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A Riesz-Medvedev Stieltjes Integral Method and Nearness Principle for Solvability of Fractional Integral Equations

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15 September 2025

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19 September 2025

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Abstract
A Riesz-Medvedev type of total variation method is employed to study solvabil- 1 ity of quadratic Voltera-Stieltjes integral equations. This solvability method is then shown 2 to be an invaluable approach to the solvability of a very general class of fractional dynamic 3 problems and other singular integral equations. We have given several illustrative exam- 4 ples to coroborate known solvabilty cases for particular fractional and singular integral 5 equations in literature.
Keywords: 
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1. Introduction

In this paper we present, below, solvability results for quadratic type Volterra-Stieltjes integral equations with applications to a very general class of fractional dynamic problems and various singular problems taking the general form.
u ( t ) = h ( t ) + f ( t , u ( t ) ) 0 t k ( t , s ) g ( s , u ( s ) ) d s Φ ( t , s ) ; t [ 0 , 1 ] .
In this presentation, we are particularly motivated by the newer approach reported in a series of publications [10,11,13,14] by Banas and his followers using the properties of the classical total variation functions. We recall, in 2011, Jozef Banas and Tomasz Zajac [10] presented a new approach to the investigation of functional equations of Volterra-Stieltjes type integral equations of fractional integral order. In particular, they initiated a very natural solvability formulation for functional integral equation of Volterra-Stieljes type, subject to existence of solution r 0 to the two auxiliary inequalities below:
h + K ( k F 1 ) Φ ( r ) r ; and k K Φ ( r ) < 1 .
In the same year, Banas and Rzepka [11] published another set of enlightening results for the solvability of the more general formulation below:
u ( t ) = h ( t , u ( t ) ) , u ( a ( t ) ) + ( G u ) ( t ) 0 t k ( t , s ) ν ( t , s ) g ( u ( s ) ) d s ;
subject to solvabilty requirement on a more complicated auxiliary inequalities. viz the solvability requirement that the following auxiliary inequalities,
η 1 r + h ¯ + k ¯ ν ¯ φ ( r ) ψ ( r ) r ;
has a solution r 0 which satisfies
η 1 + k ¯ ν ¯ η 2 ψ ( r 0 ) < 1 .
The aim of this paper is to employ the more general Riesz-Medvedev type of total variation and the principle of nearness of superposition operators to modify this new approach to obtain a more natural and more relaxed but similar constraint on solvability results which yield invaluable applications to fractional dynamics problems. The quadratic fractional integral equations we study herein are the form below:
u ( t ) = h ( t ) + f ( t , u ( t ) ) Γ ( α ) 0 t k ( t , s ) ( t s ) 1 α g ( s , u ( s ) ) d s ; t [ 0 , 1 ] .
Though our method is newer and more natural, equations (6) are special cases of (3) investigated by Banas Rzepka [11] which constitutes generalizations and extensions of problems studied in literature [12,28,33] under the broad class called quadratic integral equations which includes a wide class of singular integral equations as special cases. The class of quadratic integral equations are mostly used to formulate models describing numerous events and problems of real world problems like the theory of radiative transfer [17,18,20], the kinetic theory of gases [29], the theory of neutron transfer [17,20] and the theory of vehicular traffic [6,12]. The Chandrasekhar [20] type quadratic integral equations are special cases of such problems often encountered in models formulations for neutron transport theory and vehicular traffic theory [4,6,12,22,33,37].
It should be noted that solvability requirement for the pair of auxiliary inequalities in (36) is an inevitable constraint (inherent in applications of Darbo fixed point theorem) on the hypotheses for existence of solution of associated equations like (3). It is also important to highlight that the inequalities in (36) are more complicated than the inequalities in (2) because the associated integral equation is less complicated than the integral equation (3). Apart from these complications, the inequalities further impose smallness constraints on the data h , f , k , and g of the integral equations. But the novelty of our presentation includes relaxation of these smallness constraints on these data by allowing for alternations of smallness among the data in our formulation herein. In particular, it is only the Young function Φ ( t , s ) that is affected by smallness constraints in our presentation.
Under similar constraints by sets of auxiliary inequalities, various authors have attempted improvements in order to relax the requirement of solvability of complicated auxiliary inequalities (2) and (5). In this direction, we mention the following recent contributions: Benkerouche [15], Darwish [22,23,24]. El-Sayed et al [26], Zhou et al [38], Cicho [21], Danville [25], Kelley [28] and various others [1,2] and the references therein.

