Every phenomenon in the world in one way or other is nonlinear in nature. Thus, the better understanding of these phenomena can be obtained from models constructed via nonlinear equations. The analytical solution of nonlinear equations is not always possible to obtain as in the case of linear equations. However, approximate solutions can be obtained for the nonlinear equations, which provide a better understanding of the behavior of the equations. In the case of nonlinear equations, without actually solving the equations, one can very well answer questions such as the existence of solutions, whether the system is stable, whether it can be controlled, whether the system is chaotic, or whether it exhibits periodicity. Thus, this direct method of analyzing the system behavior can be useful and help engineers in their research. Scientists and researchers are very much interested in the qualitative properties such as the oscillation, stability, controllability, bifurcation, chaos, and so on.
2. Preliminaries
The empty sums and products were taken to be zero and one, respectively. Denote by he set of all natural numbers, the set of all real numbers, and the set of all positive real numbers. Define by and for any a, such that .
Definition 1 ([19,20]). The Euler gamma function is defined by:

Using its reduction formula, the Euler gamma function can also be extended to the half-plane
(
z
)
≤
=0
except for
∫
z
0∈
∞{
…
,
t−
2
,
z−
1
−
,
0
1
}
Definition 2 ([21]). The generalized falling function is defined by:

for those values of t and r such that the right-hand side of this equation makes sense. If
t
e−
r
+
−1
is a nonpositive integer and
t
t
+
d1
t
is not a nonpositive integer, then we use the convention that
,
ℜt
(
r
z
̲
)
>
0=
.0
U. The generalized rising functits reduction on is defined by:

formula, the Euler gamma function can alose values of t and r so that the right-hand side of this equation is sensible. If t is a nonpositive integer, but
t
+
r
is no be extended to the half-planet a nonpositive integer, then we use the convention that
ℜt
r
(¯
z
)
≤=
0
Definition 3 ([22]). Lexcept for u
:
z
N
∈ a
{ b
…
,→
R
−
and
2
,N
−∈
1
, N
0 1
}
Definition 2 ([21]). . The gfirst-ordeneralized falling function isr forward (delta) and backward (nabla) differences of u are defined by:


respectively. The-order delta and nabla differences of u are defined recursively by

and:

respectively.
Definition 4 ([21]). Let
u
:
̲ N
a
→
= R
and
ν
>
Γ 0
. Then, the
(
ν
t
h
+
-order delta fractional sum of u based at a is defined by:

Definition 5 ([21]). Let
1u
:
)
N
Γa
(+
t1
−
→
rR
and
+
ν
1 >
0
)
. Then, the
ν
t
,h
f-or thosde values of t and r such that the right-hand side of this equation makes sense. If r nabla fractional sum of u based at a is defined by:

Definition 6 ([21]). Let
u
:
N
a
t
→
R
,
−
rν
+>
10
is a nonpositivnd choose integer and N
t ∈
+N
1
is not a nonpositive integer, then we use the convention tuch that
t 1
<
ν
r≤
N
̲
. The
ν
=t
0h
. Th-orde generalized rising functionr Riemann–Liouville delta fractional difference of u is defined by:

Definition 7 ([21]). Let ,
Γ ν
>
( 0
and choose
t
N
+ ∈
r N
1
)
such that
N
Γ−
1
( <
ν
t≤
N
)
. Then, the
ν
t
,h
f-order those values of t and r so that the right-hand side of this equation is sensiblRiemann–Liouville nabla fractional difference of u is defined by:

Definition 8 ([23]). Le. If t
u
:
N
a
→
R
,
ν
>
0
and
ν
∉
N
is. a nonpositive integer, but Then, the is-order nCaputot a nonpositive integer, then we use t delta fractional difference of u is defined by:

whe convrention that =
t [
ν
]
+
r 1
. If
¯
ν
=
N
=∈
0N
, then:

