Open Access

Structure of positive solution sets of differential boundary value problems

Boundary Value Problems20132013:100

DOI: 10.1186/1687-2770-2013-100

Received: 26 September 2012

Accepted: 8 March 2013

Published: 22 April 2013

Abstract

In this paper, we first obtain some results on the structure of positive solution sets of differential boundary value problems. Then by using the results, we obtain an existence result for differential boundary value problems. The method used to show the main result is the global bifurcation theory.

Keywords

structure of positive solution sets differential boundary value problems bifurcation theory

1 Introduction

This paper considers the differential boundary value problem
{ ( p ( t ) ϕ ( u ) ) + λ p ( t ) f ( t , u ) = 0 , a < t < b , u ( a ) = u ( b ) = 0 ,
(1.1)

where f is ϕ-superlinear at ∞ and f ( t , 0 ) maybe negative and p is a positive continuous function, λ > 0 is a parameter.

Equations of form (1.1) occur in the study for the p-Laplacian equation, non-Newtonial fluid theory and the turbulent flow of a gas in a porous medium. The case where
α ( | u | 2 ) | u | = | u | p 2 | u | , p > 1 ,

i.e., perturbations of the p-Laplacian, has received much attention in the recent literature. Also, problem (1.1) with f ( t , 0 ) > 0 has been studied by several authors in recent years (see [1] and the references therein). Here, we are interested in the case when f ( t , 0 ) may be negative (the so-called semipositone case) (see [2] and its references for a review). As pointed out by Lions in [3], semi-positone problems are mathematically very challenging. During the last ten years, finding positive solutions to semi-positone problems has been actively pursued and significant progress on semi-positone problems has taken place; see [48] and the references therein. For instance, Hai et al. [9] considered the existence positive solution of (1.1). Under some super-linear conditions on the non-linear term f, they proved that there exists λ > 0 such that (1.1) has one positive solution for 0 < λ < λ . The main method in [9] used to show the main result are the fixed-point theorems.

The main purpose of this paper is going to study the structure of the positive set of (1.1). Rabinowitz [10] gave the first important results on the structure of the solution sets of non-linear equations and obtained by the degree theoretic method. Amamn [11] studied the structure of the positive solution set of non-linear equations; the reader is referred to [12, 13] for other results concerning the structure of solution sets of non-linear equations. In our paper, we will study the existence results for an unbounded connected component of a positive solution set for the differential boundary value problem of (1.1). This paper generalizes some results from the literature [9]. The paper is arranged as follows. In Section 2, we will give some preliminary lemmas. The main results will be given in Section 3.

2 Some lemmas

For convenience, we make the following assumptions:

(A1) ϕ is an odd, increasing homeomorphism on R with ϕ 1 concave on R + .

(A2) For each c > 0 , there exists A c > 0 such that ϕ 1 ( c u ) A c ϕ 1 ( u ) , u R + and lim c A c = + (note that (A2) implies the existence of B c > 0 such that ϕ 1 ( c u ) B c ϕ 1 ( u ) , u R + and lim c B c = 0 ).

(A3) p : [ a , b ] ( 0 , + ) is continuous.

(A4) f : [ a , b ] × R 1 R 1 is continuous and
lim u + f ( t , u ) ϕ ( u ) = +

uniformly for t [ a , b ] .

Let E = C [ 0 , 1 ] , the usual real Banach space of continuous functions with the maximum norm . Let e ( t ) = ( t a ) ( b t ) ( b a ) 2 for t [ a , b ] and P = { x E : u ( t ) 0 , t [ a , b ] } . Then P is a cone of E. Define
f ( t , u ) = { f ( t , u ) , u 0 , f ( t , 0 ) , u < 0 .
Then f ( t , u ) m for u R 1 (here m > 0 is a constant). For u E , λ R + , define
A ( λ , u ) = a t ϕ 1 ( C p ( s ) λ p ( s ) a s p ( r ) f ( r , u ) d r ) d s ,
here C is a constant such that
a b ϕ 1 ( C p ( s ) λ p ( s ) a s p ( r ) f ( r , u ) d r ) d s = 0 .
We know that C exists and is unique for every u P (see [14]). Then u = A ( λ , u ) if and only if u is a solution of
{ ( p ( t ) ϕ ( u ) ) + λ p ( t ) f ( t , u ) = 0 , a < t < b , u ( a ) = u ( b ) = 0 .

From [9], we have the following Lemmas 2.1 and 2.2.

Lemma 2.1 Let ϕ satisfy (A1) and (A2). Then for each d > 0 , there exist constants K d and L d such that
K d ϕ ( x ) ϕ ( d x ) L d ϕ ( x ) , x 0 .