2. Preliminaries

Our methodology requires applications of the following classical results.
Definition 1. 
[31,37] Let Ω denote a compact metric space and Z ( Ω ) denote a class of functions f : Ω × R R . The function f ( t , x ) is said to generate a superposition operator F : Z 1 ( Ω ) Z 2 ( Ω ) if for each x Z 1 ( Ω ) there corresponds a function y Z 2 ( Ω ) such that
( F x ) ( t ) = y ( t ) = f ( t , x ( t ) ) i . e . F ( x ) = y Z 2 ( Ω ) , x Z 1 ( Ω )
The theory of superposition operators ( F x ) ( t ) = f ( t , x ( t ) ) often called Nemytskii operators (or outer composition operators or substitution operators) still has many open problems [3,35] which are extension of the basic basic problem in the theory of superposition operators. The basic problem of superposition operators concerned with formulations of conditions (called defining conditions) to guarantee validity of definition of a superposition operator F : Z 1 ( Ω ) Z 2 ( Ω ) between any given pair of function spaces Z 1 ( Ω ) and Z 2 ( Ω ) . But this theory for superposition operators F : C [ 0 , 1 ] C [ 0 , 1 ] on the space of continuous functions on a bounded closed interval [ a , b ] has been well established [3,31].
In the space C [ 0 , 1 ] of continuous functions defined on the unit interval [ 0 , 1 ] we have the following important properties;
Theorem 1. 
[3] The superposition operator F : Ω [ 0 , 1 ] generated by a function f : Ω × R R maps the space C [ 0 , 1 ] of continuous functions into itself if and only if f ( t , x ) is continuous on Ω × R where Ω denotes the derived set of Ω (i.e. Ω is the set of all limit points of Ω i.e.
F ( Ω ) C ( Ω ) iff f : Ω × R R
is continuous.
Observe that theorem 1 implies continuity of f ( . , u ) on Ω u R .
Theorem 2. 
[3] Suppose that the superposition F : C ( Ω ) C ( Ω ) generated by f ( t , x ) maps C ( Ω ) into itself. Then F is bounded if and only if f ( x , . ) is bounded t Ω Ω where Ω denotes the derived set of Ω .
Theorem 3. 
Suppose F : C [ 0 , 1 ] C [ 0 , 1 ] is a superposition operator F ( u ) = generated by f : [ 0 , 1 ] × R R . Then the following condonations are equivalent:
(a)
There exists a superposition operator G : B r ( C [ 0 , 1 ] ) B k ( r ) ( C ( 0 , 1 ) ) generated by a function g : [ 0 , 1 ] × R R such that | f ( t , x ) f ( t , y ) | g ( t , z ) | x y | where, z = max | x | , | y | .
(b)
The superposition operator F ( u ) = f ( t , u ) satisfies the Lipschitz condition | F ( x ) F ( y ) | k ( r ) | x y |
(c)
The superposition operator F ( u ) = f ( t , u ) satisfies the Darbo condition H C ( F ( Ω ) ) k ( r ) H C ( Ω ) ; for all Ω B r ( C [ 0 , 1 ] ) , where H C denotes the Hausdorff measure of no compactness in C [ 0 , 1 ] .
Theorem 4 
