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Article

Analysis of Hilfer Fractional Integro-Differential Equations with Almost Sectorial Operators

by
Kulandhaivel Karthikeyan
1,
Amar Debbouche
2,3,* and
Delfim F. M. Torres
3
1
Department of Mathematics, Centre for Research and Development, KPR Institute of Engineering and Technology, Coimbatore, Tamil Nadu 641407, India
2
Department of Mathematics, Guelma University, Guelma 24000, Algeria
3
Center for Research and Development in Mathematics and Applications (CIDMA), Department of Mathematics, University of Aveiro, 3810-193 Aveiro, Portugal
*
Author to whom correspondence should be addressed.
Submission received: 31 December 2020 / Revised: 22 February 2021 / Accepted: 4 March 2021 / Published: 8 March 2021
(This article belongs to the Special Issue 2020 Selected Papers from Fractal Fract’s Editorial Board Members)

Abstract

:
In this work, we investigate a class of nonlocal integro-differential equations involving Hilfer fractional derivatives and almost sectorial operators. We prove our results by applying Schauder’s fixed point technique. Moreover, we show the fundamental properties of the representation of the solution by discussing two cases related to the associated semigroup. For that, we consider compactness and noncompactness properties, respectively. Furthermore, an example is given to illustrate the obtained theory.

1. Introduction

We consider nonlocal integro-differential equations involving Hilfer fractional derivatives and almost sectorial operators:
D 0 + α , γ u ( t ) + A u ( t ) = g t , u ( t ) , 0 t k ( t , s ) f ( s , u ( s ) ) d s , t ( 0 , T ] = J ,
I 0 + ( 1 α ) ( 1 γ ) [ u ( t ) ] | t = 0 + h ( u ( t ) ) = u 0 ,
where D 0 + α , γ is the Hilfer fractional derivative of order α ( 0 , 1 ) and type γ [ 0 , 1 ] . We assume that A is an almost sectorial operator on a Banach space Y with norm · . Let f : J × Y Y , g : J × Y × Y Y and h : C ( J : Y ) Y to be given abstract functions to be specified later. For brevity, we take
B u ( t ) = 0 t k ( t , s ) f ( s , u ( s ) ) d s .
Over the last decades, mathematical modeling has been supported by the field of fractional calculus, with several successful results and fractional operators shown to be an excellent tool to describe the hereditary properties of various materials and processes. Recently, this combination has gained a large amount of importance, mainly because fractional differential equations have become powerful tools for the modeling of several complex phenomena in numerous seemingly diverse and widespread fields of science and engineering; see, for instance, the basic text books in [1,2,3,4] and recent research works in [5,6,7]. In fact, abrupt changes, such as shocks, harvesting, or natural disasters, may occur in the dynamics of evolving processes. These short-term perturbations are often treated in the form of impulses. Recently, in many published works, Hilfer fractional differential equations have received attention [8,9,10,11,12,13,14,15,16,17].
In [15], Jaiswal and Bahuguna studied equations of Hilfer fractional derivatives with almost sectorial operators in the abstract sense:
D 0 + λ , v u ( t ) + A u ( t ) = g ( t , u ( t ) ) , t ( 0 , T ] , I 0 + ( 1 λ ) ( 1 v ) u ( 0 ) = u 0 .
We also refer to the work in [8], where Ahmed et al. studied the question of the existence of nonlinear Hilfer fractional differential equations with controls. Sufficient conditions are also established, where the time fractional derivative is the Hilfer derivative. In [18], Zhang and Zhou studied fractional Cauchy problems with almost sectorial operators of the form
( L D 0 + q x ) ( t ) = A x ( t ) + f ( t , x ( t ) ) , for almost all t [ 0 , a ] , ( I 0 + ( 1 q ) x ) ( 0 ) = x 0 ,
where L D 0 + q is the Riemann–Liouville derivative of order q, I 0 + ( 1 q ) is the Riemann–Liouville integral of order 1 q , 0 < q < 1 , A is an almost sectorial operator on a complex Banach space, and f is a given function. Motivated by these results, here, we extend the previous available results of the literature to a class of Hilfer fractional integro-differential equations in which the closed operator is almost sectorial. Moreover, we also consider both compactness and noncompactness cases of the semigroup operator.
The paper is structured as follows. In Section 2, we present necessary information about the Hilfer derivative, almost sectorial operators, measures of non-compactness, mild solutions of Equations (1) and (2) and some useful definitions, results and lemmas. We discuss fundamental results for mild solutions to Equations (1) and (2) in Section 3. In Section 4, we prove the solvability question in two cases, when associated semigroups are compact and noncompact, respectively. An example is then given in Section 5 to illustrate our main results. We end with Section 6, which presents our conclusions.

2. Preliminaries

In this section, we recall the necessary theory that is used throughout the work in order to obtain new results.

