1 Introduction

In 2006, Luo and Ma [1] considered the second-order dynamic boundary value problem on time scales

u Δ 2 ( t ) + f ˆ ( u σ ( t ) ) = 0 , t [ 0 , 1 ] T , u ( 0 ) = u ( 1 ) = 0 ,
(1.1)

where f ˆ C([0,),(0,)). They proved that (1.1) has at least one positive solution if either

f ˆ 0 < μ 1 < f ˆ
(1.2)

or

f ˆ < μ 1 < f ˆ 0 ,
(1.3)

where

f ˆ 0 = lim s 0 + f ˆ ( s ) s , f ˆ = lim s f ˆ ( s ) s

and μ 1 is the first eigenvalue of the linear problem

u Δ 2 (t)+μ u σ (t)=0,u(0)=u(1)=0.

Notice that conditions (1.2) and (1.3) are optimal! Inspired by this paper, we have a natural question if we could establish some optimal results for the fourth-order dynamic boundary value problem

u Δ 4 ( t ) = f ( t , u ( t ) , u Δ 2 ( t ) ) , t [ 0 , ρ 2 ( T ) ] T , u ( 0 ) = u ( σ 2 ( T ) ) = u Δ 2 ( 0 ) = u Δ 2 ( T ) = 0 ,
(1.4)

where T is a time scale and 0,TT, 0<ρ(T), f: [ 0 , ρ ( T ) ] T ×[0,)×(,0][0,) is continuous. To the best of our knowledge, few papers can be found to study such a problem in the literature. Wang and Sun [2] and Luo and Gao [3] applied the Schauder fixed point theorem to show the existence of positive solutions of a fourth-order dynamic boundary value problem under different boundary value conditions. However, the key conditions in these two papers are not directly related to the first eigenvalue of the associated linear eigenvalue problems.

For the continuous cases, Ma and Xu [4] discussed

u ( 4 ) ( x ) = g ( x , u ( x ) , u ( x ) ) , x ( 0 , 1 ) , u ( 0 ) = u ( 1 ) = u ( 0 ) = u ( 1 ) = 0 ,

where g:[0,1]×[0,)×(,0][0,) is continuous. And for the discrete cases, there exists no work corresponding exactly to the continuous cases, but we can refer the reader to Xu, Gao and Ma [5] and Ma and Gao [6] and Gao and Xu [7] for the similar discussions. Moreover, nothing is known about the time scales extension analog (1.4) except for [8] for second-order dynamic equations. The likely reason is that few properties of the associated linear eigenvalue problem

u Δ 4 ( t ) + λ [ B ( t ) u Δ 2 ( t ) A ( t ) u ( t ) ] = 0 , t [ 0 , ρ 2 ( T ) ] T , u ( 0 ) = u ( σ 2 ( T ) ) = u Δ 2 ( 0 ) = u Δ 2 ( T ) = 0
(1.5)

are known.

In this paper, we establish spectrum properties of (1.5) in Section 2 and use the global bifurcation techniques on time scales (see Davidson and Rynne [[9], Theorem 7.1] or Luo and Ma [1]) to discuss the existence of positive solutions for problem (1.4) in Section 3. Our existence result is related to the first eigenvalue of the associated linear eigenvalue problem (1.5) and thus should be optimal.

For convenience, here we will not introduce the concepts and notations about time scale. The reader is referred to [10, 11] or most of the time-scales-related papers for details.

2 Generalized eigenvalues

For a compact interval [ a , b ] T , C [ a , b ] T is a Banach space with the norm

y [ a , b ] T =sup { | y ( t ) | t [ a , b ] T } .

For hC [ 0 , ρ ( T ) ] T , let us consider the linear problem

u Δ 4 ( t ) = h ( t ) , t [ 0 , ρ 2 ( T ) ] T , u ( 0 ) = u ( σ 2 ( T ) ) = u Δ 2 ( 0 ) = u Δ 2 ( T ) = 0 .
(2.1)

Let u Δ 2 (t)=y(t) for t [ 0 , T ] T . Then

y Δ 2 ( t ) = h ( t ) , t [ 0 , ρ 2 ( T ) ] T , y ( 0 ) = y ( T ) = 0 .