(cf [5]). A function φ ( t , s ) is a convex function if, and only if, Φ ( t , s ) has monotonically increasing one-sided partial derivative φ ( t , s ) = Φ ( t , s ) s with respect to s.
Corollary 1 
(cf [5]). Let f ( x ) be a twice differentiable function. Then f ( x ) is convex if, and only if, f ( x ) 0 for all x of our interval.
Definition 2. 
A continuous function Φ : [ 0 , ) [ 0 , ) is called a young function if
(i)
Φ ( 0 ) = 0
(ii)
Φ ( t ) > 0 t > 0
(iii)
lim t Φ ( t ) =
A Young function is often called a gauge function.
Definition 3. 
Given a Young function Φ : [ 0 , ) [ 0 , ) , and a partition P = { t 0 , t 1 , , t n } P ( [ 0 , 1 ] ) and a function f : [ 0 , 1 ] R , the Wiener-Young variation v a r Φ W ( f , P ) = j = i Φ ( | f ( t j ) f ( t t 1 ) | ) .
Definition 4. 
Given a Young function Φ, a partition P = { t 0 , t 1 , t 2 , , t n } of [ 0 , 1 ] and a function f : [ 0 , 1 ] R . The Riesz-Medvedev variation of f on [ 0 , 1 ] with respect to a partition P is defined by
v a r Φ R ( f ) = j = 1 n Φ | f ( t j ) f ( t j 1 ) | t j t j 1 · ( t j t j 1 )
Observe that the Riesz-Medvedev variation with respect to a partition P is the Wiener-Young variation if Φ ( | f ( t j ) f ( t j 1 ) ) is replaced with | f ( t j ) f ( t j 1 ) | t j t j 1 · ( t j t j 1 ) .
Definition 5. 
The Riesz-Medvedev total variation of f on [ 0 , 1 ] is given as sup { u Φ R ( f , P ) : P P ( [ 0 , 1 ] ) } where P ( [ 0 , 1 ] ) denotes the set of all possible finite partitions P of [ 0 , 1 ] .
Example 1. 
Let 0 s t 1 . Then the function Φ ( t , s ) = t α ( t s ) α α is of bounded Riesz-Medvedev total variation.
We recall [36] a mapping A : X E of a subset X of a Banach space E is said to be near a mapping B : X E if there exist two constants λ > 0 and η 2 [ 0 , 1 ) such that the following property holds:
( B u B v ) λ ( A u A v ) η 2 B u B v
It follows from (8) that when B is the identity mapping i.e. B = I then A is said to be near identity mapping I. Our investigation is limited to the property of nearness of A to identity mapping given below:
( u v ) λ ( A u A v ) η 2 u v
The nearness principle [16,34] follows from the following generalization of Neuman’s lemma by Campanato
Theorem 5. 
[16,19] Let E be a real Banach space. T : E E a nonlinear mapping such that there exist λ > 0 and η 2 [ 0 , 1 ) and
( u v ) λ ( T u T v ) η 2 u v then L i p ( I λ A ) η 2 and L i p ( A 1 ) λ 1 c
Where L i p ( T ) is the Lipchitz norm of T.
Our solvability procedure is based on application of Rothe fixed point theorem below to prove existence and uniqueness of the quadratic integral equations studied herein.
Theorem 6. 
[27,32] Let E be a Banach space, X a closed unit ball in E with boundary X . Let T be a countable compact mapping of X into E such that T ( X ) X , then T has a fixed point.