2.1. Fractional Derivatives

We start with a short introduction of the main definitions in fractional calculus [13,19].
Definition 1.
The left-sided Riemann–Liouville fractional integral of order α > 0 with a lower limit a for a function h : [ a , + ) R is defined as
I a + α h ( t ) = 1 Γ ( α ) a t ( t s ) α 1 h ( s ) d s ,
provided the right hand side is defined almost everywhere (a.e.) on [ a , + ) .
Remark 1.
If a = 0 , then we write I 0 + α f ( t ) = ( g α * f ) ( t ) , where
g α ( t ) : = 1 Γ ( α ) t α 1 , t > 0 , 0 , t 0 ,
and, as usual, * denotes the convolution of functions. Note that lim α 0 + g α ( t ) = δ ( t ) with δ the delta Dirac function.
Definition 2.
The left-sided Riemann–Liouville fractional derivative of order α > 0 , n 1 α < n , n N , for a function h : [ a , + ) R , is defined by
L D a + α h ( t ) = 1 Γ ( n α ) d n d t n a t h ( s ) ( t s ) α + 1 n d s , t > a ,
provided the right hand side is defined a.e. on [ a , + ) .
Definition 3.
The left-sided Caputo’s fractional derivative of order α > 0 , n 1 < α < n , n N , for a function h : [ a , + ) R , is defined by
C D a + α h ( t ) = 1 Γ ( n α ) a t h ( n ) ( s ) ( t s ) α + 1 n d s = I a + n α h ( n ) ( t ) , t > a ,
provided the right hand side is defined a.e. on [ a , + ) .
Definition 4.
The left-sided Hilfer fractional derivative of order 0 < α < 1 and type γ [ 0 , 1 ] , of a function h : [ a , + ) R , is defined as
D a + α , γ h ( t ) = I a + ( 1 α ) γ D I a + ( 1 α ) ( 1 γ ) h ( t ) .
Remark 2.
(i) If γ = 0 , 0 < α < 1 and a = 0 , then the Hilfer fractional derivative corresponds to the classical Riemann–Liouville fractional derivative:
D 0 + α , 0 h ( t ) = d d t I 0 + 1 α h ( t ) = L D 0 + α h ( t ) .
(ii) If γ = 1 , 0 < α < 1 and a = 0 , then the Hilfer fractional derivative corresponds to the classical Caputo fractional derivative:
D 0 + α , 1 h ( t ) = I 0 + 1 α d d t h ( t ) = C D 0 + α h ( t ) .

2.2. Measure of Non-Compactness

The motivation to consider our problem can be found in [18,19]. Here, we generalize the results in [18,19]. Let L Y be bounded. The Hausdorff measure of non-compactness is considered as
Θ ( L ) = inf θ > 0 such that L j = 1 m B θ ( x j ) , where x j Y , m N
while the Kurtawoski measure of noncompactness Φ on a bounded set B Y is given by
Φ ( L ) = inf ϵ > 0 such that L j = 1 m M j and diam ( M j ) ϵ
with the following properties:
  • L 1 L 2 gives Θ ( L 1 ) Θ ( L 2 ) , where L 1 , L 2 are bounded subsets of Y ;
  • Θ ( L ) = 0 if and only if L is relatively compact in Y ;
  • Θ ( { z } L ) = Θ ( L ) for all z Y L Y ;
  • Θ ( L 1 L 2 ) max { Θ ( L 1 ) , Θ ( L 2 ) } ;
  • Θ ( L 1 + L 2 ) Θ ( L 1 ) + Θ ( L 2 ) ;
  • Θ ( r L ) | r | Θ ( L ) for r R .
Let M C ( I , Y ) and M ( r ) = υ ( r ) Y | υ M . One defines
0 t M ( r ) d r : = 0 t υ ( r ) d r | υ M , t J .
Proposition 1.
If M C ( J , Y ) is equicontinuous and bounded, then t Θ ( M ( t ) ) is continuous on I. Furthermore,
Θ ( M ) = max Θ ( M ( t ) ) , Θ 0 t υ ( r ) d r 0 t Θ ( υ ( r ) ) d r , for t I .
Proposition 2.
Let { υ n : J Y , n N } be Bochner integrable functions. This implies that υ n m ( t ) a.e. for n N and m L 1 ( I , R + ) . Then, ξ ( t ) = Θ { υ n ( t ) } n = 1 L 1 ( I , R + ) and satisfies
Θ 0 t υ n ( r ) d r : n N 2 0 t ξ ( r ) d r .
Proposition 3.
Let M be a bounded set. Then, for any θ > 0 , there exists a sequence { υ n } n = 1 M such that
Θ ( M ) 2 Θ { υ n } n = 1 + θ .