Consequently,

y(t)= 0 ρ ( T ) H 1 (t,s)h(s)Δs,t [ 0 , T ] T ,
(2.2)

where

H 1 (t,s)= 1 T { t ( T σ ( s ) ) , t s , σ ( s ) ( T t ) , σ ( s ) t .
(2.3)

Now, (2.1) is equivalent to

u Δ 2 ( t ) = y ( t ) , t [ 0 , T ] T , u ( 0 ) = u ( σ 2 ( T ) ) = 0 .

Consequently again,

u(t)= 0 σ ( T ) H(t,s)y(s)Δs,t [ 0 , σ 2 ( T ) ] T ,
(2.4)

where

H(t,s)= 1 σ 2 ( T ) { t ( σ 2 ( T ) σ ( s ) ) , t s , σ ( s ) ( σ 2 ( T ) t ) , σ ( s ) t .
(2.5)

And we can easily check that

H(t,s) H 1 (t,s),t [ 0 , T ] T ,s [ 0 , ρ ( T ) ] T .
(2.6)

To sum up, we have proved the following.

Lemma 2.1 For each hC [ 0 , ρ 2 ( T ) ] T , problem (2.1) has a unique solution

u(t)= 0 σ ( T ) H(t,s) 0 ρ ( T ) H 1 (s,τ)h(τ)ΔτΔs,t [ 0 , σ 2 ( T ) ] T .
(2.7)

Let 0<l< l ˜ <1: sin l ( σ 2 (T),0)=0, sin l ˜ (T,0)=0. Then e(t)= sin l (t,0) solves the problem

e Δ 2 ( t ) + l e ( t ) = 0 , t [ 0 , T ] T , e ( 0 ) = e ( σ 2 ( T ) ) = 0
(2.8)

and e ˜ (t)= sin l ˜ (t,0) solves the problem

e ˜ Δ 2 ( t ) + l ˜ e ˜ ( t ) = 0 , t [ 0 , ρ 2 ( T ) ] T , e ˜ ( 0 ) = e ˜ ( T ) = 0
(2.9)

from [[10], pp.92-93].

Remark 2.1

sin l ( t , 0 ) = e i l ( t , 0 ) e i l ( t , 0 ) 2 i ; sin l ˜ ( t , 0 ) = e i l ˜ ( t , 0 ) e i l ˜ ( t , 0 ) 2 i ; e p ( t , s ) = exp ( s t ξ μ ( τ ) ( p ( τ ) ) Δ τ ) ; ξ h ( z ) = { 1 h Log ( 1 + z h ) = 1 h [ log | 1 + z h | + i arg ( 1 + z h ) ] , h > 0 , z , h = 0 .

It is clear that

e(t)>0,t ( 0 , σ 2 ( T ) ) T , e ˜ (t)>0,t ( 0 , T ) T
(2.10)

and so there exist ϵ 1 , ϵ 2 >0 such that

e ˜ (t) ϵ 1 e(t),t [ 0 , ρ ( T ) ] ,
(2.11)
e(t) ϵ 2 e ˜ (t),t [ 0 , ρ ( T ) ] .
(2.12)

Remark 2.2 (2.11) holds for any time scale T with 0,TT, but (2.12) does not hold for the case of T:ρ(T)=T<σ(T), i.e., T is an left-dense and right-scattered point (abbreviated to ldrs point) of the time scale T.