Main Result

Proposition 1. 
Let ν ( s ) be right differentiable increasing function such that ν ( s ) > 0 s > 0 . Then any composition function which is convex in s is of bounded Riesz-Medvedev variation.
Proof. 
Given a differentiable increasing functions φ ( s ) with φ ( s ) > 0 s > 0 , a composition function ( Φ φ ) ( s ) which is convex in s. We are to prove that the Riesz-Medvedev variation
V Φ R ( ν , P ) = j = 1 n Φ ν ( s j ) ν ( s j 1 ) s j s j 1 ( s j s j 1 ) = j = 1 n Φ ( ν ( c j ) ) ( s j s j 1 )
sup V Φ R ( ν , P ) = sup P P ( [ 0 , 1 ] ) j = 1 n Φ ( ν ( c j ) ) ( s j s j 1 ) = sup c j ν ( 0 , 1 ) Φ ( ν ( c j ) ) j = 1 n ( s j s j 1 ) = sup c j ν ( 0 , 1 ) ν ( c j ) ( t 0 0 ) <
Corollary 2. 
Let Φ ( t , s ) = t α ( t s ) α Then the total Riesz-Medvedev variation v s t 0 a r Φ R ( ν ) of the function ν ( t s ) = ( t s ) α satisfies
lim t 0 0 v s t 0 a r Φ R ( ν ( t , s ) ) = 0
Example 2. 
For all t 0 ( 0 , 1 ) , the function ν ( s ) = ( t s ) α is of bounded Riesz-Medvedev bounded variation.
PROOF
The function ν ( s ) = ( t s ) α is an increasing function of s with ν ( t , s ) s > 0 s ( 0 , 1 ) . Let ( Φ ν ) ( s ) be a positive increasing function of s. Then we have
Φ ( t s j ) α + ( t s j 1 ) α s j s j 1 = Φ ( t s j 1 ) α ( t s j ) α s j s j 1 = Φ 1 ( t c j ) 1 α · ( t s j 1 ) ( t s j ) s j s j 1 = Φ 1 ( t c j ) 1 α
for some c j ( t s j 1 , t s j )
j = 1 n Φ ν ( s j ) ν ( s j 1 ) s j s j 1 ( s j s j 1 ) = j = 1 n s j s j 1 ( t c j ) 1 α
sup P P ( [ 0 , 1 ] ) ν ( s j ) ν ( s j 1 ) s j s j 1 ( s j s j 1 ) = sup c j t o ( t c j ) 1 α < 0
In what follows, we shall investigate solvability of the quadratic integral equation () shown below
u ( t ) = h ( t ) + f ( t , u ( t ) ) 0 t k ( t , s ) g ( s , u ( s ) ) d s Φ ( t , s ) ;
subject to under-listed hypotheses on its data; viz - the functions h ( t ) , k ( s , t ) , Φ ( t , s ) and the superposition operators ( F u ) ( t ) = f ( t , u ) and ( G u ) ( t ) = g ( t , u ) :
H1
h C [ 0 , 1 ]
H2
f : [ 0 , 1 ] × R R satisfies the Lipschitz condition in its second variable with Lipschitz constant η 1 ie;
| f ( t , u 1 ) f ( t , u 2 ) | η 1 | u 1 u 2 |
H3
k : Δ R is continuous on the triangle Δ = { ( t , s ) [ 0 , 1 ] : 0 s t 1 }
H4
The nonlinearities f , g : [ 0 , 1 ] × R R generates the superposition operators F , G : C [ 0 , 1 ] C [ 0 , 1 ] respectively; i.e ( F u ) ( t ) = f ( t , u ( t ) ) and ( G u ) ( t ) = g ( t , u ( t ) )
H5