2.3. Almost Sectorial Operators

Let 0 < β < π and 1 < β < 0 . We define S β 0 : = { υ C { 0 } such that | arg υ | < β } and its closure by S β , such that S β = { υ C { 0 } with | arg υ | β } { 0 } .
Definition 5
(See [20]). For 1 < β < 0 and 0 < ω < π 2 , we define Θ ω β as the family of all closed and linear operators A : D ( A ) Y Y such that
  • σ ( A ) is contained in S ω ;
  • for all β ( ω , π ) there exists M β such that
    R ( z , A ) L ( Y ) M β | z | β ,
where R ( z , A ) = ( z I A ) 1 is the resolvent operator and A Θ ω β is said to be an almost sectorial operator on Y .
Proposition 4
(See [20]). Let A Θ ω β for 1 < β < 0 and 0 < ω < π 2 . Then the following properties hold:
  • Q ( t ) is analytic and d n d t n Q ( t ) = ( A n Q ( t ) ( t S π 2 0 ) ;
  • Q ( t + s ) = Q ( t ) Q ( s ) t , s S π 2 0 ;
  • Q ( t ) L ( Y ) C 0 t β 1 ( t > 0 ) , where C 0 = C 0 ( β ) > 0 is a constant;
  • if Q = { x Y : lim t 0 + Q ( t ) x = x } , then D ( A θ ) Q if θ > 1 + β ;
  • R ( r , A ) = 0 e r s Q ( s ) d s , r C with R e ( r ) > 0
We use the following Wright-type function [19]:
M α ( θ ) = n N ( θ ) n 1 Γ ( 1 α n ) ( n 1 ) ! , θ C .
For 1 < σ < , r > 0 , the following properties hold:
(A1)
M α ( θ ) 0 , t > 0 ;
(A2)
0 θ σ M α d θ = Γ ( 1 + σ ) Γ ( 1 + α σ ) ;
(A3)
0 α θ α + 1 e r θ M α ( 1 θ α ) d θ = e r α .
The characteristic operators { S α ( t ) } | t S π 2 w 0 and { T α ( t ) } | t S π 2 w 0 are defined by
S α ( t ) : = 0 M α ( θ ) Q ( t α θ ) d θ
and
T α ( t ) : = 0 α θ M α ( θ ) Q ( t α θ ) d θ .
Theorem 1
(See Theorem 4.6.1 of [19]). For each fixed t S π 2 ω 0 , S α ( t ) and T α ( t ) are bounded linear operators on Y . Moreover,
S α ( t ) C 1 t α ( 1 + β ) , T α ( t ) C 2 t α ( 1 + β ) , t > 0 ,
where C 1 and C 2 are constants dependent on α and β.
Theorem 2
(See [19]). The operators S α ( t ) and T α ( t ) are continuous in the uniform operator topology for t > 0 . For s > 0 , the continuity is uniform on [ s , ] .
Define Ω r ( J ) : = { y C ( J , Y ) | y r } . Our main results are proved in relation to the following hypotheses:
Hypothesis 1 (H1).
For t J , g ( t , · , · ) : Y × Y Y and f ( t , · ) : Y Y are continuous functions and, for each u C ( J , Y ) , g ( · , u , B u ) : J Y and f ( · , u ) : J Y are strongly measurable.
Hypothesis 2 (H2).
There exist functions   k 1 , k 2 L 1 ( J , R + ) satisfying g ( t , · , · ) k 1 ( t ) + k 2 ( t ) e δ t for all u Ω r ( J ) and almost all t on J and
I 0 + α β [ k 1 ( t ) + k 2 ( t ) e δ t ] C ( J , R ) , lim t 0 + t ( 1 + α β ) ( 1 γ ) I 0 + α β [ k 1 ( t ) + k 2 ( t ) e δ t ] = 0 .
Hypothesis 3 (H3).
Function h : C ( J , Y ) Y is completely continuous and there exists a positive constant k such that h ( u ) k .
Hypothesis 4 (H4).
We assume that
sup [ 0 , T ] ( t ( 1 + α β ) ( 1 γ ) S α , γ ( t ) [ u 0 + k ] + t ( 1 + α β ) ( 1 γ ) 0 t ( t r ) α β 1 [ k 1 ( r ) + k 2 ( r ) e δ r ] d r ) r ,
for r > 0 , u 0 D ( A θ ) , and θ > 1 + β , where S α , γ ( t ) = I 0 + γ ( 1 α ) t α 1 T α ( t ) .
For the next two lemmas, we refer to [9,12].
Lemma 1
(See [9,12]). The fractional Cauchy problem (1)–(2) is equivalent to the integral equation
u ( t ) = [ u 0 h ( u ( t ) ) ] Γ ( γ ( 1 α ) + α ) t ( 1 α ) ( γ 1 ) + 1 Γ ( α ) 0 1 ( t r ) α 1 [ A u ( r ) + g ( r , u ( r ) , ( B u ) r ) ] d r , t J .
Lemma 2
(See [9,12]). If u is a solution to the integral Equation (3), then it satisfies
u ( t ) = S α , γ ( t ) [ u 0 h ( u ( t ) ) ] + 0 t R α ( t r ) g ( r , u ( r ) , ( B u ) r ) d r ,
where S α , γ ( t ) = I 0 + γ ( 1 α ) R α ( t ) with R α = t α 1 T α ( t ) .
Definition 6.
By a mild solution of the Cauchy problem in Equations (1) and (2), we mean a function u C ( J , Y ) that satisfies
u ( t ) = S α , γ ( t ) [ u 0 h ( u ( t ) ) ] + 0 t R α ( t r ) g ( r , u ( r ) , ( B u ) r ) d r , t J .
We define operator P : Ω r ( J ) Ω r ( J ) as
( P u ) ( t ) : = S α , γ ( t ) [ u 0 h ( u ( t ) ) ] + 0 t ( t r ) α 1 T α ( t r ) g ( r , u ( r ) , ( B u ) r ) d r .
Lemma 3
(See [15]). The operators R α ( t ) and S α , γ ( t ) are bounded linear operators on Y for every fixed t S π 2 ω 0 . Also, for t > 0 , we have
R α ( t ) x C 2 t 1 α β x , S α , γ ( t ) x Γ ( α β ) Γ ( γ ( 1 α ) α β ) C 2 t γ ( 1 α ) α β 1 x .
Proposition 5
(See [15]). The operators R α ( t ) and S α , γ ( t ) are strongly continuous for t > 0 .