Let

X= { u C 2 [ 0 , σ 2 ( T ) ] T | u ( 0 ) = u ( σ 2 ( T ) ) = u Δ 2 ( 0 ) = u Δ 2 ( T ) = 0 ; γ ( 0 , ) γ e ˜ ( t ) u Δ 2 ( t ) γ e ˜ ( t )  for  t [ 0 , T ] T ; δ ( 0 , ) δ e ( t ) u ( t ) δ e ( t )  for  t [ 0 , σ 2 ( T ) ] T }

and define the norm of uX by

u X :=inf { | ( γ , δ ) | | γ e ˜ ( t ) u Δ 2 ( t ) γ e ˜ ( t )  for  t [ 0 , T ] T ; δ e ( t ) u ( t ) δ e ( t )  for  t [ 0 , σ 2 ( T ) ] T } ,
(2.13)

where |(γ,δ)|= γ 2 + δ 2 . It is easy to check that (X, X ) is a Banach space. Let

P:= { u X u Δ 2 ( t ) 0  for  t [ 0 , T ] T ; u ( t ) 0  for  t [ 0 , σ 2 ( T ) ] T } .

Then the cone P is normal and has nonempty interiors intP.

Lemma 2.2 For uX,

u C [ 0 , σ 2 ( T ) ] T q u X , u Δ 2 C [ 0 , T ] T q u X ,
(2.14)

where q:=max{ e C [ 0 , σ 2 ( T ) ] T , e ˜ C [ 0 , T ] T }.

Proof Since uX, there exist δ(0,): δe(t)u(t)δe(t), t [ 0 , σ 2 ( T ) ] T and γ(0,): γ e ˜ (t) u Δ 2 (t)γ e ˜ (t), t [ 0 , T ] T , we have

u C [ 0 , σ 2 ( T ) ] T δ e C [ 0 , σ 2 ( T ) ] T | ( γ , δ ) | e C [ 0 , σ 2 ( T ) ] T

and

u Δ 2 C [ 0 , T ] T γ e ˜ C [ 0 , T ] T | ( γ , δ ) | e ˜ C [ 0 , T ] T .

Thus

u C [ 0 , σ 2 ( T ) ] T e C [ 0 , σ 2 ( T ) ] T u X q u X , u Δ 2 C [ 0 , T ] T e ˜ C [ 0 , T ] T u X q u X .

 □

Let us make the assumption

(H0) A,BC( [ 0 , ρ ( T ) ] T ,[0,)) with A(t)>0 or B(t)>0 on [ 0 , ρ ( T ) ] T .

Define a linear operator G:X C 4 [ 0 , σ 2 ( T ) ] T by

G u ( t ) : = 0 σ ( T ) H ( t , s ) 0 ρ ( T ) H 1 ( s , τ ) [ A ( τ ) u ( τ ) B ( τ ) u Δ 2 ( τ ) ] Δ τ Δ s , t [ 0 , σ 2 ( T ) ] T .
(2.15)

Then (1.5) is equivalent to

u(t)=λGu(t),t [ 0 , σ 2 ( T ) ] T .

Definition 2.1 We say λ is an eigenvalue of the linear problem

u Δ 4 ( t ) + λ [ B ( t ) u Δ 2 ( t ) A ( t ) u ( t ) ] = 0 , t [ 0 , ρ 2 ( T ) ] T , u ( 0 ) = u ( σ 2 ( T ) ) = u Δ 2 ( 0 ) = u Δ 2 ( T ) = 0
(2.16)

if (2.16) has nontrivial solutions.

Theorem 2.1 Let (H0) hold and T be not an ldrs point of the time scale T. Then

  1. (1)

    G(P)P, and G:PP is strongly positive;

  2. (2)

    Problem (1.5) has an algebraically simple eigenvalue, λ 1 (A,B)= ( r ( G ) ) 1 , with a nonnegative eigenfunction φ 1 ()intP;

  3. (3)

    There is no other eigenvalue with a nonnegative eigenfunction.

Proof We prove G:XX firstly.