The superposition operator G ( u ) satisfies the following nearness condition with nearness constant η 2 , with respect to the identity operator I i.e; there exists η 2 ( 0 , 1 ) s.t
| ( u 1 ( t ) u 2 ( t ) ) [ ( G u 1 ) ( t ) ( G u 2 ) ( t ) ] | η 2 | u 1 ( t ) u 2 ( t ) |
H6
The function Φ ( t , s ) = Φ : Δ R is a Young’s function with respect to the second variable s and its one-sided partial derivative with respect to s is denoted by
d Φ ( t , s ) d s = φ ( t , s ) = Φ ( t , s ) s
To resolve existence issues for the quadratic integral equation (), we need to solve the corresponding linear equation (10) below. After which, we will employ variation of parameter method involving the linear part and the nonlinearity to resolve the nonlinear problem.
Theorem 7. 
Let the data h ( t ) , f ( u , t ) and Φ ( t , s ) of the quadratic integral equation
u ( t ) = h ( t ) + f ( t , u ) o t k ( t , s ) g ( u ( s ) ) d s Φ ( t , s )
satisfy the properties ( H 1 ) , ( H 2 ) , ( H 4 ) , ( H 4 ) and ( H 6 ) . Let t 0 ( 0 , 1 ) be such that the following condition holds:
η 1 k ¯ Φ 0 h < ( 1 f ¯ h ¯ k ¯ Φ 0 ) 2 where :
f ¯ = sup ( t , s ) [ 0 , t 0 ] × [ 0 , t 0 ] f ( t , s ) ;
k ¯ = sup ( t , s ) Δ 0 k ( t , s ) .
Φ 0 = sup ( t , s ) Δ 0 Φ ( t , s ) ; ;
Δ 0 = { ( t , s ) [ 0 , t 0 ] × [ 0 , t 0 ] : 0 s t 0 < 1 } .
Then the integral equation (10) has a unique solution z C [ 0 , t 0 ] .
PROOF
Let B r be a ball centered at the origin with radius r, We are to determine a value r 0 for r such that a mapping T : B r 0 C ( [ 0 , 1 ] ) satisfies the requirements of Theorem 6 of Rothe; where the mapping T is defined by
T z = h ( t ) + f ( t , z ) 0 t z ( s ) d s Φ ( t , s ) .
Clearly,
| ( T z ) ( t ) | | h ( t ) | + | f ( t , z ( t ) ) | 0 t | k ( t , s ) | | z ( s ) | d s Φ ( t , s )
Hence,
T z h + f ¯ k ¯ Φ 0 z .
This leads to an auxiliary inequality below:
h + f ¯ k ¯ Φ 0 z r .
For z B r ( h ) the inequality (16) becomes the following:
h ¯ + f ¯ k ¯ Φ 0 r r .
But (17) yields the first estimate for r 0 as below:
r h 1 k ¯ Φ 0 f ¯ .
Next, is to show that T is Lipschitz
| ( T z 1 ) ( t ) ( T z 2 ) ( t ) | = 0 t k ( t , s ) f ( t , z 1 ( t ) ) ) z 1 ( s ) f ( t , z 2 ( t ) ) ) z 2 ( s ) d Φ ( t , s ) 0 t | k ( t , s ) | [ | f ( t , z 1 ( t ) ) | | z 1 ( s ) z 2 ( s ) | + z 2 ( t ) | f ( t , z 1 ( t ) ) f ( t , z 2 ( t ) ) | ] d s Φ ( t , s ) 0 t | k ( t , s ) | [ | f ( t ) | | z 1 ( s ) z 2 ( s ) | + | z 2 ( t ) | η 1 | z 1 ( t ) z 2 ( t ) | ] d s Φ ( t , s ) k ¯ ( f ¯ + η 1 z 2 ) z 1 z 2 × 0 t d s Φ ( t , s ) k ¯ Φ 0 ( f ¯ + η 2 z 2 ) z 1 z 2 .