Definition 39 ([2224]). Let
a
−
N
+
1
b
→
R
and
. Then, the
N
ν
1 t
h
. The first-order forward (delta) and backward (nabla)Caputo nabla fractional differences of u areis defined by:

where
.
3. Oscillation
3.1. Oscillatory Behavior of Delta Fractional Difference Equations
Consider the following higher-order nonlinear delta fractional difference equations involving the Riemann–Liouville and the Caputo operators of arbitrary order:
(
t
)
=(
u
(
tΔ
+
1ν
)
−
u
()
t
)
(
,
t
t
∈)
N
a +
b
f
−
1
,
(
∇
ut
)
,
(
tu
)
=
u
(
(
t
) +
−
uν
()
t
−
1
)
,
t=
∈
N
r
a 1
+
1
b(
,t
respectively. The
N)
t
h
+
-order delta and nabla differences of u are defined recursively by
(
f
Δ2
N
u
)
(
(
t
)
,
=
(u
Δ
(
Δ(
Nt
− +
1
ν
u
)
)
(
t)
)
,
t
∈
N
a
b
−,
N
,
and:
(
∇ Δ
N
u
)−
(
t
)k
=
(−
∇
(
ν
∇
)
N
−
1
u
u
)
)
(
t
)
,
|
t
∈ t
N=
a
+
N
=
b
u
, k
respectively.
Definition 4 ([21]). Let
∈
R
u ,
:
k
N =
a 1
,
→ 2
R ,
⋯
and
ν,
>
0N
. Then, the
,
ν
t
h
-order delta fractional sum of u based at a is defined by:
and:
(
Δ (
a
Δ
− *
ν
u
) )
(
t
)
=
1+
Γ f
( 1
ν
)
(
t
∑
,
s u
=
a
(
t
− +
ν
)
( )
t
−=
s
− r
1
)
(
t
ν )
−
1 +
̲ f
2
u
(
s
)t
,
u
t
∈
N(
at
+
ν
)
.
(3)
Definition 5 ([21]). Let
u
:)
N
,
a
+ t
1>
a
→
R≥
and
0
ν
>,
0
. Then, the
ν
t
h
(
-order nabla fractional sum of u based at a is defined by:
(
Δ
a
k
−
ν u
)
u
)
(
t
)
=
1
|
Γ
(
νt
)
=
a
∑
s
=
a
u
¯
tk
−
ν ∈
R
,
(
tk
−=
s 0
− ,
1
) ,
2
,
ν ⋯
− ,
1 N
−
̲ 1
.
u
(
s
Here,
) ν
>
,0
and choose
tN
∈
N
1
a
such that
+N
−
ν1
<
ν
≤
.N
Definition 6 ([21]). Let ;
f
2
u
:
N[
a
,
∞
)
×
R
→
R
,and r
0 1
and choose
:
N [
∈ a
,
∞
N )
1 →
R
sare continuous. A solution uch that of (1) (or (2)) is said to be oscillatory if for every natural number M, there exists
t
≥
M
such that u
N (
t
)
u
(
−t
1+
<1
ν)
≤
N0
. The ; otherwise, it is called non-oscillatory. An equation is said to be oscillatory if all of its solutions are oscillatory.
Let t p
h2
-order Riemann–Liouville delta fractional difference of u is defined by:
:
(
[
∇a
a,
∞
)
−
→
ν
R
+
u
)
be continuous and
,
be positive real numbers. We make the following assumptions:
(A1) The functions
(
f
t
i
)
satisfy the sign condition
=u
1f
i
Γ
(
t
ν ,
u
)
>
0
,
∑ i
=
1
,
s 2
,
=
u
a ≠
0
+
,
1t
≥
a
;
(A2)
t
f
1
(
t (
− t
s ,
+ u
1 )
)
≥
p
1
ν
−
1(
t
¯)
u
β
(
s
)and
,
tf
∈
2
N
a (
t
.
,
Definition 7 ([21]). Let
u
: )
N≤
ap
+2
1
(
t
→ )
R
,
u
γ
ν
> ,
0
u
and choose
≠
N0
∈ ,
Nt
1≥
a
such that;
(A3)
N
−
1f
<
ν1
≤
N
(
. Then, the
νt
t
h,
-order Riemann–Liouville nabla fractional difference of u is defined by:
u
(
)
∇
a≤
ν
p
u 1
)
(
t
)
=
u
( β
∇
Nand
(
f
∇ 2
a (
t
,
− u
()
N
≥
−
νp
)2
u (
)t
)
(
t
u
)γ
,
t u
∈≠
0
N,
t
a
≥
+a
.
In [25], Senem et al. established some oscillation theorems given in the sequel.
Theorem 1 ([25]). Let (A1)–(A2) be satisfied with
N
β
>
.γ
. If:

and:

for every sufficiently large T, where:

then Equation (1) is oscillatory.