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Kamenev-type oscillation criteria for higher-order nonlinear dynamic equations on time scales

Advances in Difference Equations20132013:248

https://doi.org/10.1186/1687-1847-2013-248

Received: 7 April 2013

Accepted: 1 August 2013

Published: 20 August 2013

Abstract

In this paper, we investigate the oscillation of the following higher-order dynamic equation:

{ r n ( t ) [ ( r n 1 ( t ) ( ( r 1 ( t ) x ( t ) ) ) ) ] γ } + F ( t , x ( τ ( t ) ) ) = 0

on an arbitrary time scale T, where n 2 , 1 r k ( t ) ( 1 k n ) are positive rd-continuous functions on T, and γ is the quotient of two odd positive integers, τ : T T with τ ( t ) > t and F C ( T × R , R ) . We give sufficient conditions under which every solution of this equation is either oscillatory or tends to zero.

MSC:34K11, 39A10, 39A99.

Keywords

oscillationdynamic equationtime scale

1 Introduction

Let R be the set of all real numbers, and let T be a time scale (i.e., a closed nonempty subset of R) with sup T = . In this paper, we study Kamenev-type oscillation criteria of solutions of the following higher-order dynamic equation:
{ r n ( t ) [ ( r n 1 ( t ) ( ( r 1 ( t ) x ( t ) ) ) ) ] γ } + F ( t , x ( τ ( t ) ) ) = 0 , t [ t 0 , ) T ,
(1.1)

where t 0 T is a constant and [ t , ) T = [ t , ) T for any t T . Throughout this paper, we assume that the following conditions are satisfied:

( H 1 ) 1 r k ( t ) C rd ( [ t 0 , ) T , ( 0 , ) ) ( 1 k n ).

( H 2 ) γ is the quotient of two odd positive integers.

( H 3 ) t 0 1 r k ( s ) s = t 0 [ 1 r n ( s ) ] 1 γ s = ( 1 k n 1 ).

( H 4 ) τ : T T is a nondecreasing function with τ ( t ) > t for any t T .

( H 5 ) F C ( T × R , R ) and there exists a positive rd-continuous function q ( t ) defined on T such that for any u 0 ,
F ( t , u ) u γ q ( t ) .
(1.2)
Write
S k ( t , x ( t ) ) = { x ( t ) if  k = 0 , r k ( t ) S k 1 ( t , x ( t ) ) if  1 k n 1 , r n ( t ) [ S n 1 ( t , x ( t ) ) ] γ if  k = n .
Then Eq. (1.1) reduces to the equation
S n ( t , x ( t ) ) + F ( t , x ( τ ( t ) ) ) = 0 .
(1.3)

By a solution of Eq. (1.3) we mean a nontrivial real-valued function x ( t ) C rd 1 ( [ T x , ) T ) with T x t 0 , which has the property that S k ( t , x ( t ) ) C rd 1 ( [ T x , ) T ) for 0 k n and satisfies Eq. (1.3) on [ T x , ) T , where C rd 1 is the space of differentiable functions whose derivative is rd-continuous. The solutions vanishing in some neighborhood of infinity will be excluded from our consideration. A solution x ( t ) of Eq. (1.3) is said to be oscillatory if it is neither eventually positive nor eventually negative; otherwise, it is called nonoscillatory.

The theory of time scales, which has recently received a lot of attention, was introduced by Stefan Hilger in his PhD thesis [1] in order to unify continuous and discrete analysis. The cases when a time scale T is equal to R or all integers Z represent the classical theories of differential and difference equations. Many results concerning differential equations carry over quite easily to corresponding results for difference equations, while other results seem to be completely different from their continuous counterparts. The study of dynamic equations on time scales reveals such discrepancies and helps avoid proving results twice - once for differential equations and once again for difference equations. The general idea is to prove a result for a dynamic equation where the domain of the unknown function is a time scale T. In this way results not only related to the set of real numbers or the set of integers but those pertaining to more general time scales are obtained. Therefore, not only can the theory of dynamic equations unify the theories of differential equations and difference equations, but it also extends these classical cases to cases ‘in between’, e.g., to the so-called q-difference equations when T = q N 0 , which has important applications in quantum theory (see [2]). In the last years there has been much research activity concerning the oscillation and asymptotic behavior of solutions of some dynamic equations on time scales, and we refer the reader to the papers [317] and the references cited therein.

Recently, Wang [18] extended the Hille and Nehari oscillation theorems to the third-order dynamic equation
( r 2 ( t ) ( ( r 1 ( t ) x ( t ) ) ) γ ) + q ( t ) f ( x ( t ) ) = 0 .
(1.4)
Erbe et al. in [1921] considered the third-order dynamic equations
( a ( t ) [ r ( t ) x ( t ) ] ) + p ( t ) f ( x ( t ) ) = 0 ,
(1.5)
x ( t ) + p ( t ) x ( t ) = 0
(1.6)
and
( a ( t ) { [ r ( t ) x ( t ) ] } γ ) + f ( t , x ( t ) ) = 0 ,
(1.7)

respectively, and established some sufficient conditions for oscillation.

Hassan [22] studied the third-order dynamic equation
( a ( t ) { [ r ( t ) x ( t ) ] } γ ) + f ( t , x ( τ ( t ) ) ) = 0
(1.8)

and obtained some oscillation criteria, which improved and extended the results that were established in [1921].

Hassan [23] studied the Kamenev-type oscillation criteria of the second-order dynamic equation
( r ( t ) ( x ( t ) ) γ ) + f ( t , x ( g ( t ) ) ) = 0
(1.9)

and established some new sufficient conditions, which improved some oscillation results for second-order differential and difference equations.

2 Some auxiliary lemmas

We shall employ the following lemmas.

Lemma 2.1 [24]

Let 1 m n . Then:
  1. (1)

    lim inf t S m ( t , x ( t ) ) > 0 implies lim t S i ( t , x ( t ) ) = for 0 i m 1 .

     
  2. (2)

    lim sup t S m ( t , x ( t ) ) < 0 implies lim t S i ( t , x ( t ) ) = for 0 i m 1 .

     
Lemma 2.2 Suppose that x ( t ) is an eventually positive solution of Eq. (1.3), then there exist an integer [ 0 , n ] and T [ t 0 , ) T such that:
  1. (1)

    n + is even.

     
  2. (2)

    > 0 implies that S i ( t , x ( t ) ) > 0 for any t T and 0 i 1 .

     
  3. (3)

    n 1 implies that ( 1 ) + i S i ( t , x ( t ) ) > 0 for any t T and i n 1 .

