7)

In the case of almost the same equation

d1DR2.1u(x)+d2DR1.5u(x)+d3DR0.7u(x)+u(x)=0,d_{1}D_{R}^{2.1}u(x)+d_{2}D_{R}^{1.5}u(x)+d_{3}D_{R}^{0.7}u(x)+u(x)=0,

which turns into

d1x2.1DR2.1u(x)+d2x1.5+0.6DR1.5u(x)+d3x0.7+1.4DR0.7u(x)+x2.1u(x)=0,d_{1}x^{2.1}D_{R}^{2.1}u(x)+d_{2}x^{1.5+0.6}D_{R}^{1.5}u(x)+d_{3}x^{0.7+1.4}D_{R}^{0.7}u(x)+x^{2.1}u(x)=0, (5.8)

we obtain the same three roots γ1=0.9,γ2=0.1\gamma_{1}=-0.9,\gamma_{2}=0.1 and γ3=1.1\gamma_{3}=1.1, but the step here becomes s=0.1s=0.1. In this case, γ2=0.1=0.9+100.1=γ1+10s\gamma_{2}=0.1=-0.9+10\cdot 0.1=\gamma_{1}+10s, which makes c10=c_{10}=\infty, which invalidates series solution (5.5); γ3=1.1=0.1+100.1=γ2+10s\gamma_{3}=1.1=0.1+10\cdot 0.1=\gamma_{2}+10s, which also makes c10=c_{10}=\infty, and therefore invalidates series solution (5.6) (see detailed explanation in example in Remark 1). Consequently, neither γ1\gamma_{1} nor γ2\gamma_{2} represent a root which can be used to generate a series solution in the proposed form.

Root γ3=α11\gamma_{3}=\alpha_{1}-1 (γ3=1.1\gamma_{3}=1.1 in our example) is the largest and, in view of Remark 1, cannot be eliminated and is always valid. Therefore, in the case of equation (5.1) with Riemann-Liouville derivatives we can always generate at least one series solution

u(x)=n=0cnxα11+snu(x)=\sum_{n=0}^{\infty}c_{n}x^{\alpha_{1}-1+sn} (5.9)

since, unlike roots γ1,γ2\gamma_{1},\gamma_{2} of the characteristic equation, root γ3\gamma_{3} does not generate blow-up of the series solution.

Step ss is described in Section 2 for our modified equation (5.2), in which
pi=α1αi,β=α1,ν=0p_{i}=\alpha_{1}-\alpha_{i},\beta=\alpha_{1},\nu=0, and the coefficients are calculated based on equation (2). ∎

As we see, constant-coefficient equations with Rieman-Liouville derivatives can be transformed into quasi-Bessel equations. Examples 2 and 3 in Section 6 provide additional demonstrations of this ansatz.

Besides constant coefficients, the methodology described above is also applicable to equations with some terms having factors as powers of xx. We assume that β1\beta_{1}, the power of xx at the highest derivative α1\alpha_{1}, satisfies inequality β1α1\beta_{1}\leq\alpha_{1}. We consider equation

i=1mdixβiDRαiu(x)+xδu(x)=0,\displaystyle\sum_{i=1}^{m}d_{i}x^{\beta_{i}}D_{R}^{\alpha_{i}}u(x)+x^{\delta}u(x)=0, (5.10)
α1>αi>0,i=2,,m,α1β1,α1β1αiβi,\displaystyle\alpha_{1}>\alpha_{i}>0,i=2,...,m,\ \alpha_{1}\geq\beta_{1},\ \alpha_{1}-\beta_{1}\geq\alpha_{i}-\beta_{i},

where αi,βi,δr+=r+\alpha_{i},\beta_{i},\delta\in\mathbb{Q}_{r}^{+}=r\mathbb{Q^{+}} for some r+r\in\mathbb{R^{+}}. We multiply each term by xα1β1x^{\alpha_{1}-\beta_{1}} and obtain

d1xα1DRα1u(x)+i=2mdixα1β1+βiDRαiu(x)+(xα1β1+δ0)u(x)=0,d_{1}x^{\alpha_{1}}D_{R}^{\alpha_{1}}u(x)+\sum_{i=2}^{m}d_{i}x^{\alpha_{1}-\beta_{1}+\beta_{i}}D_{R}^{\alpha_{i}}u(x)+(x^{\alpha_{1}-\beta_{1}+\delta}-0)u(x)=0, (5.11)

which is a quasi-Bessel equation. In this case ν=0,β=α1β1+δ\nu=0,\beta=\alpha_{1}-\beta_{1}+\delta. Then, we can apply the above described methodology for equations with constant coefficients to this equation. In this case characteristic equation (1.8) is exactly the same as for equation with constant coefficients (5.3), and the approach for solving equations with constant coefficients applies verbatim.