Further, L d 0 as d 0 and K d as d .

Lemma 2.2 Let ϕ be as in Lemma  2.1. Then there exist 0 < α 1 and β 1 such that ϕ 1 ( x y ) α ϕ 1 ( x ) β ϕ 1 ( y ) for x 0 , y 0 .

Lemma 2.3 Let p 0 , p 1 > 0 such that p 0 p ( t ) p 1 for t [ a , b ] . Let λ > 0 and ω be a solution of
{ ( p ( t ) ϕ ( ω ) ) + λ p ( t ) h ( t ) = 0 , t [ a , b ] , ω ( a ) = ω ( b ) = 0 ,
(2.1)
here h ( t ) is continuous function with h ( t ) m (here m > 0 is a constant) for t [ a , b ] , if ω β ( b a ) α ϕ 1 ( λ m δ ) , then
ω ( t ) ( α ω β ϕ 1 ( λ m δ ) ( b a ) ) e ( t ) for t [ a , b ] ,

where δ = p 1 ( b a ) p 0 .

Proof By integrating, it follows that (3.1) has the unique solution given by
ω ( t ) = a t ϕ 1 { 1 p ( s ) ( C λ a s p ( r ) h ( r ) d r ) } d s ,
where C is such that ω ( b ) = 0 . Let ω = | ω ( t 0 ) | for some t 0 ( a , b ) . Then
ω ( t ) = a t ϕ 1 { λ p ( s ) ( s t 0 p ( r ) h ¯ ( r ) d r λ m p ( s ) s t 0 p ( r ) d r ) } d s ,
where h ¯ ( t ) = h ( t ) + m 0 . By Lemma 2.2, we get
ω ( t ) α a t ϕ 1 [ λ p ( s ) s t 0 p ( r ) h ¯ ( r ) d r ] d s β a t ϕ 1 ( λ m p ( s ) s t 0 p ( r ) d r ) d s .
Now
a t ϕ 1 ( λ m p ( s ) s t 0 p ( r ) d r ) d s a t ϕ 1 ( λ m p 0 s t 0 p 1 d r ) d s a t ϕ 1 ( λ m p 1 p 0 ( b a ) ) d s = ϕ 1 ( λ m δ ) ( t a ) .
And so
ω ( t ) α ω ¯ ( t ) β ϕ 1 ( λ m δ ) ( t a ) β ϕ 1 ( λ m δ ) ( t a ) for  t [ a , t 0 ] ,
(2.2)
here
ω ¯ ( t ) = a t ϕ 1 [ λ p ( s ) s t 0 p ( r ) h ¯ ( r ) d r ] d s for  t [ a , t 0 ] .
Note that ω ¯ satisfies
{ ( p ( t ) ϕ ( ω ¯ ) ) + λ p ( t ) h ¯ ( t ) = 0 , t [ a , t 0 ] , ω ¯ ( a ) = 0 , ω ¯ ( t 0 ) | ω ( t 0 ) | .
In fact, ω ¯ ( t ) ω ( t ) for t [ a , t 0 ] . We next prove that ω ¯ ( t ) ν ( t ) for t [ a , t 0 ] , here ν satisfies
{ ( p ( t ) ϕ ( ν ) ) = 0 , t [ a , t 0 ] , ν ( a ) = 0 , ν ( t 0 ) = ω .
Suppose it is not true, then ω ¯ ν has a negative absolute minimum at τ ( a , t 0 ) . Since
ω ¯ ( a ) ν ( a ) = 0 , ω ¯ ( t 0 ) ν ( t 0 ) 0 ,
there exist τ 0 , τ 1 [ a , t 0 ] such that
ω ¯ ( τ 0 ) ν ( τ 0 ) = ω ¯ ( τ 1 ) ν ( τ 1 ) = 0 ,
and
ω ¯ ( t ) ν ( t ) < 0 , t ( τ 0 , τ 1 ) .
Then
( p ( t ) ϕ ( ω ( t ) ) ) ( p ( t ) ϕ ( ν ( t ) ) ) = λ p ( t ) h ¯ ( t ) 0 for  t ( τ 0 , τ 1 ) .
Let u ( t ) = ω ¯ ( t ) ν ( t ) , t ( τ 0 , τ 1 ) , then
τ 0 τ 1 ( ( p ( t ) ϕ ( ω ¯ ( t ) ) ) ( p ( t ) ϕ ( ν ( t ) ) ) ) u ( t ) d t 0 .
On the other hand, using the inequality
( ϕ ( b ) ϕ ( a ) ) ( b a ) 0 , a , b R 1 ,
and the fact that there exists τ [ τ 0 , τ 1 ] such that ω ¯ ( τ ) ν ( τ ) , we have
τ 0 τ 1 ( ( p ( t ) ϕ ( ω ¯ ( t ) ) ) ( p ( t ) ϕ ( ν ( t ) ) ) ) u ( t ) d t = τ 0 τ 1 ( ( p ( t ) ϕ ( ω ¯ ( t ) ) ) ( p ( t ) ϕ ( ν ( t ) ) ) ) ( ω ¯ ν ) d t < 0 ,
which is a contradiction. So, ω ¯ ( t ) ν ( t ) for t [ a , t 0 ] . Obviously, ν ( t ) = ω t 0 a ( t a ) , t [ a , t 0 ] , since ω ¯ θ for each t [ a , t 0 ] . From (2.2), we have
ω ( t ) ( α ω β ϕ 1 ( λ m δ ) ( b a ) ) t a t 0 a , t [ a , t 0 ] .
Similarly,
ω ( t ) ( α ω β ϕ 1 ( λ m δ ) ( b a ) ) b t b t 0 , t [ t 0 , b ] .
If ω β ( b a ) α ϕ 1 ( λ m δ ) , then
ω ( t ) ( α ω β ϕ 1 ( λ m δ ) ( b a ) ) e ( t ) for  t [ a , b ] .