3. Auxiliary Results

Below, we present our original contributions.
Theorem 3.
Let A Θ ω β for 1 < β < 0 and 0 < ω < π 2 . Assuming that ( H 1 ) ( H 4 ) are satisfied, then the operator { P y : y Ω r ( J ) } is equicontinuous, provided u 0 D ( A θ ) with θ > 1 + β .
Proof. 
For y Ω r ( J ) and t 1 = 0 < t 2 T , we have
P y ( t 2 ) P y ( 0 ) = t 2 ( 1 + α β ) ( 1 γ ) S α , γ ( t 2 ) [ u 0 h ( u ( t ) ) ] + 0 t 2 ( t 2 r ) α 1 T α ( t 2 r ) g ( r , u ( r ) , ( B u ) r ) d r t 2 ( 1 + α β ) ( 1 γ ) S α , γ ( t 2 ) ( u 0 + k ) + t 2 ( 1 + α β ) ( 1 γ ) 0 t 2 ( t 2 r ) α 1 T α ( t 2 r ) g ( r , u ( r ) , ( B u ) r ) d r 0 , as t 2 0 .
Now, let 0 < t 1 < t 2 T . One has
P y ( t 2 ) P y ( t 1 ) t 2 ( 1 + α β ) ( 1 γ ) S α , γ ( t 2 ) [ u 0 h ( u ( t ) ) ] t 1 ( 1 + α β ) 1 γ S α , γ ( t 1 ) [ u 0 h ( u ( t ) ) ] + t 2 ( 1 + α β ) ( 1 γ ) 0 t 2 ( t 2 r ) α 1 T α ( t 2 r ) g ( r , u ( r ) , ( B u ) r ) d r t 1 ( 1 + α β ) ( 1 γ ) 0 t 1 ( t 1 r ) α 1 T α ( t 1 r ) g ( r , u ( r ) , ( B u ) r ) d r .
Using the triangle inequality, we get
P y ( t 2 ) P y ( t 1 ) t 2 ( 1 + α β ) ( 1 γ ) S α , γ ( t 2 ) [ u 0 h ( u ( t ) ) ] t 1 ( 1 + α β ) ( 1 γ ) S α , γ ( t 1 ) [ u 0 h ( u ( t ) ) ] + t 2 ( 1 + α β ) ( 1 γ ) t 1 t 2 ( t 2 r ) α 1 T α ( t 2 r ) g ( r , u ( r ) , ( B u ) r ) d r + t 2 ( 1 + α β ) ( 1 γ ) 0 t 1 ( t 2 r ) α 1 T α ( t 2 r ) g ( r , u ( r ) , ( B u ) r ) d r t 1 ( 1 + α β ) ( 1 γ ) 0 t 1 ( t 1 r ) α 1 T α ( t 2 r ) g ( r , u ( r ) , ( B u ) r ) d r + t 1 ( 1 + α β ) ( 1 γ ) 0 t 1 ( t 1 r ) α 1 T α ( t 2 r ) g ( r , u ( r ) , ( B u ) r ) d r t 1 ( 1 + α β ) ( 1 γ ) 0 t 1 ( t 1 r ) α 1 T α ( t 1 r ) g ( r , u ( r ) , ( B u ) r ) d r = : I 1 + I 2 + I 3 + I 4 .
From the strong continuity of S α , γ ( t ) , we have I 1 0 as t 2 t 1 . Also,
I 2 C 2 t 2 ( 1 + α β ) ( 1 γ ) t 1 t 2 ( t 2 r ) α β 1 [ k 1 ( r ) + k 2 ( r ) e δ r ] d r C 2 | t 2 ( 1 + α β ) ( 1 γ ) 0 t 2 ( t 2 r ) α β 1 [ k 1 ( r ) + k 2 ( r ) e δ r ] d r t 2 ( 1 + α β ) ( 1 γ ) 0 t 1 ( t 1 r ) α β 1 [ k 1 ( r ) + k 2 ( r ) e δ r ] d r | C 2 0 t 1 | t 1 ( 1 + α β ) ( 1 γ ) ( t 1 r ) α β 1 t 2 ( 1 + α β ) ( 1 γ ) ( t 2 r ) α β 1 | [ k 1 ( r ) + k 2 ( r ) e δ r ] d r .
Then, by using (H2) and the dominated convergence theorem, I 2 0 as t 2 t 1 . Since
I 3 C 2 0 t 1 ( t 2 r ) α α β | t 2 ( 1 + α β ) ( 1 γ ) ( t 2 r ) α 1 t 1 ( 1 + α β ) ( 1 γ ) ( t 1 r ) α 1 | [ k 1 ( r ) + k 2 ( r ) e δ r ] d r ,
( t 2 r ) α α β | t 2 ( 1 + α β ) ( 1 γ ) ( t 2 r ) α 1 t 1 ( 1 + α β ) ( 1 γ ) ( t 1 r ) α 1 | [ k 1 ( r ) + k 2 ( r ) e δ r ] t 2 ( 1 + α β ) ( 1 γ ) ( t 2 r ) α 1 [ k 1 ( r ) + k 2 ( r ) e δ r ] + t 1 ( 1 + α β ) ( 1 γ ) ( t 1 r ) α 1 [ k 1 ( r ) + k 2 ( r ) e δ r ] 2 t 1 ( 1 + α β ) ( 1 γ ) ( t 1 r ) α 1 [ k 1 ( r ) + k 2 ( r ) e δ r ]
and 0 t 1 2 t 1 ( 1 + α β ) ( 1 γ ) ( t 1 r ) α 1 [ k 1 ( r ) + k 2 ( r ) e δ r ] d r exists, we obtain I 3 0 as t 2 t 1 . For ϵ > 0 , we have