On assuming z ( B r ) and in view of contraction principle, this yields:
k ¯ Φ 0 ( f ¯ + η 2 r ) k ¯ Φ 0 < 1 .
From (19) we obtain a complementary estimate for r 0 below:
r < 1 k ¯ Φ 0 f ¯ η 2 k ¯ Φ 0 .
Combining (18) and (20) and in view of (11) we obtain the desired valid estimates for r 0 as follows:
h 1 k ¯ Φ 0 f ¯ r 0 < 1 k ¯ Φ 0 f ¯ η 2 k ¯ Φ 0 .
So, choosing t 0 ( 0 , 1 ) such that (19) holds we obtain a contraction constant η 3 for T as below:
η 3 = k ¯ Φ 0 ( f ¯ + η 2 r 0 ) k ¯ Φ 0 .
Based on above we apply Rothe’s fixed point theorem (Theorem6) to conclude that there exists a unique fixed point z C ( [ 0 , t 0 ] ) of T which is the desired unique solution of (10). □
We will employ solvabity procedure of Theorem fo obtain solution of the linear part of the problem below to enable us apply method of variation of parameters for its sovability.
Theorem 8. 
Let the data h ( t ) , f ( u , t ) , Φ ( t , s ) , and g ( t , u ) , and of the quadratic integral equation
u ( t ) = h ( t ) + f ( t , u ) o t k ( t , s ) g ( s , u ( s ) ) d s Φ ( t , s )
satisfy the properties ( H 1 ) , ( H 2 ) , ( H 3 ) ( H 4 ) , ( H 4 ) and ( H 6 ) . Let t 0 ( 0 , 1 ) be such that the following condition holds:
Φ 0 k ¯ η 1 ( η 2 + 1 ) h < ( 1 Φ 0 k ¯ η 1 f ¯ ) ( 1 Φ 0 k ¯ η 1 f ¯ ( η 2 + 1 ) ) where :
f ¯ = sup ( t , s ) [ 0 , t 0 ] × [ 0 , t 0 ] f ( t , s ) ;
k ¯ = sup ( t , s ) Δ 0 k ( t , s ) .
Φ 0 = sup ( t , s ) Δ 0 Φ ( t , s ) ; ;
Δ 0 = { ( t , s ) [ 0 , t 0 ] × [ 0 , t 0 ] : 0 s t 0 < 1 } .
Then the integral equation (23) has a unique solution u C [ 0 , t 0 ] .
PROOF
Without loss of generality, we shall assume that g ( t , 0 ) = 0 for all t ( 0 , t 0 ) and as in the proof of Theorem we are to estimate values r 0 for r > 0 to enable application of Rothe fixed point theorem on an operator T : B r C [ 0 , t 0 ] .
Again, B r denotes a ball centered at the origin with radius r > 0 , we are to determine a value r 0 for r such that a mapping T : B r 0 C ( [ 0 , 1 ] ) satisfies the requirements of Rothe’s Theorem 6. Here, we define the mapping T by
( T u ) ( t ) = h ( t ) + f ( t , u ( t ) ) 0 t k ( t , s ) g ( u ( s ) ) d s Φ ( t , s ) .
To apply nearness of the superposition operator G ( u ) = g ( t , u ) to identity map I; the last equation is modified into:
( T u ) ( t ) = h ( t ) + f ( t , u ( t ) ) 0 t k ( t , s ) u ( s ) d s Φ ( t , s ) + f ( t , u ( t ) ) 0 t k ( t , s ) [ g ( u ( s ) ) u ( s ) ) ] d s Φ ( t , s ) .
Clearly,