     
Proof Since x ( t ) is an eventually positive solution of Eq. (1.3), there exists a t 1 t 0 such that x ( t ) > 0 and x ( τ ( t ) ) > 0 on [ t 1 , ) T . It follows from (1.3) that
S n ( t , x ( t ) ) = F ( t , x ( τ ( t ) ) ) q ( t ) x γ ( τ ( t ) ) < 0 for  t t 1 .

Hence S n ( t , x ( t ) ) is decreasing on [ t 1 , ) T .

We claim that S n ( t , x ( t ) ) > 0 for all t [ t 1 , ) T . If not, there exists a t 2 [ t 1 , ) T such that
S n ( t , x ( t ) ) S n ( t 2 , x ( t 2 ) ) < 0 for  t t 2 .
Then we obtain
S n 1 ( t , x ( t ) ) S n 1 ( t 2 , x ( t 2 ) ) + S n 1 γ ( t 2 , x ( t 2 ) ) t 2 t [ 1 r n ( s ) ] 1 γ s ( t ) .

By Lemma 2.1, we get lim t x ( t ) = , which contradicts with x ( t ) > 0 eventually. Then S n ( t , x ( t ) ) > 0 for all t [ t 1 , ) T . This implies that exactly one of the following is true:

( a 1 ) S n 1 ( t , x ( t ) ) < 0 for t t 1 ;

( b 1 ) There exists a t 3 t 1 such that S n 1 ( t , x ( t ) ) S n 1 ( t 3 , x ( t 3 ) ) > 0 for t t 3 .

If ( b 1 ) holds, then we obtain by Lemma 2.1
lim t S n 2 ( t , x ( t ) ) = lim t S n 3 ( t , x ( t ) ) = = lim t x ( t ) = .

Thus the conclusions of Lemma 2.2 hold.

If ( a 1 ) holds, then S n 2 ( t , x ( t ) ) is strictly decreasing on [ t 1 , ) T and exactly one of the following is true:

( a 2 ) S n 2 ( t , x ( t ) ) > 0 for t t 1 ;

( b 2 ) There exists a t 4 t 1 such that S n 2 ( t , x ( t ) ) S n 1 ( t 4 , x ( t 4 ) ) < 0 for t t 4 .

If ( b 2 ) holds, then we obtain by Lemma 2.1
lim t S n 3 ( t , x ( t ) ) = lim t S n 4 ( t , x ( t ) ) = = lim t x ( t ) = ,

which contradicts with x ( t ) > 0 eventually. Hence ( b 2 ) is impossible.

From ( a 2 ), we see that S n 3 ( t , x ( t ) ) is strictly increasing on [ t 1 , ) T and exactly one of the following is true:

( a 3 ) S n 3 ( t , x ( t ) ) < 0 for t t 1 ;

( b 3 ) There exists a t 5 t 1 such that S n 3 ( t , x ( t ) ) S n 3 ( t 5 , x ( t 5 ) ) > 0 for t t 5 .

Therefore we can repeat the above argument and show that the conclusions of Lemma 2.2 hold. The proof is completed. □

Remark 2.3 Let r n ( t ) = = r 1 ( t ) = 1 and T be the set of integers. Then Lemma 2.1 and Lemma 2.2 are Lemma 1.8.10 and Theorem 1.8.11 of [3] respectively.

Lemma 2.4 Assume that
t 0 1 r n 1 ( s ) { s [ 1 r n ( u ) u q ( v ) v ] 1 γ u } s =
(2.1)
holds and x ( t ) is an eventually positive solution of Eq. (1.3). Then there exists T [ t 0 , ) T sufficiently large such that either of the following cases holds:
  1. (1)

    S i ( t , x ( t ) ) > 0 for any t T and 0 i n .

     
  2. (2)

    lim t x ( t ) = 0 .

     
Proof Since x ( t ) is an eventually positive solution of Eq. (1.3), there exists a t 1 t 0 such that x ( t ) > 0 and x ( τ ( t ) ) > 0 on [ t 1 , ) T . It follows from (1.3) that
S n ( t , x ( t ) ) = F ( t , x ( τ ( t ) ) ) q ( t ) x γ ( τ ( t ) ) < 0 for  t t 1 .

By Lemma 2.2, we see that there exists an integer 0 n , with + n being even, such that ( 1 ) + i S i ( t , x ( t ) ) > 0 for t t 1 and i n , and x ( t ) is eventually monotone.

We claim that lim t x ( t ) 0 implies = n . If not, then S n 1 ( t , x ( t ) ) < 0 ( t t 1 ) and S n 2 ( t , x ( t ) ) > 0 ( t t 1 ). It is easy to see that there exist a t 2 t 1 and a constant M > 0 such that x ( τ ( t ) ) M on [ t 2 , ) T . Integrating Eq. (1.3) from t to ∞, we get that for t t 2 ,
r n ( t ) [ S n 1 ( t , x ( t ) ) ] γ = S n ( t , x ( t ) ) M γ t q ( s ) s .
Thus
S n 1 ( t , x ( t ) ) M t [ 1 r n ( s ) s q ( u ) u ] 1 γ s for  t t 2 .
Again, integrating the above inequality from t 2 to t, we obtain that for t t 2 ,
S n 2 ( t , x ( t ) ) S n 2 ( t 2 , x ( t 2 ) ) M t 2 t 1 r n 1 ( s ) { s [ 1 r n ( u ) u q ( v ) v ] 1 γ u } s .

It follows from (2.1) that lim t S n 2 ( t , x ( t ) ) = , which is a contradiction to S n 2 ( t , x ( t ) ) > 0 ( t t 1 ). Thus = n . The proof is completed. □