I 4 = 0 t 1 t 1 ( 1 + α β ) ( 1 γ ) [ T α ( t 2 r ) T α ( t 1 r ) ] ( t 1 r ) α 1 g ( r , u ( r ) , ( B u ) r ) d r 0 t 1 ϵ t 1 ( 1 + α β ) ( 1 γ ) T α ( t 2 r ) T α ( t 1 r ) L ( Y ) ( t 1 r ) α 1 [ k 1 ( r ) + k 2 ( r ) e δ r ] + t 1 ϵ t 1 t 1 ( 1 + α β ) ( 1 γ ) T α ( t 2 r ) T α ( t 1 r ) L ( Y ) ( t 1 r ) α 1 [ k 1 ( r ) + k 2 ( r ) e δ r ] t 1 ( 1 + α β ) ( 1 γ ) 0 t 1 ( t 1 r ) α 1 [ k 1 ( r ) + k 2 ( r ) e δ r ] d r sup s [ 0 , t 1 ϵ ] T α ( t 2 r ) T α ( t 1 r ) L ( Y ) + C 2 t 1 ϵ t 1 t 1 ( 1 + α β ) ( 1 γ ) ( ( t 2 r ) α α β + ( t 1 r ) α α β ) ( t 1 r ) α 1 [ k 1 ( r ) + k 2 ( r ) e δ r ] d r t 1 ( 1 + α β ) ( 1 γ ) + α ( 1 + β ) 0 t 1 ( t 1 r ) α β 1 [ k 1 ( r ) + k 2 ( r ) e δ r ] d r sup s [ 0 , t 1 ϵ ] T α ( t 2 r ) T α ( t 1 r ) L ( Y ) + 2 C 2 t 1 ϵ t 1 t 1 ( 1 + α β ) ( 1 γ ) ( t 1 r ) α β 1 [ k 1 ( r ) + k 2 ( r ) e δ r ] d r .
Since T α ( t ) is uniformly continuous and lim t 2 t 1 I 2 = 0 , then I 4 0 as t 2 t 1 , independent of y Ω r ( J ) . Hence, P y ( t 2 ) P y ( t 1 ) 0 , independently of y Ω r ( J ) as t 2 t 1 . Therefore, { P y : y Ω r ( J ) } is equicontinuous. □
Theorem 4.
Let 1 < β < 0 , 0 < ω < π 2 , and A Θ ω β . Then, under Hypotheses (H1)–(H4), the operator { P y : y Ω r ( J ) } is continuous and bounded, provided u 0 D ( A θ ) with θ > 1 + β .
Proof. 
We verify that P maps Ω r ( J ) into itself. Taking y Ω r ( J ) and defining
u ( t ) : = t ( 1 + α β ) ( 1 γ ) y ( t ) ,
we have u Ω r ( J ) . Let t [ 0 , T ] ,
P t ( 1 + α β ) ( 1 γ ) S α , γ ( t ) [ u 0 h ( u ( t ) ) ] + t ( 1 + α β ) ( 1 γ ) 0 t ( t r ) α 1 T α ( t r ) g ( r , u ( r ) , ( B u ) r ) d r .
From (H2)–(H4), we get
P y ( t ) t ( 1 + α β ) ( 1 γ ) S α , γ ( t ) [ u 0 h ( u ( t ) ) ] + t ( 1 + α β ) ( 1 γ ) 0 t ( t r ) α β 1 [ k 1 ( r ) + k 2 ( r ) e δ r ] d r sup [ 0 , T ] t ( 1 + α β ) ( 1 γ ) S α , γ ( t ) [ u 0 + k ] + t ( 1 + α β ) ( 1 γ ) 0 t ( t r ) α β 1 [ k 1 ( r ) + k 2 ( r ) e δ r ] d r r .
Thus, P y r for any y Ω r ( J ) . Now, to verify P is continuous in Ω r ( J ) , let y n , y Ω r ( J ) , n = 1 , 2 , with lim n y n = y ; that is, lim n y n ( t ) = y ( t ) ; lim n t ( 1 + α β ) 1 γ y n ( t ) = t ( 1 + α β ) 1 γ y ( t ) and lim n t ( 1 + α β ) ( 1 γ ) y n ( t ) = t ( 1 + α β ) ( 1 γ ) y ( t ) on J . Then, (H1) implies that
g ( t , u n ( t ) , B ( u n ( t ) ) ) = g t , t ( 1 + α β ) ( 1 γ ) y n ( t ) , t ( 1 + α β ) ( 1 γ ) B ( y n ( t ) ) g t , t ( 1 + α β ) ( 1 γ ) y ( t ) , t ( 1 + α β ) ( 1 γ ) B ( y ( t ) )
as n . From (H2), we obtain the inequality
( t r ) α β 1 | g ( r , u n ( r ) , B ( u n ( r ) ) ) | 2 ( t r ) ( α β ) ( 1 γ ) [ k 1 ( r ) + k 2 ( r ) e δ r ] ,
that is,
0 t ( t r ) α β 1 g ( r , u n ( r ) , B ( u n ( r ) ) ) g ( r , u ( r ) , B ( u ( r ) ) d r 0 as n .
Let t [ 0 , T ] . Now,
P y n ( t ) P y ( t ) t ( 1 + α β ) ( 1 γ ) 0 t ( t r ) α 1 T α ( t r ) ( g ( r , u n ( r ) , B ( u n ( r ) ) g ( r , u ( r ) , B ( u ( r ) ) ) d r .
Applying Theorem 1, we have
P y n ( t ) P y ( t ) C 2 t ( 1 + α β ) ( 1 γ ) 0 t ( t r ) α β 1 g ( r , u n ( r ) , B ( u n ( r ) ) g ( r , u ( r ) , B ( u ( r ) ) d r ,
which tends to 0 as n , i.e., P y n P y pointwise on J . Moreover, Theorem 3 implies that P y n P y uniformly on J as n , that is, P is continuous. □