Examples of equations with constant coefficients and with terms having powers of xx as factors are in Section 6, Examples 2-4.

6 Examples of some equations and their solutions.

Example 1 (quasi-Bessel equation with Caputo derivatives).

Let us consider equation

1.5x1.5DC1.5u(x)1.2x1.9DC1.1u(x)+3xDC0.5u(x)+(x2ν2)u(x)=0.1.5x^{1.5}D_{C}^{1.5}u(x)-1.2x^{1.9}D_{C}^{1.1}u(x)+3xD_{C}^{0.5}u(x)+(x^{2}-\nu^{2})u(x)=0. (6.1)

Here β=2,d1=1.5,d2=1.2,d3=3,α1=1.5,α2=1.1,α3=0.5,p2=0.8,p3=0.5\beta=2,d_{1}=1.5,d_{2}=-1.2,d_{3}=3,\alpha_{1}=1.5,\alpha_{2}=1.1,\alpha_{3}=0.5,\\ p_{2}=0.8,p_{3}=0.5.

Equation (2.3) becomes:

G(γ)=1.5Γ(1+γ)Γ(1+γ1.5)ν2=0.G(\gamma)=\frac{1.5\Gamma(1+\gamma)}{\Gamma(1+\gamma-1.5)}-\nu^{2}=0. (6.2)

The graph of the expression on the left side of equation (6.2) is in Figure 1. It is the same for any ν\nu except for the ν2\nu^{2} shift down difference. To satisfy equation (6.2) for ν=2\nu=2 we found γ=2.1995\gamma=2.1995, for ν=3.5\nu=3.5γ=4.3181\gamma=4.3181 (see [5] for the detail explanation on how to find all γ\gamma).

Refer to caption
Figure 1: Function G(γ)ν2G(\gamma)-\nu^{2} for equation (6.1) with ν=2\nu=2.

Other parameters involved in the process as described before are:

  • Since all pi,β+p_{i},\beta\in\mathbb{Q^{+}} we get p20=p2=0.8=45;\displaystyle p_{2}^{0}=p_{2}=0.8=\frac{4}{5};
    p30=p3=0.5=12;s0=β=2=21\displaystyle p_{3}^{0}=p_{3}=0.5=\frac{1}{2};\ \ \ s^{0}=\beta=2=\frac{2}{1}.

  • The lowest common denominator NLCD=LCM{5,2,1}=10N_{LCD}=\text{LCM}\{5,2,1\}=10.

  • s=1NLCD=110=0.1,np2=p2s=0.80.1=8,np3=p3s=0.50.1=5\displaystyle s=\frac{1}{N_{LCD}}=\frac{1}{10}=0.1,n_{p_{2}}=\frac{p_{2}}{s}=\frac{0.8}{0.1}=8,n_{p_{3}}=\frac{p_{3}}{s}=\frac{0.5}{0.1}=5,
    nβ=βs=20.1=20,(Ngcf=1)n_{\beta}=\displaystyle\frac{\beta}{s}=\frac{2}{0.1}=20,(N_{gcf}=1).

The solutions are represented in Figure 2. Red line - recalculation of equation (6.1) by plugging in the calculated solution u(x)u(x) into the equation. Fractional derivatives are calculated using the substitution method for calculation of Caputo fractional derivatives as in [6].

Refer to caption
Refer to caption
Figure 2: Solution for equation in Example 1. Red line close to zero is the check for the accuracy of the solution. Step h=0.001h=0.001.

It is important to understand that the closer ν\nu is to the minimum acceptable ν\nu as explained in [5], the less accurate the result is due to loss of accuracy in the calculation of fractional derivative.

Figure 3 reflects distributions of cnc_{n} for two cases of ν\nu. It’s easy to see that coefficients converge to zero very fast.

Refer to caption
Refer to caption
Figure 3: Example 1. Distribution of coefficients (cn>105c_{n}>10^{-5}).