Lemma 2.5 Let x ( t ) be a solution of Eq. (1.3) such that case (1) of Lemma  2.4 holds for t [ T , ) T with some T [ t 0 , ) T . Then we have that for t [ T , ) T ,
S i ( t , x ( t ) ) S n 1 γ ( t , x ( t ) ) ϑ i + 1 ( t , T ) , 0 i n 1
(2.2)
and
S n 1 ( t , x ( t ) ) x σ ( t ) [ t q ( s ) s r n ( t ) ] 1 γ ,
(2.3)
where
ϑ i ( t , T ) = { T t [ 1 r n ( s ) ] 1 γ s if i = n , T t ϑ i + 1 ( s , T ) r i ( s ) s if 1 i n 1 .
(2.4)
Proof Because x ( t ) is an eventually positive solution of Eq. (1.3), there exists a T t 0 sufficiently large such that x ( t ) > 0 and x ( τ ( t ) ) > 0 for t T . Note S n ( t , x ( t ) ) = F ( t , x ( τ ( t ) ) ) q ( t ) x γ ( τ ( t ) ) < 0 , we know that S n ( t , x ( t ) ) is strictly decreasing on [ T , ) T . Then for t T ,
S n 1 ( t , x ( t ) ) S n 1 ( t , x ( t ) ) S n 1 ( T , x ( T ) ) = T t [ S n ( s , x ( s ) ) r n ( s ) ] 1 γ s S n 1 γ ( t , x ( t ) ) ϑ n ( t , T ) , S n 2 ( t , x ( t ) ) S n 2 ( t , x ( t ) ) S n 2 ( T , x ( T ) ) = T t S n 1 ( s , x ( s ) ) r n 1 ( s ) s S n 1 γ ( t , x ( t ) ) ϑ n 1 ( t , T ) .
Repeating the above process, we have
S 1 ( t , x ( t ) ) S 1 ( t , x ( t ) ) S 1 ( T , x ( T ) ) = T t S 2 ( s , x ( s ) ) r 2 ( s ) s S n 1 γ ( t , x ( t ) ) ϑ 2 ( t , T ) , S 0 ( t , x ( t ) ) x ( t ) x ( T ) = T t S 1 ( s , x ( s ) ) r 1 ( s ) s S n 1 γ ( t , x ( t ) ) ϑ 1 ( t , T ) .
Thus it follows
r n ( t ) [ S n 1 ( t , x ( t ) ) ] γ = S n ( t , x ( t ) ) t F ( s , x ( τ ( s ) ) ) s t q ( s ) x γ ( τ ( s ) ) s x γ ( τ ( t ) ) t q ( s ) s x γ ( σ ( t ) ) t q ( s ) s .
That is,
S n 1 ( t , x ( t ) ) x σ ( t ) [ t q ( s ) s r n ( t ) ] 1 γ .

The proof is completed. □

Lemma 2.6 [25]

Let f : R R be continuously differentiable and suppose that g : T R is delta differentiable. Then f g is delta differentiable and the formula
( f g ) ( t ) = g ( t ) 0 1 f ( h g σ ( t ) + ( 1 h ) g ( t ) ) d h
(2.5)

holds.

Lemma 2.7 [23]

Suppose that a and b are nonnegative real numbers and λ 1 . Then
λ a b λ 1 a λ ( λ 1 ) b λ ,
(2.6)

where the equality holds if and only if a = b .

3 Main results

For convenience, we write D { ( t , s ) | t s t 0 } . Now we state and prove our main results.

Theorem 3.1 Assume that (2.1) holds. Furthermore, suppose that there exist G , g C rd ( D , R ) with G s C rd ( D , R ) such that
G ( t , t ) = 0 for any t t 0 and G ( t , s ) > 0 for any t > s t 0 ,
(3.1)
where G s is the -partial derivative with respect to the second variable, and there exist m : T R , such that r n ( t ) m ( t ) is a delta differentiable function, and a delta differentiable function M : T ( 0 , ) such that
G s ( t , s ) + G ( t , s ) β ( s , T ) M σ ( s ) = g ( t , s ) M σ ( s ) M ( s ) G ( t , s ) for t > s t 0
(3.2)
and
lim sup t 1 G ( t , T ) T t [ G ( t , s ) ψ ( s , T ) g 2 ( t , s ) r 1 ( s ) 4 γ η ( s , T ) ] s =
(3.3)
for all sufficiently large T, where
η ( t , T ) = { ϑ 2 ( t , T ) ( t q ( s ) s ) 1 γ γ if 0 < γ 1 , ϑ 1 γ 1 ( t , T ) ϑ 2 ( t , T ) if γ 1 ,
(3.4)
ψ ( t , T ) = M ( t ) q ( t ) M ( t ) ( r n ( t ) m ( t ) ) + γ M ( t ) r 1 ( t ) η ( t , T ) ( ( r n ( t ) m ( t ) ) σ ) 2 ,
(3.5)
β ( t , T ) = M ( t ) + 2 γ M ( t ) η ( t , T ) r 1 ( t ) ( r n ( t ) m ( t ) ) σ
(3.6)
and
g ( t , s ) = max { 0 , g ( t , s ) } .
(3.7)

Then every solution x ( t ) of Eq. (1.3) is either oscillatory or tends to zero.

Proof Assume that Eq. (1.3) has a nonoscillatory solution x ( t ) on [ t 0 , ) T . Then, without loss of generality, there is a T t 0 , sufficiently large, such that x ( t ) > 0 for t T . By Lemma 2.4, there are two possible cases:
  1. (1)

    S i ( t , x ( t ) ) > 0 for any t T and 0 i n .

     
  2. (2)

    lim t x ( t ) = 0 .

     
If case (1) holds, then set
ω ( t ) = M ( t ) [ S n ( t , x ( t ) ) x γ ( t ) + r n ( t ) m ( t ) ] = M ( t ) r n ( t ) [ ( S n 1 ( t , x ( t ) ) x ( t ) ) γ + m ( t ) ] ,
(3.8)
we have
ω ( t ) = ( M ( t ) S n ( t , x ( t ) ) x γ ( t ) ) + ( M ( t ) r n ( t ) m ( t ) ) = M ( t ) x γ ( t ) S n ( t , x ( t ) ) + ( M ( t ) x γ ( t ) ) S n σ ( t , x ( t ) ) + M ( t ) ( r n ( t ) m ( t ) ) + M ( t ) ( r n ( t ) m ( t ) ) σ = M ( t ) x γ ( t ) S n ( t , x ( t ) ) + ( M ( t ) x γ σ ( t ) M ( t ) ( x γ ( t ) ) x γ ( t ) x γ σ ( t ) ) S n σ ( t , x ( t ) ) + M ( t ) ( r n ( t ) m ( t ) ) + M ( t ) ( r n ( t ) m ( t ) ) σ .
It follows from (1.3) and the definition of ω ( t ) that for all t T ,
ω ( t ) = M ( t ) x γ ( t ) F ( t , x ( τ ( t ) ) ) + M ( t ) ( r n ( t ) m ( t ) ) + M ( t ) M σ ( t ) ω σ ( t ) M ( t ) ( x γ ( t ) ) x γ ( t ) S n σ ( t , x ( t ) ) x γ σ ( t ) .
Using the fact that F ( t , x ( τ ( t ) ) ) q ( t ) x γ ( τ ( t ) ) and x ( t ) is increasing on [ T , ) T , we get
ω ( t ) M ( t ) q ( t ) + M ( t ) ( r n ( t ) m ( t ) ) + M ( t ) M σ ( t ) ω σ ( t ) M ( t ) ( x γ ( t ) ) x γ ( t ) S n σ ( t , x ( t ) ) x γ σ ( t ) .
(3.9)

Now we consider the following two cases.