4. Main Results

We prove the existence of a mild solution to the problem in Equations (1) and (2) when the associated semigroup is compact (Theorem 5) and noncompact (Theorem 6).

4.1. Compactness of the Semigroup

Here, we assume Q ( t ) to be compact.
Theorem 5.
Let 1 < β < 0 , 0 < ω < π 2 and A Θ ω β . If Q ( t ) ( t > 0 ) is compact and (H1)–(H4) hold, then there exists a mild solution of (1)–(2) in Ω r ( J ) for every u 0 D ( A θ ) with θ > 1 + β .
Proof. 
Because we assume Q ( t ) to be compact, then the equicontinuity of Q ( t ) ( t > 0 ) is ensured. Moreover, by Theorems 3 and 4, P : Ω r ( J ) Ω r ( J ) is continuous and bounded and ε : Ω r ( J ) Ω r ( J ) is bounded and continuous, and { ε y : y Ω r ( J ) } is equicontinuous. We can write ϵ : Ω r ( J ) Ω r ( J ) by ( ϵ y ) ( t ) = ( ϵ 1 y ) ( t ) + ( ϵ 2 y ) ( t ) , where
( ϵ 1 y ) ( t ) = t ( 1 + α β ) ( 1 γ ) S α , γ ( t ) ( u 0 h ( u ) ) = t ( 1 + α β ) ( 1 γ ) I 0 + γ ( 1 α ) t α 1 T α ( t ) ( u 0 h ( u ) ) = t ( 1 + α β ) ( 1 γ ) Γ ( γ ( 1 α ) ) 0 t ( t r ) γ ( 1 α ) 1 r α 1 0 α θ M α ( θ ) Q ( r α θ ) ( u 0 h ( u ) ) d θ d r = α t ( 1 + α β ) ( 1 γ ) Γ ( γ ( 1 α ) ) 0 t 0 ( t r ) γ ( 1 α ) 1 r α 1 θ M α ( θ ) Q ( r α θ ) ( u 0 h ( u ) ) d θ d r
and
( ε 2 y ) ( t ) = t ( 1 + α β ) ( 1 γ ) 0 t ( t r ) α 1 T α ( t r ) g ( r , u ( r ) ( B u ) r ) d r .
For σ > 0 and θ ( 0 , t ) , we define an operator ε θ , σ 1 on Ω r ( J ) by
( ε θ , σ 1 y ) ( t ) = t ( 1 + α β ) ( 1 γ ) Γ ( γ ( 1 α ) ) θ t σ ( t r ) ( 1 α ) γ 1 r α 1 θ M α ( θ ) Q ( r α θ ) ( u 0 h ( u ) ) d θ d r = α t ( 1 + α β ) ( 1 γ ) Γ ( γ ( 1 α ) ) T ( θ α σ ) θ t σ ( t r ) ( 1 α ) γ 1 r α 1 θ M α ( θ ) Q ( r α θ θ α σ ) ( u 0 h ( u ) ) d θ d r .
Since T ( ϵ α δ ) is compact, V θ , σ 1 ( t ) = { ε θ , σ 1 y ) ( t ) , y Ω r ( J ) } is precompact in Y for all θ ( 0 , t ) and δ > 0 . Moreover, for any y Ω r ( J ) , one has
( ε 1 y ) ( t ) ( ε θ , σ 1 y ) ( t ) K ( α , γ ) t ( 1 + α β ) ( 1 γ ) 0 t 0 σ ( t r ) γ ( 1 α ) 1 r α 1 θ M α ( θ ) Q ( r α θ ) ( u 0 h ( u ) ) d θ d r + K ( α , γ ) t ( 1 + α β ) ( 1 γ ) 0 θ σ ( t r ) γ ( 1 α ) 1 r α 1 θ M α ( θ ) Q ( r α θ ) ( u 0 h ( u ) ) d θ d r K ( α , γ ) t ( 1 + α β ) ( 1 γ ) 0 t 0 σ ( t r ) γ ( 1 α ) 1 r α 1 θ M α ( θ ) r α γ α ( u 0 h ( u ) ) θ β 1 d θ d r + K ( α , γ ) t ( 1 + α β ) ( 1 γ ) 0 θ σ ( t r ) γ ( 1 α ) 1 r α 1 θ M α ( θ ) r α β α θ β 1 ( u 0 h ( u ) ) d θ d r = K ( α , γ ) t ( 1 + α β ) ( 1 γ ) 0 t ( t r ) γ ( 1 α ) 1 r α β 1 ( u 0 h ( u ) ) d r 0 σ θ β M α ( θ ) d θ + K ( α , γ ) t ( 1 + α β ) ( 1 γ ) 0 θ ( t r ) γ ( 1 α ) 1 r α β 1 ( u 0 h ( u ) ) d r η θ β M α ( θ ) d θ K t α γ ( 1 + β ) ( u 0 h ( u ) ) 0 η θ β M α ( θ ) d θ + K t α γ ( 1 + β ) [ u 0 + k ] 0 θ ( 1 s ) γ ( 1 α ) 1 r α β 1 d r η θ β M α ( θ ) d θ 0 as θ 0 and σ 0 ,
where K ( α , γ ) = α Γ ( γ ( 1 α ) ) . Therefore, V θ , σ 1 ( t ) = { ( ε θ , σ 1 y ) ( t ) , y Ω r ( J ) } are arbitrarily close to V 1 ( t ) = { ( ε 1 y ) ( t ) , y Ω r ( J ) } for t > 0 . Hence, V 1 ( t ) , for t > 0 , is precompact in Y . For θ ( 0 , t ) and σ > 0 , we can present an operator ε θ , σ 2 on Ω r ( J ) by
( ε θ , σ 2 y ) ( t ) = α t ( 1 + α β ) ( 1 γ ) 0 t θ σ θ M α ( θ ) ( t r ) α 1 Q ( ( t r ) α θ ) g ( r , u ( r ) , ( B u ) r ) d θ d r = α t ( 1 + α β ) ( 1 γ ) T ( θ α σ ) 0 t θ σ θ M α ( θ ) ( t r ) α 1 Q ( ( t r ) α θ θ α σ ) g ( r , u ( r ) , ( B u ) r ) d θ d r .
Thus, due to the compactness of Q ( θ α σ ) , V θ , σ 2 ( t ) = { ( ε θ , σ 2 y ) ( t ) , y Ω r ( J ) } is precompact in Y for all θ ( 0 , t ) and σ > 0 . For every y Ω r ( J ) , we get
( ε 2 y ) ( t ) ( ε θ , σ 2 y ) ( t ) α t ( 1 + α β ) ( 1 γ ) 0 t 0 σ θ M α ( θ ) ( t r ) α 1 Q ( ( t r ) α θ ) g ( r , u ( r ) , ( B u ) r ) d θ d r + α t ( 1 + α β ) ( 1 γ ) t θ t σ ( t r ) α 1 θ M α ( θ ) Q ( ( t r ) α θ ) g ( r , u ( r ) , ( B u ) r ) d θ d r α C 0 t ( 1 + α β ) ( 1 γ ) 0 t ( t r ) α β 1 [ k 1 ( r ) + k 2 ( r ) e δ r ] d r 0 σ θ β M α ( θ ) d θ + α C 0 t ( 1 + α β ) ( 1 γ ) t θ t ( t r ) α β 1 [ k 1 ( r ) + k 2 ( r ) e δ r ] d r 0 θ β M α ( θ ) d θ α C 0 t ( 1 + α β ) ( 1 γ ) 0 t ( t r ) α β 1 [ k 1 ( r ) + k 2 ( r ) e δ r ] d r 0 σ θ β M α ( θ ) d θ + α C 0 Γ ( 1 β ) Γ ( 1 α β ) t ( 1 + α β ) ( 1 γ ) t θ t ( t r ) α β 1 [ k 1 ( r ) + k 2 ( r ) e δ r ] d r 0 as σ 0 .
Therefore, V θ , σ 2 ( t ) = { ( ε θ , σ 2 y ) ( t ) , y Ω r ( J ) } are arbitrarily close to V 2 ( t ) = { ( ε 2 y ) ( t ) , y Ω r ( J ) } , t > 0 . This implies the relative compactness of V 2 ( t ) , t > 0 , in Y . Also, V ( t ) = { ( ε y ) ( t ) , y Ω r ( J ) } is relatively compact in Y t [ 0 , T ] . It follows, from the Arzela–Ascoli theorem, that { ε y , y Ω r ( J ) } is relatively compact for ε , it is continuous, and { ε y , y Ω r ( J ) } is relatively compact. This implies, by the Schauder fixed point theorem, the existence of a fixed point y * Ω r ( J ) of ε . Let u * ( t ) : = t ( 1 + α β ) ( γ 1 ) y * ( t ) . Then, u * is a mild solution of Equations (1) and (2). □