For uX, we have

δ e ( t ) u ( t ) δ e ( t ) , t [ 0 , σ 2 ( T ) ] T and γ e ˜ ( t ) u Δ 2 ( t ) γ e ˜ ( t ) , t [ 0 , T ] T

for some positive δ and γ. From (2.15), the condition (H0), (2.11) and (2.12), we have

( G u ) ( t ) = 0 σ ( T ) H ( t , s ) 0 ρ ( T ) H 1 ( s , τ ) [ A ( τ ) u ( τ ) B ( τ ) u Δ 2 ( τ ) ] Δ τ Δ s 0 σ ( T ) H ( t , s ) 0 ρ ( T ) H 1 ( s , τ ) [ δ A ( τ ) e ( τ ) + γ B ( τ ) e ˜ ( τ ) ] Δ τ Δ s 0 σ ( T ) H ( t , s ) 0 ρ ( T ) H 1 ( s , τ ) [ ϵ 2 δ A ( τ ) + γ B ( τ ) ] e ˜ ( τ ) Δ τ Δ s [ ϵ 2 δ A C [ 0 , ρ ( T ) ] T + γ B C [ 0 , ρ ( T ) ] T ] 0 σ ( T ) H ( t , s ) 0 ρ ( T ) H 1 ( s , τ ) e ˜ ( τ ) Δ τ Δ s 1 l ˜ [ ϵ 2 δ A C [ 0 , ρ ( T ) ] T + γ B C [ 0 , ρ ( T ) ] T ] 0 σ ( T ) H ( t , s ) ϵ 1 e ( s ) Δ s = ϵ 1 l l ˜ [ ϵ 2 δ A C [ 0 , ρ ( T ) ] T + γ B C [ 0 , ρ ( T ) ] T ] e ( t ) .
(2.17)

By (2.15), the condition (H0) and (2.12), we have

( G u ) Δ 2 ( t ) = 0 ρ ( T ) H 1 ( t , τ ) [ A ( τ ) u ( τ ) B ( τ ) u Δ 2 ( τ ) ] Δ τ 0 ρ ( T ) H 1 ( t , τ ) [ δ A ( τ ) e ( τ ) + γ B ( τ ) e ˜ ( τ ) ] Δ τ 0 ρ ( T ) H 1 ( t , τ ) [ ϵ 2 δ A ( τ ) + γ B ( τ ) ] e ˜ ( τ ) Δ τ [ ϵ 2 δ A C [ 0 , ρ ( T ) ] T + γ B C [ 0 , ρ ( T ) ] T ] 0 ρ ( T ) H 1 ( t , τ ) e ˜ ( τ ) Δ τ = 1 l ˜ [ ϵ 2 δ A C [ 0 , ρ ( T ) ] T + γ B C [ 0 , ρ ( T ) ] T ] e ˜ ( t ) .
(2.18)

Similarly, we get

(Gu)(t) ϵ 1 l l ˜ [ ϵ 2 δ A C [ 0 , ρ ( T ) ] T + γ B C [ 0 , ρ ( T ) ] T ] e(t)
(2.19)

and

( G u ) Δ 2 (t) 1 l ˜ [ ϵ 2 δ A C [ 0 , ρ ( T ) ] T + γ B C [ 0 , ρ ( T ) ] T ] e ˜ (t).
(2.20)

Thus G:XX. Furthermore, since G(X) C 4 [ 0 , σ 2 ( T ) ] T XX, we have that G:XX is compact.

Next, we show that G:PP is strongly positive.

For uP{0}, if A(t)>0 on [ 0 , ρ ( T ) ] T , then A(t)k on [ 0 , ρ ( T ) ] T for some constant k>0, and subsequently,

G u ( t ) = 0 σ ( T ) H ( t , s ) 0 ρ ( T ) H 1 ( s , τ ) [ A ( τ ) u ( τ ) B ( τ ) u Δ 2 ( τ ) ] Δ τ Δ s k 0 σ ( T ) H ( t , s ) 0 ρ ( T ) H 1 ( s , τ ) u ( τ ) Δ τ Δ s = : ( G 1 u ) ( t ) , t [ 0 , σ 2 ( T ) ] T .