| T u ( t ) | | h ( t ) + | f ( t , u ( t ) | 0 t | k ( t , s ) | | u ( s ) | d s Φ ( t , s ) + | f ( t , u ( t ) ) | 0 t | k ( t , s ) [ g ( s , u ( s ) ) u ( s ) ] d s Φ ( t , s ) | h ( t ) | + | f ( t , s ) | 0 t | k ( t , s ) | | u ( s ) | d s Φ ( t , s ) + | f ( t , u ( t ) ) | 0 t | k ( t , s ) | [ ( u ( s ) 0 ) g ( s , u ( s ) ) g ( s . 0 ) ] d s Φ ( t , s ) = | h ( t ) | + | f ( t , u ( t ) ) | 0 t | k ( t , s ) | ( ( u ( s ) 0 ) [ ( G ( u ) ) ( s ) G ( 0 ) ] d s Φ ( t , s ) | h ( t ) | + η 1 | f ( t , u ( t ) ) | 0 t | k ( t , s ) | | u ( s ) | d s Φ ( t , s ) T u h + f ¯ k ¯ Φ 0 r + Φ 0 f ¯ k ¯ η 2 r r h + [ Φ 0 f ¯ k ¯ + Φ 0 f ¯ η 2 k ¯ ] r r = h + [ Φ 0 f ¯ k ¯ [ η 2 + 1 ] ] r r
yielding:
r h 1 f ¯ Φ 0 k ¯ [ η 2 + 1 ]
To show that the mapping T is a contraction, we proceed as follows to find its contraction constant η T .
But
| ( T u 1 ) ( t ) ( T u 2 ) ( t ) | f ( t , u ( t ) | 0 t k ( t , s ) [ u 1 ( s ) u 2 ( s ) ] d s Φ ( t , s ) + 0 t k ( t , s ) [ f ( t , u 1 ( t ) ( g ( u 1 ) u 1 ) f ( t , u ( t ) ) g ( u 2 ) u 2 ] d s Φ ( t s ) | f ( t , u ( t ) | 0 t | k ( t , s ) | | u 1 ( s ) u 2 ( s ) | d s Φ ( t , s ) + 0 t | k ( t , s ) | [ f ( t , u 1 ( t ) | | ( g ( u 1 ) u 1 ( g ( u 2 ) u 2 ) | + | g ( u 2 ) | | f ( t , u 1 ) f ( t , u 2 ) | ] d s Φ ( t s ) = | f ( t , u ( t ) | 0 t | k ( t , s ) | | u 1 ( s ) u 2 ( s ) | d s Φ ( t , s ) + 0 t | k ( t , s ) | [ f ( t , u 1 ( s ) | | ( u 1 u 2 ) ( g ( u 1 ( s ) ) g ( u 2 ( s ) ) | + | g ( u 2 ) | | f ( u 1 ) f ( u 2 ) | ] d s Φ ( t , s ) = | f ( t , u ( t ) | 0 t | k ( t , s ) | | u 1 ( s ) u 2 ( s ) | d s Φ ( t , s ) + 0 t | k ( t , s ) | [ η 2 f ( t , u 1 ( s ) | | ( u 1 ( s ) u 2 ( s ) | + | g ( u 2 ) | η 1 | u 1 ( s ) u 2 ( s ) | d s Φ ( t , s ) T f ¯ Φ 0 k ¯ u 1 u 2 + k ¯ Φ 0 [ η 2 f ¯ u 1 u 2 + r 0 η 1 u 1 u 2 ] = f ¯ Φ 0 k ¯ + k ¯ Φ 0 [ η 2 f ¯ + r 0 η 1 ] u 1 u 2
To obtain a contraction constant η 3 < 1 , we set
η 3 = f ¯ Φ 0 k ¯ + k ¯ Φ 0 η 2 f ¯ + k ¯ Φ 0 η 1 r < 1
But 32 can yield a complementary estimate for r 0 as follows:
k ¯ Φ 0 η 1 r < 1 f ¯ Φ 0 k ¯ ( η 2 + 1 )
r < 1 f ¯ Φ 0 k ¯ ( η 2 + 1 ) k ¯ Φ 0 η 1
we, combining estimate 30 and estimate 33, we obtain the desired valid estimates for r 0 using
h 1 f ¯ Φ 0 k ¯ ( η 2 + 1 ) r 1 f ¯ Φ 0 k ¯ ( η 2 + 1 ) k ¯ Φ 0 η 1
In view of the requirement (24) we conclude that for T ( B r 0 ) B r 0 we must have
r 0 h 1 f ¯ Φ 0 k ¯ ( η 2 + 1 ) , 1 f ¯ Φ 0 k ¯ ( η 2 + 1 ) k ¯ Φ 0 η 1
From above, we conclude that the operator T has a unique fixed point u C [ 0 , t 0 ] ) .