4.2. Non-Compactness of the Semigroup

Now, we assume that Q ( t ) is noncompact. We need the following supplementary condition:
Hypothesis 5. (H5)
There exists a constant k > 0 satisfying
Θ ( g ( t , E 1 , E 2 ) ) k Θ ( E 1 , E 2 ) for almost all t [ 0 , T ]
and for every bounded subsets E 1 , E 2 Y .
Theorem 6.
Let 1 < β < 0 , 0 < ω < π 2 , and A Θ ω β . Suppose (H1)–(H5) hold. Then, problem (1)–(2) has a mild solution in Ω r ( J ) for every u 0 D ( g θ ) with θ > 1 + β .
Proof. 
From Theorems 3 and 4, we find that ε : Ω r ( J ) Ω r ( J ) is continuous and bounded, and { ε y : y Ω r ( J ) } is equicontinuous. Furthermore, we prove that there is a subset of Ω r ( J ) such that ε is compact in it. For any bounded set P 0 Ω r ( J ) , set
ε ( 1 ) ( P 0 ) = ε ( P 0 ) , ε ( n ) ( P 0 ) = ε ( c o ¯ ( ε ( n 1 ) ( P 0 ) ) ) , n = 2 , 3 ,
For any ϵ > 0 , we can obtain from Propositions 1–3 a subsequence { y n ( 1 ) } n = 1 P 0 satisfying
Θ ( ε ( 1 ) ( P 0 ( t ) ) ) 2 Θ t ( 1 + α β ) ( 1 γ ) 0 t ( t r ) α 1 T α ( t r ) g ( r , { r ( 1 + α β ) ( 1 γ ) ( y n ( 1 ) ( r ) , B y n ( 1 ) ( r ) ) } n = 1 ) d r 4 C p t ( 1 + α β ) ( 1 γ ) 0 t ( t r ) α β 1 Θ ( g ( r , { r ( 1 + α β ) ( 1 γ ) ( y n ( 1 ) ( r ) , B y n ( 1 ) ( r ) ) } n = 1 ) ) d r 4 C p k t ( 1 + α β ) ( 1 γ ) Θ ( P 0 ) 0 t ( t r ) α β 1 r ( 1 + α β ) ( 1 γ ) d r = 4 C p k t α β Θ ( P 0 ) Γ ( α β ) Γ ( ( α β + γ ( 1 + α β ) ) Γ ( 2 α β + γ ( 1 + α β ) ) .
Since ϵ is arbitrary, then
Θ ( ε ( 1 ) ( P 0 ( t ) ) ) 4 C p k t α β Θ ( P 0 ) Γ ( α β ) Γ ( ( α β + γ ( 1 + α β ) ) Γ ( 2 α β + γ ( 1 + α β ) ) .
Again, for any ϵ > 0 , we can get from Propositions 1–3 a subsequence { y n ( 2 ) , B y n ( 2 ) } n = 1 c o ¯ ( ε ( 1 ) ( P 0 ) ) , which implies that
Θ ( ε ( 2 ) ( P 0 ( t ) ) ) = Θ ( ε ( c o ¯ ( ε ( 1 ) ( P 0 ( t ) ) ) ) ) 2 Θ t ( 1 + α β ) ( 1 γ ) 0 t ( t r ) α 1 Q α ( t r ) g ( r , { r ( 1 + α β ) ( 1 γ ) ( y n ( 2 ) ( r ) , B y n ( 2 ) ( r ) ) } n = 1 ) d r 4 C p t ( 1 + α β ) ( 1 γ ) 0 t ( t r ) α β 1 Θ ( g ( r , { r ( 1 + α β ) ( 1 γ ) ( y n ( 2 ) ( r ) , B y n ( 2 ) ( r ) ) } n = 1 ) d r 4 C p k t ( 1 + α β ) ( 1 γ ) 0 t ( t r ) α β 1 Θ ( r ( 1 + α β ) ( 1 γ ) ( { y n ( 2 ) ( r ) , B y n ( 2 ) ( r ) } n = 1 ) ) d r 4 C p k t ( 1 + α β ) ( 1 γ ) 0 t ( t r ) α β 1 r ( 1 + α β ) ( 1 γ ) Θ ( { y n ( 2 ) ( r ) , B y n ( 2 ) } n = 1 ) d r ( 4 C p k ) 2 t ( 1 + α β ) ( 1 γ ) Γ ( α β ) Γ ( α β + γ ( 1 + α β ) ) Γ ( 2 α β + γ ( 1 + α β ) ) Θ ( P 0 ) × 0 t ( t r ) α β 1 r ( 1 + α β ) ( 1 γ ) α β d r = ( 4 C p k ) 2 t 2 α β Γ 2 ( α β ) Γ ( α β + γ ( 1 + α β ) ) Γ ( 3 α β + γ ( 1 + α β ) ) Θ ( P 0 ) .
Now,
Θ ( ε ( n ) ( P 0 ( t ) ) ) ( 4 C p k ) n t n α β Γ n ( α β ) Γ ( α β + γ ( 1 + α β ) ) Γ ( ( n + 1 ) α β + γ ( 1 + α β ) ) Θ ( P 0 ) , n N .
Let M = 4 C p k T α β Γ ( α β ) . We can find m , k N large enough such that 1 k < α β < 1 k 1 and n + 1 k > 2 for n > m Γ ( ( n + 1 ) α β + γ ( 1 + α β ) ) > Γ ( n + 1 k ) , that is,
( 4 C p k ) n T n α β Γ n ( α β ) Γ ( α β + γ ( 1 + α β ) ) Γ ( ( n + 1 ) α β + γ ( 1 + α β ) ) < ( 4 C p k ) n T n α β Γ n ( α β ) Γ ( α β + γ ( 1 + α β ) ) Γ n + 1 k .
Replacing ( n + 1 ) by ( j + 1 ) k , then the right-hand side of the inequality given above becomes
M ( j + 1 ) k 1 Γ ( α β + γ ( 1 + α β ) ) Γ ( j + 1 ) = ( M k ) j M k 1 Γ ( α β + γ ( 1 + α β ) ) j ! 0 as j .
Therefore, there exists a constant n 0 N such that
( 4 C p k n t n α β Γ n ( α β ) Γ ( α β + γ ( 1 + α β ) Γ ( ( n + 1 ) α β + γ ( 1 + α β ) ) ( 4 C p k ) n 0 T n 0 α β Γ n 0 ( α β ) Γ ( α β + γ ( 1 + α β ) ) Γ ( ( n 0 + 1 ) α β + γ ( 1 + α β ) ) = p < 1 .
Now, Θ ( ε ( n 0 ) ( P 0 ( t ) ) ) p Θ ( P 0 ) . Since ε ( n 0 ) ( P 0 ( t ) ) is bounded and equicontinuous, it follows from Proposition 1 that
Θ ( ε ( n 0 ) ( P 0 ) ) = max t [ 0 , T ] Θ ( ε n 0 ( P 0 ( t ) ) ) .
Thus, Θ ( ε n 0 ( P 0 ) ) p Θ ( P 0 ) , where p < 1 . Using a similar technique as in Theorem 5, we obtain C in Ω r ( J ) with ε ( C ) C and ε ( C ) compact. By applying Schauder’s fixed point theorem, we obtain a fixed point y * in Ω r ( J ) of ε . Let u * ( t ) = t ( 1 + α β ) ( γ 1 ) y * ( t ) . Then, u * ( t ) is a mild solution of problem (1)–(2). □