The solution becomes unstable on a larger interval because xγ+snx^{\gamma+sn} becomes a very large number and more terms in the sequence are needed for accurate results but these terms are a product of a very small coefficient cnc_{n} and very large power of xx which numerically becomes unstable. If a solution is needed on a larger interval we can solve the equation using the substitution technique [6] after making sure that it matches on a smaller interval. The solution at zero is zero and its first derivative is also zero. With these initial conditions the substitution method only finds the trivial solution. We can slightly perturb the system by assigning a small value for the derivative and, as we know, it only effects the constant in front of the function u(x)u(x). After this minor perturbation/calibration of the first derivative we can generate the solution on a larger interval. These solutions are shown in Figure 4.

Refer to caption
Refer to caption
Figure 4: Example 1. Light Blue - exact series solution, red - solution generated by the substitution method [6]. On [0,5] graphs of both methods match.



Example 2 (constant coefficients, integer derivatives).

This example demonstrates how the methodology works on a very simple example for which we know the analytic solution.

u+u=0.u^{\prime}+u=0.

We know that its solution is u=Cexu=Ce^{-x}. Our method converts this equation into

xu+xu=0xu^{\prime}+xu=0

and states that series solution exists and is in the form u(x)=n=0cnxsnu(x)=\displaystyle\sum_{n=0}^{\infty}c_{n}x^{sn}.
Solution for characteristic equation

Γ(1+γ)Γ(1+γ1)=0\frac{\Gamma(1+\gamma)}{\Gamma(1+\gamma-1)}=0

is γ=0\gamma=0. Based on (2.8) step s=1s=1. Therefore, we get

cn=cnβ=cn1Q(n,1)=cn1Γ(1+n1)Γ(1+n)=cn1n=c0(1)nn!c_{n}=c_{n}^{\beta}=-\frac{c_{n-1}}{Q(n,1)}=-c_{n-1}\frac{\Gamma(1+n-1)}{\Gamma(1+n)}=-\frac{c_{n-1}}{n}=c_{0}\frac{(-1)^{n}}{n!}

and the solution as expected is

u(x)=n=0cnxsn=c0n=0(1)nn!xn=c0ex.u(x)=\sum_{n=0}^{\infty}c_{n}x^{sn}=c_{0}\sum_{n=0}^{\infty}\frac{(-1)^{n}}{n!}x^{n}=c_{0}e^{-x}.



Example 3 (fractional derivative with constant coefficients).

Let us consider equation 4.1.21 [8] with specific values of parameters

DR1.7u(x)2u(x)=0\displaystyle D_{R}^{1.7}u(x)-2u(x)=0 (6.3)

with initial conditions

DR0.7u(0)=1.2,DR0.3u(0)=1.5.\displaystyle D_{R}^{0.7}u(0)=1.2,D_{R}^{-0.3}u(0)=1.5. (6.4)

The characteristic equation for (6.3) becomes

Γ(1+γ)Γ(1+γ1.7)=0.\frac{\Gamma(1+\gamma)}{\Gamma(1+\gamma-1.7)}=0. (6.5)

It has two roots with γ>1:γ1=0.7,γ2=0.3\gamma>-1:\gamma_{1}=0.7,\gamma_{2}=-0.3. Step s=1.7s=1.7
(no pi;β=1.7p_{i};\beta=1.7). Therefore we get two series solutions:

u(x)\displaystyle u(x) =\displaystyle= n=0cn1x0.7+1.7n,\displaystyle\sum_{n=0}^{\infty}c_{n}^{1}x^{0.7+1.7n},
u(x)\displaystyle u(x) =\displaystyle= n=0cn2x0.3+1.7n.\displaystyle\sum_{n=0}^{\infty}c_{n}^{2}x^{-0.3+1.7n}.

In this case (since coefficient in front of u(x)u(x) needs to be one) d1=0.5d_{1}=-0.5 and therefore