Case 1: If 0 < γ 1 , then it follows from x ( t ) > 0 and Lemma 2.6 that x σ ( t ) x ( t ) and
( x γ ( t ) ) = γ x ( t ) 0 1 ( h x σ ( t ) + ( 1 h ) x ( t ) ) γ 1 d h γ x ( t ) 0 1 ( h x σ ( t ) + ( 1 h ) x σ ( t ) ) γ 1 d h = γ ( x σ ( t ) ) γ 1 x ( t ) .
(3.10)
By (3.9) and (3.10), we have
ω ( t ) M ( t ) q ( t ) + M ( t ) ( r n ( t ) m ( t ) ) + M ( t ) M σ ( t ) ω σ ( t ) γ M ( t ) x ( t ) x σ ( t ) x γ σ ( t ) x γ ( t ) S n σ ( t , x ( t ) ) x γ σ ( t ) .
(3.11)
It follows from Lemma 2.5 that
x ( t ) S n 1 γ ( t , x ( t ) ) ϑ 2 ( t , T ) r 1 ( t ) , x ( t ) S n 1 γ ( t , x ( t ) ) ϑ 1 ( t , T ) , S n 1 ( t , x ( t ) ) x σ ( t ) [ t q ( s ) s r n ( t ) ] 1 γ .
(3.12)
Then
x ( t ) x σ ( t ) = r n 1 γ 1 ( t ) S n ( t , x ( t ) ) x γ σ ( t ) ( S n 1 ( t , x ( t ) ) x σ ( t ) ) 1 γ x ( t ) S n 1 γ ( t , x ( t ) ) r n 1 γ 1 ( t ) S n ( t , x ( t ) ) x γ σ ( t ) ( ( t q ( s ) s r n ( t ) ) 1 γ ) 1 γ ϑ 2 ( t , T ) r 1 ( t ) ϑ 2 ( t , T ) r 1 ( t ) ( t q ( s ) s ) 1 γ γ S n σ ( t , x ( t ) ) x γ σ ( t ) .
(3.13)
Combining (3.11) with (3.13), we get
ω ( t ) M ( t ) q ( t ) + M ( t ) ( r n ( t ) m ( t ) ) + M ( t ) M σ ( t ) ω σ ( t ) γ M ( t ) ϑ 2 ( t , T ) r 1 ( t ) [ t q ( s ) s ] 1 γ γ ( S n σ ( t , x ( t ) ) x γ σ ( t ) ) 2 .
(3.14)
Case 2: If γ 1 , then it follows from x ( t ) > 0 and Lemma 2.6 that x σ ( t ) x ( t ) and
( x γ ( t ) ) = γ x ( t ) 0 1 ( h x σ ( t ) + ( 1 h ) x ( t ) ) γ 1 d h γ x ( t ) 0 1 ( h x ( t ) + ( 1 h ) x ( t ) ) γ 1 d h = γ ( x ( t ) ) γ 1 x ( t ) .
(3.15)
By (3.9) and (3.15), we have
ω ( t ) M ( t ) q ( t ) + M ( t ) ( r n ( t ) m ( t ) ) + M ( t ) M σ ( t ) ω σ ( t ) γ M ( t ) x ( t ) x ( t ) S n σ ( t , x ( t ) ) x γ σ ( t ) .
(3.16)
It follows from (3.12) that
x ( t ) x ( t ) = S n ( t , x ( t ) ) x γ ( t ) ( x ( t ) S n 1 γ ( t , x ( t ) ) ) γ 1 x ( t ) S n 1 γ ( t , x ( t ) ) S n ( t , x ( t ) ) x γ ( t ) ( ϑ 1 ( t , T ) ) γ 1 ϑ 2 ( t , T ) r 1 ( t ) ( ϑ 1 ( t , T ) ) γ 1 ϑ 2 ( t , T ) r 1 ( t ) S n σ ( t , x ( t ) ) x γ σ ( t ) .
(3.17)
Combining (3.16) with (3.17) gives
ω ( t ) M ( t ) q ( t ) + M ( t ) ( r n ( t ) m ( t ) ) + M ( t ) M σ ( t ) ω σ ( t ) γ M ( t ) ( ϑ 1 ( t , T ) ) γ 1 ϑ 2 ( t , T ) r 1 ( t ) ( S n σ ( t , x ( t ) ) x γ σ ( t ) ) 2 .
(3.18)
Noting that the definitions of η ( t , T ) , ψ ( t , T ) and β ( t , T ) . It follows from (3.14), (3.18) and the fact
S n σ ( t , x ( t ) ) x γ σ ( t ) = ω σ ( t ) M σ ( t ) r n σ ( t ) m σ ( t )
that for γ > 0 ,
ψ ( t , T ) ω ( t ) + β ( t , T ) M σ ( t ) ω σ ( t ) γ M ( t ) η ( t , T ) r 1 ( t ) ( M σ ( t ) ) 2 ( ω σ ( t ) ) 2 .
(3.19)
Multiplying both sides of (3.19), with t replaced by s, by G ( t , s ) and integrating with respect to s from T to t ( t T ), one gets
T t G ( t , s ) ψ ( s , T ) s T t G ( t , s ) ω ( s ) s + T t G ( t , s ) β ( s , T ) M σ ( s ) ω σ ( s ) s T t γ G ( t , s ) M ( s ) η ( s , T ) r 1 ( s ) ( M σ ( s ) ) 2 ( ω σ ( s ) ) 2 s .
Integrating by parts and using (3.1) and (3.2), we have
T t G ( t , s ) ψ ( s , T ) s G ( t , T ) ω ( T ) + T t G s ( t , s ) ω σ ( s ) s + T t G ( t , s ) β ( s , T ) M σ ( s ) ω σ ( s ) s T t γ G ( t , s ) M ( s ) η ( s , T ) r 1 ( s ) ( M σ ( s ) ) 2 ( ω σ ( s ) ) 2 s = G ( t , T ) ω ( T ) + T t [ g ( t , s ) M σ ( s ) M ( s ) G ( t , s ) ω σ ( s ) γ G ( t , s ) M ( s ) η ( s , T ) r 1 ( s ) ( M σ ( s ) ) 2 ( ω σ ( s ) ) 2 ] s G ( t , T ) ω ( T ) + T t [ g ( t , s ) M σ ( s ) M ( s ) G ( t , s ) ω σ ( s ) γ G ( t , s ) M ( s ) η ( s , T ) r 1 ( s ) ( M σ ( s ) ) 2 ( ω σ ( s ) ) 2 ] s .
(3.20)
It is easy to check that
g ( t , s ) M σ ( s ) M ( s ) G ( t , s ) ω σ ( s ) γ G ( t , s ) M ( s ) η ( s , T ) r 1 ( s ) ( M σ ( s ) ) 2 ( ω σ ( s ) ) 2 = g 2 ( t , s ) r 1 ( s ) 4 γ η ( s , T ) γ M ( s ) η ( s , T ) r 1 ( s ) ( M σ ( s ) ) 2 ( G ( t , s ) ω σ ( s ) g ( t , s ) M σ ( s ) r 1 ( s ) 2 γ M ( s ) η ( s , T ) ) 2 ,
which implies
g ( t , s ) M σ ( s ) M ( s ) G ( t , s ) ω σ ( s ) γ G ( t , s ) M ( s ) η ( s , T ) r 1 ( s ) ( M σ ( s ) ) 2 ( ω σ ( s ) ) 2 g 2 ( t , s ) r 1 ( s ) 4 γ η ( s , T ) .
(3.21)
Combining (3.21) with (3.20), it follows
1 G ( t , T ) T t [ G ( t , s ) ψ ( s , T ) g 2 ( t , s ) r 1 ( s ) 4 γ η ( s , T ) ] s ω ( T ) ,