Since ( G 1 u)(0)=( G 1 u)( σ 2 (T))=0 and

( G 1 u ) Δ 2 (t)=k 0 ρ ( T ) H 1 (t,τ)u(τ)Δτ>0,t ( 0 , T ) T ,

it follows that there exists r>0 such that G 1 u(t)re(t) on [ 0 , σ 2 ( T ) ] T . Thus

Gu(t)re(t),t [ 0 , σ 2 ( T ) ] T .
(2.21)

If B(t)>0 on [ 0 , ρ ( T ) ] T , then B(t) k 1 on [ 0 , ρ ( T ) ] T for some constant k 1 >0, and subsequently,

G u ( t ) k 1 0 σ ( T ) H ( t , s ) 0 ρ ( T ) H 1 ( s , τ ) [ u Δ 2 ( τ ) ] Δ τ Δ s = k 1 0 σ ( T ) H ( t , s ) u ( s ) Δ s = : ( G 2 u ) ( t ) , t [ 0 , σ 2 ( T ) ] T .

Then there exists r 1 >0 such that G 2 u(t) r 1 e(t) on [ 0 , σ 2 ( T ) ] T . So,

Gu(t) r 1 e(t),t [ 0 , σ 2 ( T ) ] T .
(2.22)

Similarly, for any uP{0}, if A(t)>0 on [ 0 , ρ ( T ) ] T , then there exists r 2 >0 such that for t [ 0 , T ] T ,

( G u ) Δ 2 ( t ) = 0 ρ ( T ) H 1 ( t , τ ) [ A ( τ ) u ( τ ) B ( τ ) u Δ 2 ( τ ) ] Δ τ 0 ρ ( T ) H 1 ( t , τ ) A ( τ ) u ( τ ) Δ τ k 0 ρ ( T ) H 1 ( t , τ ) u ( τ ) Δ τ r 2 e ˜ ( t ) .
(2.23)

If B(t)>0 on [ 0 , ρ ( T ) ] T , then there exists r 3 >0 such that for t [ 0 , T ] T ,

( G u ) Δ 2 ( t ) 0 ρ ( T ) H 1 ( t , τ ) [ B ( τ ) u Δ 2 ( τ ) ] Δ τ k 1 0 ρ ( T ) H 1 ( t , τ ) [ u Δ 2 ( τ ) ] Δ τ r 3 e ˜ ( t ) .
(2.24)

It follows from (2.21)-(2.24) that GuintP.

Now, by the Krein-Rutman theorem ([[12], Theorem 7.C] or [[13], Theorem 19.3]), G has an algebraically simple eigenvalue λ 1 (A,B) with an eigenfunction φ 1 ()intP. Moreover, there is no other eigenvalue with a nonnegative eigenfunction. □

3 The main result

In this section, we will make the following assumptions:

(H1) T is not an ldrs point of the time scale T.

(H2) f: [ 0 , ρ ( T ) ] T ×[0,)×(,0][0,) is continuous and there exist functions a,b,c,dC( [ 0 , ρ ( T ) ] T ,[0,)) with a(t)+b(t)>0 and c(t)+d(t)>0 on [ 0 , ρ ( T ) ] T such that

f(t,u,p)=a(t)ub(t)p+o ( | ( u , p ) | ) as  | ( u , p ) | (0,0)

uniformly for t [ 0 , ρ ( T ) ] T , and

f(t,u,p)=c(t)ud(t)p+o ( | ( u , p ) | ) as  | ( u , p ) |

uniformly for t [ 0 , ρ ( T ) ] T . Here

| ( u , p ) | := u 2 + p 2 .

(H3) f(t,u,p)>0 for t [ 0 , ρ ( T ) ] T and (u,p)([0,)×(,0]){(0,0)}.

(H4) There exist functions a 0 : [ 0 , ρ ( T ) ] T [0,) and b 0 C( [ 0 , ρ ( T ) ] T ,(0,)) such that

f(t,u,p) a 0 (t)u b 0 (t)p,(t,u,p) [ 0 , ρ ( T ) ] T ×[0,)×(,0].

Theorem 3.1 Let (H1)-(H4) hold. Assume that either

λ 1 (c,d)<1< λ 1 (a,b)
(3.1)

or

λ 1 (a,b)<1< λ 1 (c,d).
(3.2)

Then problem (1.4) has at least one positive solution.