3. Application to Fractional Dynamics

The results in this section are Corollaries following from our main results above and applications to problems of fractional dynamics and other singular problems.
Corollary 3. 
Let the hypotheses H1, H2, H3, and H5 hold, Suppose ϕ ( t ) is the right derivative of the Young’s function Ψ ( t , s ) then the singular integral equation
u ( t ) = h ( t ) + f ( t , u ( t ) ) 0 t k ( s , t ) ϕ ( t , s ) g ( t , s ) d s
has a unique solution.
The next theorem illustrates applications of nearness principle to resolution of hitherto difficult solvability of fractional dynamic problems with degenerate perturbation of identity by nonlinearities which are neither small nor contractive.
Theorem 9. 
Let h, f, k, and g satisfy the hypotheses H1 - H6 and 0 s φ ( t , τ ) d τ is a Young function in variable s, then the quadratic integral equation
u ( t ) = f ( t , u ( t ) ) 0 t k ( t , s ) φ ( t , s ) g ( s , u ( s ) ) d s
has a unique solution.
Theorem 10. 
Let the hypotheses (H1-H6) be satisfied for h, f, k and g in the equation
u ( t ) = h ( t ) + f ( t , u ( t ) ) 0 t k ( t , s ) ( t s ) 1 α g ( s , u ( s ) ) d s
if the condition below is satisfied
τ 0 α k ¯ η 1 ( η 2 + 1 ) h < ( 1 Φ 0 k ¯ η 1 f ¯ ) ( 1 f ¯ )
then the quadratic equation u ( t ) has a unique solution.

4. Illustrative Examples

Example 3. 
Investigate the solvability of the following quadratic integral equation
u ( t ) = h ( t ) + f ( t , u ( t ) ) 0 t t 2 s 2 1 + s sin u ( s ) d s , 0 t 1
where f ( t )
Solution
But d s 1 + s = d ln ( 1 + s ) So we set Φ ( t , s ) = ln ( 1 + s ) Since ln ( 1 + s ) is a convex increasing function. In fact ln ( 1 + s ) is convex since by theorem
d d s ln ( 1 + s ) = 1 1 + s > 0 s > 0 .
The function sin u is near identity with nearness constant i.e.
u 1 u 2 λ ( sin u 1 sin u 2 ) k u 1 u 2
with λ > 0 and k [ 0 , 1 ) Hence, by theorem 8 Also f 1 ¯ = sup f ( t , u ( t ) ) , k ¯ = 1 , Φ 0 = ln ( 1 + t 0 ) , Φ 0 η 1 , is the Lipchitz constant of f η 1 , η 2 = 1 c o s γ r ( 0 , 1 )
ln ( 1 + τ 0 ) η 1 ( 2 cos γ ) h < ( 1 l n ( 1 τ 0 ) η f ¯ )
Hence there exists solution ( u ( t ) on C [ 0 , t 0 ] for the equation 34.
Example 4. 
u ( t ) = h ( t ) + f ( t , u ( t ) ) 0 t t 2 s 2 ( t s ) 1 α sin u ( s ) d s , 0 t 1

Conclusion

It is important to remark that these auxiliary inequalities are bound to become more complicated as the integral equation () is made more complex. So, the novelty of the formulation in this present paper is in circumventing (or relaxing on) solvability requirements on equivalent auxiliary inequalities. In due course we will illustrate the complexities of these auxiliary inequalities with respect to different level of complexity of the corresponding integral equations. For instance, the next equation which is more complicated than () requires solvabilty of a more complicated pair of inequalities below:
η 1 r + h ¯ + k ¯ ν ¯ φ ( r ) ψ ( r ) r and η 1 + k ¯ ν ¯ η 2 ψ ( r ) < 1 .
The versatility of the nearness principle of operators is that, given any two functions A and B in a given Banach space, we have the following alternatives either:
(a)
A is near B
(b)
Or A is near B
(c)
Or A is orthogonal to B.
So, this informs the motivation of various researches into diverse connections between the nearness property and orthogonality property. These connections yield many positive possibilities leading to various generalizations of the concept of orthogonality in very general spaces like locally convex spaces and arbitrary metric spaces.

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