5. Example

As an illustrative example, let us consider the following Hilfer fractional partial differential equation with a nonlocal condition:
D 0 + 3 4 , 1 2 z ( t , y ) + x 2 z ( t , y ) = G ( t , z ( t , y ) , B z ( t , y ) ) , t ( 0 , 1 ] , y [ 0 , π ] , z ( t , 0 ) = z ( t , π ) = 0 , t ( 0 , 1 ] , I 0 + 1 8 [ z ( t , y ) ] | t = 0 + i = 1 m c i z ( t i , y ) = z 0 ( y ) , y [ 0 , π ] ,
where α = 3 4 , γ = 1 2 , 0 < t 1 < < t m < 1 , and c i , i = 1 , , m , are given constants. Let us take the nonlinear function G ( t , z ( · ) , B z ( · ) ) = y cos z ( t , y ) + 0 t e ( t s ) sin z ( t , y ) d s and the nonlocal function h ( z ( t , · ) ) = i = 1 m c i z ( t k , · ) . Assume that Y = L 2 [ 0 , π ] and define A : D ( A ) Y Y by A z = z y y with domain
D ( A ) = z Y : z y , z y y Y , z ( t , 0 ) = z ( t , π ) = 0 .
It follows from the work in [20] that there exist constants δ , ϵ > 0 such that A + δ π 2 ϵ π 2 1 ( Y ) . It is known that A is the infinitesimal generator of a differentiable semigroup Q ( t ) ( t > 0 ) in Y given by
( Q ( t ) x ) ( y ) = 0 π ψ ( t , y s ) x ( s ) d s , t > 0 , x ( y ) , t = 0 ,
where
ψ ( t , y ) = 1 4 π t e y 2 4 t , t > 0 , 0 < y < π ,
and x ( t ) ( y ) = z ( t , y ) . This implies Q ( t ) 1 and leads to its compactness property. We can check that all hypotheses (H1)–(H4) are fulfilled; thus, our Theorem 5 can be applied ensuring that problem (4) admits a mild solution.

6. Conclusions

In this paper, we applied Schauder’s fixed point theorem to investigate the solvability of a class of Hilfer fractional integro-differential equations involving almost sectorial operators. We discussed cases of both compactness and noncompactness related to associated semigroup operators. The obtained existence results were subject to an appropriate set of sufficient conditions. As a future direction of research, it would be desirable to consider the study of ψ -Hilfer fractional nonlocal nonlinear stochastic systems involving almost sectorial operators and impulsive effects, generalizing the current work. Another open line of research consists of the development of numerical methods to approximate the mild solutions predicted by Theorems 5 and 6.

Author Contributions

Conceptualization, A.D.; methodology, D.F.M.T.; validation, A.D.; formal analysis, D.F.M.T.; investigation, D.F.M.T.; writing—original draft preparation, K.K.; writing—review and editing, A.D. and D.F.M.T.; supervision, A.D.; project administration, D.F.M.T. All authors have read and agreed to the published version of the manuscript.

Funding

Amar Debbouche and Delfim F. M. Torres were supported by FCT within the project UIDB/04106/2020 (CIDMA).

Conflicts of Interest

The authors declare no conflict of interest. The funder had no role in the design of the study; in the collection, analyses, or interpretation of data; in the writing of the manuscript, or in the decision to publish the results.

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Karthikeyan, K.; Debbouche, A.; Torres, D.F.M. Analysis of Hilfer Fractional Integro-Differential Equations with Almost Sectorial Operators. Fractal Fract. 2021, 5, 22. https://0-doi-org.brum.beds.ac.uk/10.3390/fractalfract5010022

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Karthikeyan K, Debbouche A, Torres DFM. Analysis of Hilfer Fractional Integro-Differential Equations with Almost Sectorial Operators. Fractal and Fractional. 2021; 5(1):22. https://0-doi-org.brum.beds.ac.uk/10.3390/fractalfract5010022

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Karthikeyan, Kulandhaivel, Amar Debbouche, and Delfim F. M. Torres. 2021. "Analysis of Hilfer Fractional Integro-Differential Equations with Almost Sectorial Operators" Fractal and Fractional 5, no. 1: 22. https://0-doi-org.brum.beds.ac.uk/10.3390/fractalfract5010022

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