which contradicts assumption (3.3). Thus every solution x ( t ) of Eq. (1.3) is either oscillatory or tends to zero. The proof is completed. □

Theorem 3.2 Assume that (2.1) holds. Furthermore, suppose that there exist H , h C rd ( D , R ) with H s C rd ( D , R ) such that
H ( t , t ) = 0 for any t t 0 and H ( t , s ) > 0 for any t > s t 0 ,
(3.22)
where H s is the -partial derivative with respect to the second variable, and there exists a delta differentiable function M : T ( 0 , ) such that
H s ( t , s ) + H ( t , s ) M ( s ) M σ ( s ) = h ( t , s ) M σ ( s ) ( M ( s ) H ( t , s ) ) γ γ + 1 for t > s t 0
(3.23)
and
lim sup t 1 H ( t , T ) T t [ M ( s ) q ( s ) H ( t , s ) h γ + 1 ( t , s ) r 1 γ ( s ) ( γ + 1 ) γ + 1 ϑ 2 γ ( s , T ) ] s =
(3.24)
for all sufficiently large T, where
h ( t , s ) = max { 0 , h ( t , s ) } .
(3.25)

Then every solution x ( t ) of Eq. (1.3) is either oscillatory or tends to zero.

Proof Assume that Eq. (1.3) has a nonoscillatory solution x ( t ) on [ t 0 , ) T . Then, without loss of generality, there is a T t 0 , sufficiently large, such that x ( t ) > 0 for t T . By Lemma 2.4, there are two possible cases:
  1. (1)

    S i ( t , x ( t ) ) > 0 for any t T and 0 i n .

     
  2. (2)

    lim t x ( t ) = 0 .

     
If case (1) holds, then set
ω ( t ) = M ( t ) [ S n ( t , x ( t ) ) x γ ( t ) ] = M ( t ) r n ( t ) [ ( S n 1 ( t , x ( t ) ) x ( t ) ) γ ] .
(3.26)
By (3.9), we have
ω ( t ) M ( t ) q ( t ) + M ( t ) M σ ( t ) ω σ ( t ) M ( t ) ( x γ ( t ) ) x γ ( t ) S n σ ( t , x ( t ) ) x γ σ ( t ) M ( t ) q ( t ) + M ( t ) M σ ( t ) ω σ ( t ) M ( t ) M σ ( t ) ( x γ ( t ) ) x γ ( t ) ω σ ( t ) .
(3.27)
It follows from Lemma 2.6 that
( x γ ( t ) ) = γ x ( t ) 0 1 ( h x σ ( t ) + ( 1 h ) x ( t ) ) γ 1 d h { γ ( x σ ( t ) ) γ 1 x ( t ) if  0 < γ 1 , γ ( x ( t ) ) γ 1 x ( t ) if  γ 1 .
(3.28)
Case 1. If 0 < γ 1 , then
ω ( t ) M ( t ) q ( t ) + M ( t ) M σ ( t ) ω σ ( t ) γ M ( t ) M σ ( t ) x ( t ) x σ ( t ) x γ σ ( t ) x γ ( t ) ω σ ( t ) .
(3.29)
Case 2. If γ 1 , then
ω ( t ) M ( t ) q ( t ) + M ( t ) M σ ( t ) ω σ ( t ) γ M ( t ) M σ ( t ) x ( t ) x ( t ) ω σ ( t ) .
(3.30)
Noting that x σ ( t ) x ( t ) , we have
ω ( t ) M ( t ) q ( t ) + M ( t ) M σ ( t ) ω σ ( t ) γ M ( t ) M σ ( t ) x ( t ) x σ ( t ) ω σ ( t ) .
(3.31)
By (3.12), we obtain
ω ( t ) M ( t ) q ( t ) + M ( t ) M σ ( t ) ω σ ( t ) γ M ( t ) M σ ( t ) ϑ 2 ( t , T ) r 1 ( t ) S n 1 γ ( t , x ( t ) ) x σ ( t ) ω σ ( t ) M ( t ) q ( t ) + M ( t ) M σ ( t ) ω σ ( t ) γ M ( t ) ( M σ ( t ) ) λ ϑ 2 ( t , T ) r 1 ( t ) ( ω σ ( t ) ) λ ,
(3.32)
where λ = 1 + 1 γ . Multiplying both sides of (3.32), with t replaced by s, by H ( t , s ) and integrating with respect to s from T to t ( t T ), one gets
T t H ( t , s ) M ( s ) q ( s ) s T t H ( t , s ) ω ( s ) s + T t H ( t , s ) M ( s ) M σ ( s ) ω σ ( s ) s T t γ H ( t , s ) M ( s ) ϑ 2 ( s , T ) ( M σ ( s ) ) λ r 1 ( s ) ( ω σ ( s ) ) λ s .
Integrating by parts and using (3.22) and (3.23), we have
T t H ( t , s ) M ( s ) q ( s ) s H ( t , T ) ω ( T ) + T t H s ( t , s ) ω σ ( s ) s + T t H ( t , s ) M ( s ) M σ ( s ) ω σ ( s ) s T t γ H ( t , s ) M ( s ) ϑ 2 ( s , T ) ( M σ ( s ) ) λ r 1 ( s ) ( ω σ ( s ) ) λ s H ( t , T ) ω ( T ) + T t [ h ( t , s ) M σ ( s ) ( M ( s ) H ( t , s ) ) γ γ + 1 ω σ ( s ) γ H ( t , s ) M ( s ) ϑ 2 ( s , T ) ( M σ ( s ) ) λ r 1 ( s ) ( ω σ ( s ) ) λ ] s H ( t , T ) ω ( T ) + T t [ h ( t , s ) M σ ( s ) ( M ( s ) H ( t , s ) ) 1 λ ω σ ( s ) γ H ( t , s ) M ( s ) ϑ 2 ( s , T ) ( M σ ( s ) ) λ r 1 ( s ) ( ω σ ( s ) ) λ ] s .
(3.33)
Write
A λ = γ H ( t , s ) M ( s ) ϑ 2 ( s , T ) r 1 ( s ) ( M σ ( s ) ) λ ( ω σ ( s ) ) λ , B λ 1 = h ( t , s ) r 1 1 λ ( s ) λ γ 1 λ ϑ 2 1 λ ( s , T ) .
It follows from Lemma 2.7 that
h ( t , s ) M σ ( s ) ( M ( s ) H ( t , s ) ) 1 λ ω σ ( s ) γ H ( t , s ) M ( s ) ϑ 2 ( s , T ) ( M σ ( s ) ) λ r 1 ( s ) ( ω σ ( s ) ) λ h γ + 1 ( t , s ) r 1 γ ( s ) ( γ + 1 ) γ + 1 ϑ 2 γ ( s , T ) .
Combining the above inequality with (3.33) gives
T t [ M ( s ) q ( s ) H ( t , s ) h γ + 1 ( t , s ) r 1 γ ( s ) ( γ + 1 ) γ + 1 ϑ 2 γ ( s , T ) ] s H ( t , T ) ω ( T ) ,
which implies
1 H ( t , T ) T t [ M ( s ) q ( s ) H ( t , s ) h γ + 1 ( t , s ) r 1 γ ( s ) ( γ + 1 ) γ + 1 ϑ 2 γ ( s , T ) ] s ω ( T ) ,