Denote L:D(L)C [ 0 , σ 2 ( T ) ] T by setting

(Lu)(t):= u Δ 4 (t),uD(L),t [ 0 , ρ 2 ( T ) ] T ,
(3.3)

where

D(L)= { u C 4 [ 0 , σ 2 ( T ) ] T u ( 0 ) = u ( σ 2 ( T ) ) = u Δ 2 ( 0 ) = u Δ 2 ( T ) = 0 } .
(3.4)

From [[9], Lemma 3.7] and standard properties of compact linear operators, we can get that L 1 :C [ 0 , σ 2 ( T ) ] T C 1 [ 0 , σ ( T ) ] T is compact.

Let ζ,ξ: [ 0 , ρ ( T ) ] T ×[0,)×(,0]R be continuous and satisfy

f(t,u,p)=a(t)ub(t)p+ζ(t,u,p),
(3.5)
f(t,u,p)=c(t)ud(t)p+ξ(t,u,p).
(3.6)

Obviously, (H2) implies that

lim | ( u , p ) | 0 ζ ( t , u , p ) | ( u , p ) | =0uniformly for t [ 0 , ρ ( T ) ] T ,
(3.7)
lim | ( u , p ) | ξ ( t , u , p ) | ( u , p ) | =0uniformly for t [ 0 , ρ ( T ) ] T .
(3.8)

Let

ξ ˜ (r)=max { | ξ ( t , u , p ) | 0 | ( u , p ) | r , t [ 0 , ρ ( T ) ] T } .
(3.9)

Then ξ ˜ is nondecreasing and

lim r ξ ˜ ( r ) r =0.
(3.10)

Next we consider

(Lu)(t)=λ [ a ( t ) u ( t ) b ( t ) u Δ 2 ( t ) ] +λζ ( t , u ( t ) , u Δ 2 ( t ) ) ,λ>0,
(3.11)

as a bifurcation problem from the trivial solution u0. It is easy to check that (3.11) can be converted to the equivalent equation

u ( t ) = λ { 0 σ ( T ) H ( t , s ) 0 ρ ( T ) H 1 ( s , τ ) [ a ( τ ) u ( τ ) b ( τ ) u Δ 2 ( τ ) ] Δ τ Δ s } + λ { 0 σ ( T ) H ( t , s ) 0 ρ ( T ) H 1 ( s , τ ) ζ ( τ , u ( τ ) , u Δ 2 ( τ ) ) Δ τ Δ s } = : R ( λ , u ) ( t ) .
(3.12)

From Theorem 2.1, we have that for each fixed λ>0, the operator G ˆ :PP,

G ˆ u(t):= 0 σ ( T ) H(t,s) 0 ρ ( T ) H 1 (s,τ) [ a ( τ ) u ( τ ) b ( τ ) u Δ 2 ( τ ) ] ΔτΔs,
(3.13)

is compact and strongly positive. Define F:[0,)×XX by

F(λ,u):=λ 0 σ ( T ) H(t,s) 0 ρ ( T ) H 1 (s,τ)ζ ( τ , u ( τ ) , u Δ 2 ( τ ) ) ΔτΔs.
(3.14)

Then we have from (3.7) and Lemma 2.2 that

F ( λ , u ) X =o ( u X ) as  u X 0
(3.15)

locally uniformly in λ. Now, we have from Davidson and Rynne [[9], Theorem 7.1], or Luo and Ma [1], to conclude that there exists an unbounded connected subset C in the set

{ ( λ , u ) [ 0 , ) × P u = λ G ˆ u + F ( λ , u ) , u int P } { ( λ 1 ( a , b ) , 0 ) }

such that ( λ 1 (a,b),0)C.

Proof of Theorem 3.1 It is clear that any solution of (3.11) of the form (1,u) yields a solution u of (1.4). We will show that C crosses the hyperplane {1}×X in R×X. To do this, it is enough to show that C joins ( λ 1 (a,b),0) to ( λ 1 (c,d),). Let ( η n , y n )C satisfy

η n + y n X .
(3.16)

We note that η n >0 for all nN since (0,0) is the only solution of (3.11) for λ=0 and C({0}×X)=.

Case 1. λ 1 (c,d)<1< λ 1 (a,b).