cn1=cn11Γ(1+0.7+1.7n1.7)0.5Γ(1+0.7+1.7n)=cn112Γ(1.7n)Γ(1.7+1.7n)=c012nΓ(1.7)Γ(1.7+1.7n)\displaystyle c_{n}^{1}=-\frac{c_{n-1}^{1}\Gamma(1+0.7+1.7n-1.7)}{-0.5\Gamma(1+0.7+1.7n)}=c_{n-1}^{1}\frac{2\Gamma(1.7n)}{\Gamma(1.7+1.7n)}=c_{0}^{1}\frac{2^{n}\Gamma(1.7)}{\Gamma(1.7+1.7n)}\
cn2=cn12Γ(10.3+1.7n1.7)0.5Γ(10.3+1.7n)=cn122Γ(1.7n1)Γ(0.7+1.7n)=c022nΓ(0.7)Γ(0.7+1.7n).\displaystyle c_{n}^{2}=-\frac{c_{n-1}^{2}\Gamma(1-0.3+1.7n-1.7)}{-0.5\Gamma(1-0.3+1.7n)}=c_{n-1}^{2}\frac{2\Gamma(1.7n-1)}{\Gamma(0.7+1.7n)}=c_{0}^{2}\frac{2^{n}\Gamma(0.7)}{\Gamma(0.7+1.7n)}.

Then, the solution is

u(x)\displaystyle u(x) =\displaystyle= c01n=0Γ(1.7)2nx0.7+1.7nΓ(1.7+1.7n)+c02n=0Γ(0.7)2nx0.3+1.7nΓ(0.7+1.7n)\displaystyle c_{0}^{1}\sum_{n=0}^{\infty}\frac{\Gamma(1.7)2^{n}x^{0.7+1.7n}}{\Gamma(1.7+1.7n)}+c_{0}^{2}\sum_{n=0}^{\infty}\frac{\Gamma(0.7)2^{n}x^{-0.3+1.7n}}{\Gamma(0.7+1.7n)} (6.6)
=\displaystyle= c01Γ(1.7)n=02nx0.7+1.7nΓ(1.7+1.7n)+c02Γ(0.7)n=02nx0.3+1.7nΓ(0.7+1.7n).\displaystyle c_{0}^{1}\Gamma(1.7)\sum_{n=0}^{\infty}\frac{2^{n}x^{0.7+1.7n}}{\Gamma(1.7+1.7n)}+c_{0}^{2}\Gamma(0.7)\sum_{n=0}^{\infty}\frac{2^{n}x^{-0.3+1.7n}}{\Gamma(0.7+1.7n)}.\ \ \ \>\>

Let us see what initial condition (6.4) gives us [15]:

DR0.7u(0)\displaystyle D_{R}^{0.7}u(0) =\displaystyle= c01Γ(1.7)Γ(1+0.7)Γ(1.7)Γ(1+0.70.7)+0=c01Γ(1.7)=1.2\displaystyle c_{0}^{1}\Gamma(1.7)\frac{\Gamma(1+0.7)}{\Gamma(1.7)\Gamma(1+0.7-0.7)}+0=c_{0}^{1}\Gamma(1.7)=1.2
DR0.3u(0)\displaystyle D_{R}^{-0.3}u(0) =\displaystyle= 0+c02Γ(0.7)Γ(10.3)Γ(10.3+0.3)Γ(0.7)=c02Γ(0.7)=1.5,\displaystyle 0+c_{0}^{2}\Gamma(0.7)\frac{\Gamma(1-0.3)}{\Gamma(1-0.3+0.3)\Gamma(0.7)}=c_{0}^{2}\Gamma(0.7)=1.5,

which makes solution (6.6) the same as previously identified in [8] analytical solution. ∎

Example 4 (fractional derivatives with powers of xx).

Let us apply the methodology to another example from [8], Example 4.1.36.

DR0.5u(x)λxβu(x)=0,DR0.5u(0)=b.\displaystyle D_{R}^{0.5}u(x)-\lambda x^{\beta}u(x)=0,D_{R}^{-0.5}u(0)=b. (6.7)

For simplicity sake we will assume that β=0.7+\beta=0.7\in\mathbb{Q^{+}}. Then, our interpretation of this problem is

1λx0.5DR0.5u(x)+x1.2u(x)=0,DR0.5u(0)=b.\displaystyle-\frac{1}{\lambda}x^{0.5}D_{R}^{0.5}u(x)+x^{1.2}u(x)=0,D_{R}^{-0.5}u(0)=b. (6.8)