which contradicts assumption (3.24). Thus every solution x ( t ) of Eq. (1.3) is either oscillatory or tends to zero. The proof is completed. □

Theorem 3.3 Assume that (2.1) holds. Furthermore, suppose that for all sufficiently large T,
lim sup t ϑ 1 γ ( t , T ) t q ( s ) s > 1
(3.34)

holds. Then every solution x ( t ) of Eq. (1.3) is either oscillatory or tends to zero.

Proof Assume that Eq. (1.3) has a nonoscillatory solution x ( t ) on [ t 0 , ) T . Then, without loss of generality, there is a T t 0 , sufficiently large, such that x ( t ) > 0 for t T . By Lemma 2.4, there are two possible cases:
  1. (1)

    S i ( t , x ( t ) ) > 0 for any t T and 0 i n .

     
  2. (2)

    lim t x ( t ) = 0 .

     
If case (1) holds, then using the fact that S n ( t , x ( t ) ) < 0 , we obtain
S n ( t , x ( t ) ) t F ( s , x ( τ ( s ) ) ) s x γ ( t ) t q ( s ) s ,
which implies
t q ( s ) s ( S n 1 γ ( t , x ( t ) ) x ( t ) ) γ .
(3.35)
Combining (3.35) with (3.12) gives
ϑ 1 γ ( t , T ) t q ( s ) s 1 .
Therefore
lim sup t ϑ 1 γ ( t , T ) t q ( s ) s 1 ,

which contradicts assumption (3.34). Thus every solution x ( t ) of Eq. (1.3) is either oscillatory or tends to zero. The proof is completed. □

4 Examples

In this section, we give some examples to illustrate our main results.

Example 4.1 Consider the following higher-order dynamic equation:
S n ( t , x ( t ) ) + ρ t 4 3 x 3 ( τ ( t ) ) = 0 , t 2 Z , t 2 ,
(4.1)

where n 2 , γ = 3 , ρ is a positive constant, S k ( t , x ( t ) ) ( 0 k n ) are as in Eq. (1.3) with r n ( t ) = t 3 , r n 1 ( t ) = = r 1 ( t ) = 1 and τ is defined as in ( H 4 ). If ρ > 1 12 , then every solution of Eq. (4.1) is either oscillatory or tends to zero.

Proof Note that
t 0 t [ 1 r n ( s ) ] 1 γ s = 2 t 1 s s = log 2 t 1 ( t ) , t 0 s r i ( s ) = 2 s = for  1 i n 1
and
t 0 1 r n 1 ( s ) { s [ 1 r n ( u ) u q ( v ) v ] 1 γ u } s = 2 { s [ 1 u 3 u ρ v 4 3 v ] 1 3 u } s = ( ρ 1 2 1 3 ) 1 3 2 { s 1 u 10 9 u } s = ( ρ 1 2 1 3 ) 1 3 1 1 2 1 9 2 s 1 9 s = ( ρ 1 2 1 3 ) 1 3 1 1 2 1 9 1 2 8 9 1 lim t ( t 8 9 2 8 9 ) = .
Take M ( t ) = t , m ( t ) = 1 t 4 and G ( t , s ) = 1 if t > s 2 and G ( t , t ) = 0 if t 2 , then
ψ ( s , T ) = ρ s 1 3 + 1 σ ( s ) + 3 s η ( s , T ) σ 2 ( s ) , β ( s , T ) = 1 + 6 s η ( s , T ) σ ( s )
and
g ( t , s ) = 1 s ( 1 + 6 s η ( s , T ) σ ( s ) ) .
Note that ϑ n ( t , T ) = T t [ 1 r n ( s ) ] 1 γ s = T t 1 s s = log 2 t log 2 T . It is easy to see that
lim t ϑ 2 ( t , T ) = lim t ϑ 1 ( t , T ) = lim t ϑ n ( t , T ) = .
(4.2)
From (3.4) and (4.2), we can find T such that η ( t , T ) 1 for all t T . Therefore we have that if ρ > 1 12 , then
lim sup t 1 G ( t , T ) T t [ G ( t , s ) ψ ( s , T ) g 2 ( t , s ) r 1 ( s ) 4 γ η ( s , T ) ] s = lim sup t T t [ ρ s 1 3 1 12 s η ( s , T ) ] s ( ρ 1 12 ) lim sup t T t 1 s 1 3 s = .