In this case, we show that

( λ 1 ( c , d ) , λ 1 ( a , b ) ) { λ R ( λ , u ) C } .

We divide the proof into two steps.

Step 1. We show that if there exists a constant number M>0 such that

η n (0,M],
(3.17)

then C joins ( λ 1 (a,b),0) to ( λ 1 (c,d),).

If (3.17) holds, we have that y n X . We divide the equation

L y n (t)= η n [ c ( t ) y n ( t ) d ( t ) y n Δ 2 ( t ) ] + η n ξ ( t , y n ( t ) , y n Δ 2 ( t ) ) ,t [ 0 , ρ 2 ( T ) ] T
(3.18)

by y n X and set y ¯ n = y n y n X . Since y ¯ n is bounded in X, choosing a subsequence and relabeling if necessary, we see that y ¯ n y ¯ for some y ¯ X with y ¯ X =1. Moreover, from Lemma 2.2, we have

| ξ ( t , y n ( t ) , y n Δ 2 ( t ) ) | y n X ξ ˜ ( 2 q y n X ) y n X

and from (3.10),

lim n | ξ ( t , y n ( t ) , y n Δ 2 ( t ) ) | y n X =0.

Thus

y ¯ (t):= 0 σ ( T ) H(t,s) 0 ρ ( T ) H 1 (s,τ) η ¯ [ c ( τ ) y ¯ ( τ ) d ( τ ) y ¯ Δ 2 ( τ ) ] ΔτΔs,

where η ¯ := lim n η n , again choosing a subsequence and relabeling if necessary. Therefore,

L y ¯ (t)= η ¯ [ c ( t ) y ¯ ( t ) d ( t ) y ¯ Δ 2 ( t ) ] ,t [ 0 , ρ 2 ( T ) ] T .

This together with Theorem 2.1 yields η ¯ = λ 1 (c,d). Thus C joins ( λ 1 (a,b),0) to ( λ 1 (c,d),).

Step 2. We show that there exists a constant M such that η n (0,M] for all n.

Since ( y n , η n )C, we have

L y n = η n f ( t , y n , y n Δ 2 ) .

Therefore from (H4), we get

y n ( t ) = η n 0 σ ( T ) H ( t , s ) 0 ρ ( T ) H 1 ( s , τ ) f ( τ , y n ( τ ) , y n Δ 2 ( τ ) ) Δ τ Δ s η n 0 σ ( T ) H ( t , s ) 0 ρ ( T ) H 1 ( s , τ ) [ a 0 ( t ) y n ( τ ) b 0 ( t ) y n Δ 2 ( τ ) ] Δ τ Δ s η n b 0 σ ( T ) H ( t , s ) 0 ρ ( T ) H 1 ( s , τ ) [ y n Δ 2 ( τ ) ] Δ τ Δ s = η n b 0 σ ( T ) H ( t , s ) y n ( s ) Δ s ,
(3.19)

where b = min t [ 0 , ρ ( T ) ] T b 0 (t)>0. Set v n (t)= 0 σ ( T ) H(t,s) y n (s)Δs, we have v n Δ 2 (t)= y n (t), t [ 0 , σ 2 ( T ) ] T , v n (0)= v n ( σ 2 (T))=0 and

v n Δ 2 (t) η n b v n (t).

Furthermore,

v n (t)>0,t [ α , β ] T .

From y n (t)0, t [ 0 , σ 2 ( T ) ] T . Now we can obtain η n (0,M], ∀n for some positive constant M according to [[1], Lemma 2.2].

Case 2. λ 1 (a,b)<1< λ 1 (c,d).

According to Step 2 of Case 1, we have

η n (0,M],nN

for some M>0. Then if ( η n , y n )C is such that

lim n ( η n + y n X ) =,

applying a similar argument to that used in Step 1 of Case 1, after taking a subsequence and relabeling if necessary, it follows that

( η n , y n ) ( λ 1 ( c , d ) , ) ,n.

Again C joins ( λ 1 (a,b),0) to ( λ 1 (c,d),) and the result follows. □