Characteristic equation (5.3) produces one root γ=0.5\gamma=-0.5, step s=1.2s=1.2, and nβ=1n_{\beta}=1. Then, the solution to equation (6.8) is

u(x)=n=0cnx0.5+1.2n,u(x)=\sum_{n=0}^{\infty}c_{n}x^{-0.5+1.2n}, (6.9)

where coefficients are expressed as

cn\displaystyle c_{n} =\displaystyle= λcn11Γ(10.5+1.2n0.5)Γ(10.5+1.2n)=cn1λΓ(1.2n)Γ(0.5+1.2n)\displaystyle-\frac{-\lambda c_{n-1}^{1}\Gamma(1-0.5+1.2n-0.5)}{\Gamma(1-0.5+1.2n)}=c_{n-1}\frac{\lambda\Gamma(1.2n)}{\Gamma(-0.5+1.2n)}
=\displaystyle= c0λnj=0n1Γ(1.2+1.2n)Γ(1.7+1.2n)\displaystyle c_{0}\lambda^{n}\prod_{j=0}^{n-1}\frac{\Gamma(1.2+1.2n)}{\Gamma(1.7+1.2n)}

and the solution then is

u(x)\displaystyle u(x) =\displaystyle= c0n=0λnj=0n1Γ(1.2+1.2n)Γ(1.7+1.2n)x0.5+1.2n\displaystyle c_{0}\sum_{n=0}^{\infty}\lambda^{n}\prod_{j=0}^{n-1}\frac{\Gamma(1.2+1.2n)}{\Gamma(1.7+1.2n)}x^{-0.5+1.2n} (6.10)
=\displaystyle= c0x0.5n=0j=0n1Γ(1.2+1.2n)Γ(1.7+1.2n)λnx1.2n\displaystyle c_{0}x^{-0.5}\sum_{n=0}^{\infty}\prod_{j=0}^{n-1}\frac{\Gamma(1.2+1.2n)}{\Gamma(1.7+1.2n)}\lambda^{n}x^{1.2n}

If we apply the initial condition then we obtain

DR0.5u(0)=c0Γ(0.5)Γ(1)=c0Γ(0.5)=c0π.D_{R}^{-0.5}u(0)=c_{0}\frac{\Gamma(0.5)}{\Gamma(1)}=c_{0}\Gamma(0.5)=c_{0}\sqrt{\pi}.

Then, c0=bπc_{0}=\displaystyle\frac{b}{\sqrt{\pi}} and we arrive at solution

u(x)=bπx0.5n=0j=0n1Γ(1.2+1.2n)Γ(1.7+1.2n)λnx1.2n=bπx0.5E0.5,2.4,0.4[λx1.2],u(x)=\frac{b}{\sqrt{\pi}}x^{-0.5}\sum_{n=0}^{\infty}\prod_{j=0}^{n-1}\frac{\Gamma(1.2+1.2n)}{\Gamma(1.7+1.2n)}\lambda^{n}x^{1.2n}=\frac{b}{\sqrt{\pi}}x^{-0.5}E_{0.5,2.4,0.4}[\lambda x^{1.2}], (6.11)

where Eα,m,l(z)=k=0ckzkE_{\alpha,m,l}(z)=\displaystyle\sum_{k=0}^{\infty}c_{k}z^{k} with c0=1,ck=j=0k1Γ[α(jm+l)+1]Γ[α(jm+l+1)+1]c_{0}=1,c_{k}=\displaystyle\prod_{j=0}^{k-1}\frac{\Gamma[\alpha(jm+l)+1]}{\Gamma[\alpha(jm+l+1)+1]}. Eα,m,l(z)E_{\alpha,m,l}(z) is the generalized Mittag-Leffler function introduced by Kilbas and Saigo. Solution (6.11) matches the solution identified in [8] for this problem. ∎

7 Conclusions

The quasi-Bessel equations have terms like xα+pDαu(x)x^{\alpha+p}D^{\alpha}u(x) and extend further the multi-term fractional Bessel equations and cover an essentially broader class of equations. Now the powers of xx may avoid matching the order of corresponding fractional derivatives (except for the highest derivative), whereas such a match is usually required for the successful applications of integral Mellin transform. Particularly, the Cauchy-Euler and constant-coefficient equations are included in the class of quasi-Bessel equations.

If the deviating (shifting) parameters pp are non-negative and meet certain non-restrictive conditions, then we construct the existence theory for quasi-Bessel equations in the class of fractional series solutions. Also, we prove the uniqueness theorem for the initial value problem.

Several presented examples and computational experiments, including the examples for constant-coefficient equations, reaffirm the validity of our methodology.

The quasi-Bessel equations with p<0p<0 do not fit the presented theory and remain an open problem.

Acknowledgments

The authors would like to thank Professor L. Boyadjiev for drawing our attention to the fractional Bessel equation. Also, the authors are obliged to Professor Kiryakova for valuable recommendations.

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