Thus conditions ( H 3 ), (2.1) and (3.3) are satisfied. By Theorem 3.1, every solution of Eq. (4.1) is either oscillatory or tends to zero if ρ > 1 12 . The proof is completed. □

Example 4.2 Consider the following higher-order dynamic equation:
S n ( t , x ( t ) ) + ρ t 4 3 x 2 3 ( τ ( t ) ) = 0 , t 2 Z , t 2 ,
(4.3)

where n 2 , γ = 2 3 , S k ( t , x ( t ) ) ( 0 k n ) are as in Eq. (1.3) with r n ( t ) = t 1 2 , r n 1 ( t ) = t 1 4 , r n 2 ( t ) = = r 1 ( t ) = t , τ is defined as in ( H 4 ) and ρ is a positive constant. If ρ > 1 ( 5 3 ) 5 3 , then every solution of Eq. (4.3) is either oscillatory or tends to zero.

Proof Note that
t 0 t [ 1 r n ( s ) ] 1 γ s = 2 t 1 s 3 4 s = t 1 4 2 1 4 2 1 4 1 ( t ) , t 0 t 1 r n 1 ( s ) s = 2 t 1 s 1 4 s = t 3 4 2 3 4 2 3 4 1 ( t ) , t 0 t 1 r i ( s ) s = 2 t 1 s s = log 2 t 1 ( t )  for  1 i n 2
and
t 0 1 r n 1 ( s ) { s [ 1 r n ( u ) u q ( v ) v ] 1 γ u } s = 2 1 s 1 4 { s [ 1 u 1 2 u ρ v 4 3 v ] 3 2 u } s = ( ρ 1 2 1 3 ) 3 2 2 1 s 1 4 { s 1 u 5 4 u } s = ( ρ 1 2 1 3 ) 3 2 1 1 2 1 4 2 1 s 1 2 s = ( ρ 1 2 1 3 ) 3 2 1 1 2 1 4 lim t t 1 2 2 1 2 2 1 2 1 = .
Note that
ϑ 2 ( t , T ) = T t 1 r 2 ( u n 1 ) [ T u n 1 1 r 3 ( u n 2 ) [ [ T u 3 1 r n 1 ( u 2 ) × [ T u 2 1 r n ( u 1 ) u 1 ] 3 2 u 2 ] ] u n 2 ] u n 1 2 n 2 T t 1 u n 1 [ 2 n 3 T u n 1 1 u n 2 × [ [ 2 T u 3 [ 1 u 2 1 4 T u 2 1 u 1 1 2 u 1 ] 3 2 u 2 ] ] u n 2 ] u n 1 2 n 2 T t 1 u n 1 [ 2 n 3 T u n 1 1 u n 2 × [ [ 2 T u 3 [ 1 u 2 3 4 ( u 2 T ) ] 3 2 u 2 ] ] u n 2 ] u n 1 ( 1 2 ) n 1 2 ( t 2 n 2 T ) .
(4.4)
Pick T > T > 0 such that
1 t 1 3 1 t 1 2 1 [ ( 1 2 ) n 1 2 ( t 2 n 2 T ) ] 2 3 for  t T .
Take M ( t ) = t and H ( t , s ) = 1 for t > s 2 and H ( t , t ) = 0 for t 2 , then
h ( t , s ) = 1 s 2 5 .
Therefore we have that if ρ > 1 ( 5 3 ) 5 3 , then
lim sup t 1 H ( t , T ) T t [ M ( s ) q ( s ) H ( t , s ) h γ + 1 ( t , s ) r 1 γ ( s ) ( γ + 1 ) γ + 1 ϑ 2 γ ( s , T ) ] s = lim sup t T t [ ρ s 1 3 1 ( 5 3 ) 5 3 [ ( 1 2 ) n 1 2 ( s 2 n 2 T ) ] 2 3 ] s ( ρ 1 ( 5 3 ) 5 3 ) lim sup t T t 1 s 1 2 s = ( ρ 1 ( 5 3 ) 5 3 ) lim sup t t 1 2 ( T ) 1 2 2 1 2 1 = .

Thus conditions ( H 3 ), (2.1) and (3.24) are satisfied. By Theorem 3.2 every solution of Eq. (4.3) is either oscillatory or tends to zero if ρ > 1 ( 5 3 ) 5 3 . The proof is completed. □

Example 4.3 Consider the following higher order dynamic equation:
S n ( t , x ( t ) ) + ρ t σ ( t ) x γ ( τ ( t ) ) = 0
(4.5)

on an arbitrary time scale T, where n 2 , γ 1 is the quotient of two odd positive integers, ρ is a positive constant, S k ( t , x ( t ) ) ( 0 k n ) are as in Eq. (1.3) with r n ( t ) = 1 , r n 1 ( t ) = t 1 γ , r n 2 ( t ) = = r 1 ( t ) = t and τ is defined as in ( H 4 ). If ρ > 2 ( n 1 ) γ + 1 , then every solution of Eq. (4.5) is either oscillatory or tends to zero.

Proof Note that
t 0 [ 1 r n ( s ) ] 1 γ s = t 0 s = , t 0 1 r n 1 ( s ) s = t 0 1 s 1 γ s =
and
t 0 1 r i ( s ) s = t 0 1 s s = for  1 i n 2 .
Pick that t t 0 such that t 0 t 1 s 1 γ s > 0 , then
t 0 1 r n 1 ( s ) { s [ 1 r n ( u ) u q ( v ) v ] 1 γ u } s = t 0 1 s 1 γ { s [ u ρ v σ ( v ) v ] 1 γ u } s ( ρ ) 1 γ t 0 1 s 1 γ { s 1 u 1 γ u } s ( ρ ) 1 γ t 0 t 1 s 1 γ s s 1 u 1 γ u = .
Using arguments similar to that of (4.4), it is easy to see that ϑ 1 ( t , T ) ( 1 2 ) n 1 + 1 γ ( t 2 n 1 T ) . Therefore we have that if ρ > 2 ( n 1 ) γ + 1 , then
lim sup t ϑ 1 γ ( t , T ) t q ( s ) s ρ ( 1 2 ) ( n 1 ) γ + 1 lim sup t ( t 2 n 1 T ) γ t ρ ( 1 2 ) ( n 1 ) γ + 1 > 1 .

Thus conditions ( H 3 ), (2.1) and (3.34) are satisfied. By Theorem 3.3 every solution of Eq. (4.5) is either oscillatory or tends to zero if ρ > 2 ( n 1 ) γ + 1 . The proof is completed. □

Example 4.4 Consider the following third-order dynamic equation:
[ ( t x ( t ) ) ] + 3 t [ ( 4 t 2 + 18 t + 19 ) ( t + 1 ) + ( 4 t 2 + 10 t + 5 ) ( t + 3 ) ] ( t + 1 ) ( t + 2 ) ( t + 3 ) x ( 3 t ) = 0
(4.6)

on N = { 1 , 2 , 3 , } , where n = 2 , γ = 1 , r 2 ( t ) = 1 , r 1 ( t ) = t and τ ( t ) = 3 t for any t N . It is easy to see that conditions ( H 1 )-( H 5 ) are satisfied and x ( t ) = ( 1 ) t t is an oscillatory solution of Eq. (4.6), which tends to zero as t .

Declarations

Acknowledgements

The authors express their sincere gratitude to the referees for their valuable suggestions and comments. This paper is project is supported by NNSF of China (11261005) and NSF of Guangxi (2011GXNSFA018135, 2012GXNSFDA276040) and SF of ED of Guangxi (2013ZD061).

Authors’ Affiliations

(1)
College of Mathematics and Information Science, Guangxi University, Nanning, Guangxi, China
(2)
Department of Mathematics, Guangxi College of Finance and Economics, Nanning, Guangxi, China

References

  1. Hilger S: Analysis on measure chains - a unified approach to continuous and discrete calculus. Results Math. 1990, 18: 18–56. 10.1007/BF03323153MathSciNetView ArticleGoogle Scholar
  2. Kac V, Chueng P Universitext. Quantum Calculus 2002.View ArticleGoogle Scholar
  3. Agarwal RP: Difference Equations and Inequalities. Theory, Methods and Applications. 2nd edition. Dekker, New York; 2000.Google Scholar
  4. Agarwal RP, Bohner M, Saker SH: Oscillation of second order delay dynamic equations. Can. Appl. Math. Q. 2005, 13: 1–17.MathSciNetGoogle Scholar
  5. Bohner M, Karpuz B, Ocalan O: Iterated oscillation criteria for delay dynamic equations of first order. Adv. Differ. Equ. 2008., 2008: Article ID 458687Google Scholar
  6. Bohner M, Peterson A: Advances in Dynamic Equations on Time Scales. Birkhäuser, Boston; 2003.View ArticleGoogle Scholar
  7. Bohner M, Saker SH: Oscillation of second order nonlinear dynamic equations on time scales. Rocky Mt. J. Math. 2004, 34: 1239–1254. 10.1216/rmjm/1181069797MathSciNetView ArticleGoogle Scholar
  8. Erbe L: Oscillation results for second-order linear equations on a time scale. J. Differ. Equ. Appl. 2002, 8: 1061–1071. 10.1080/10236190290015317MathSciNetView ArticleGoogle Scholar
  9. Erbe L, Peterson A, Saker SH: Oscillation criteria for second-order nonlinear delay dynamic equations. J. Math. Anal. Appl. 2007, 333: 505–522. 10.1016/j.jmaa.2006.10.055MathSciNetView ArticleGoogle Scholar
  10. Grace SR, Agarwal RP, Kaymakcalan B, Sae-Jie W: On the oscillation of certain second order nonlinear dynamic equations. Math. Comput. Model. 2009, 50: 273–286. 10.1016/j.mcm.2008.12.007MathSciNetView ArticleGoogle Scholar
  11. Hardy GH, Littlewood JE, Polya G: Inequalities. 2nd edition. Cambridge University Press, Cambridge; 1988.Google Scholar
  12. Hassan TS: Oscillation criteria for half-linear dynamic equations on time scales. J. Math. Anal. Appl. 2008, 345: 176–185. 10.1016/j.jmaa.2008.04.019MathSciNetView ArticleGoogle Scholar
  13. Han Z, Sun S, Shi B: Oscillation criteria for a class of second-order Emden-Fowler delay dynamic equations on time scales. J. Math. Anal. Appl. 2007, 334: 847–858. 10.1016/j.jmaa.2007.01.004MathSciNetView ArticleGoogle Scholar
  14. Han Z, Shi B, Sun S: Oscillation criteria for second-order delay dynamic equations on time scales. Adv. Differ. Equ. 2007., 2007: Article ID 70730Google Scholar
  15. Sun T, Xi H, Peng X: Asymptotic behavior of solutions of higher-order dynamic equations on time scales. Adv. Differ. Equ. 2011., 2011: Article ID 237219Google Scholar
  16. Sun T, Xi H, Peng X, Yu W: Nonoscillatory solutions for higher-order neutral dynamic equations on time scales. Abstr. Appl. Anal. 2010., 2010: Article ID 428963Google Scholar
  17. Sun T, Xi H, Yu W: Asymptotic behaviors of higher order nonlinear dynamic equations on time scales. J. Appl. Math. Comput. 2011, 37: 177–192. 10.1007/s12190-010-0428-1MathSciNetView ArticleGoogle Scholar
  18. Wang Y, Xu Z: Asymptotic properties of solutions of certain third-order dynamic equations. J. Comput. Appl. Math. 2012, 236: 2354–2366. 10.1016/j.cam.2011.11.021MathSciNetView ArticleGoogle Scholar
  19. Erbe L, Peterson A, Saker SH: Asymptotic behavior of solutions of a third-order nonlinear dynamic equation on time scales. J. Comput. Appl. Math. 2005, 181: 92–102. 10.1016/j.cam.2004.11.021MathSciNetView ArticleGoogle Scholar
  20. Erbe L, Peterson A, Saker SH: Oscillation and asymptotic behavior a third-order nonlinear dynamic equation. Can. Appl. Math. Q. 2006, 14: 129–147.MathSciNetGoogle Scholar
  21. Erbe L, Peterson A, Saker SH: Hille and Nehari type criteria for third order dynamic equations. J. Math. Anal. Appl. 2007, 329: 112–131. 10.1016/j.jmaa.2006.06.033MathSciNetView ArticleGoogle Scholar
  22. Hassan TS: Oscillation of third order nonlinear delay dynamic equations on time scales. Math. Comput. Model. 2009, 49: 1573–1586. 10.1016/j.mcm.2008.12.011View ArticleGoogle Scholar
  23. Hassan TS: Kamenev-type oscillation criteria for second order nonlinear dynamic equations on time scales. Appl. Math. Comput. 2011, 217: 5285–5297. 10.1016/j.amc.2010.11.052MathSciNetView ArticleGoogle Scholar
  24. Sun T, Yu W, Xi H: Oscillatory behavior and comparison for higher order nonlinear dynamic equations on time scales. J. Appl. Math. Inf. 2012, 30: 289–304.MathSciNetGoogle Scholar
  25. Bohner M, Peterson A: Dynamic Equations on Time Scales: An Introduction with Applications. Birkhäuser, Boston; 2001.View ArticleGoogle Scholar

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© Wu et al.; licensee Springer. 2013

This article is published under license to BioMed Central Ltd. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/2.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

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