The proof is complete. □

Let Q λ = { u E u ( α u β ϕ 1 ( λ m δ ) ( b a ) ) e ( t ) , t [ a , b ] } for each λ R + , where α , β > 0 and δ > 0 are defined as that in Lemma 2.2 and Lemma 2.3, respectively. Then Q λ is also a cone of E. From Lemma 2.3, we know that A : P Q λ is completely continuous.

Let
L ( P ) = { ( λ , u ) | λ R + , u P { θ }  is a solution of  (1.1) } ¯ .

From [[15], Lemma 29.1], we have Lemma 2.4.

Lemma 2.4 Let X be a compact metric space. Assume that A and B are two disjoint closed subsets of X. Then either there exist a connected component of X meeting both A and B or X = Ω A Ω B where Ω A , Ω B are disjoint compact subsets of X containing A and B, respectively.

Let U be an open and bounded subset of the metric space [ a , b ] × E . We set U ( λ ) = { x E : ( λ , x ) U } , whose boundary is denoted by U ( λ ) . Consider a map h ( λ , x ) = x k ( λ , x ) , such that k ( λ , ) is compact and θ h ( U ) . Such a map h will also be called an admissible homotopy on U. If h is an admissible homotopy, for every λ [ a , b ] and every x U ( λ ) , one has that h λ ( x ) : = h ( λ , x ) θ and it makes sense to evaluate deg ( h λ , U ( λ ) , θ ) .

Lemma 2.5 If h is an admissible homotopy on U [ a , b ] × E , the deg ( h λ , U ( λ ) , θ ) is constant for all λ [ a , b ] .

Lemma 2.6 Let h E { θ } such that h α h e ( t ) . Then for arbitrary λ ( 0 , 1 ] , there exists R λ > 0 such that for each λ [ λ , 1 ] , R R λ and μ 0 ,
u A ( λ , u ) + μ h , u B ( θ , R ) ,

where B ( θ , R ) = { u : u < R } .

Proof From (A4), for m 1 > 0 , such that
α ( b a ) 16 ϕ 1 ( m 1 λ 0 p 0 ( b a ) 16 p 1 ) α ( b a ) 8 > 1 ,
there exists m 0 > 0 such that f ( t , u ) m 1 ϕ ( u ) for u m 0 . Let
R λ = max { 1 α [ m 0 min t [ b + 3 a 4 , 3 b + a 4 ] e ( t ) + β ϕ 1 ( λ 0 m δ ( b a ) ) ] , β ( b a ) α ϕ 1 ( λ 0 m δ ) } + 1 .
Assume by contradiction that
u 0 = A ( λ 0 , u 0 ) + μ 0 h
(2.3)
for some R R λ , u 0 B ( θ , R ) , λ 0 [ λ , 1 ] and μ 0 0 . Let
y 0 ( t ) = A ( λ 0 , u 0 ) = a t ϕ 1 ( C p ( s ) λ 0 p ( s ) a s p ( r ) f ( r , u 0 ) d r ) d s .
From Lemma 2.3, we know that y 0 ( t ) Q λ 0 . Namely,
y 0 ( t ) ( α y 0 β ϕ 1 ( λ 0 m δ ) ( b a ) ) e ( t ) .
(2.4)
From (2.3) and (2.4), we have
u 0 = y 0 ( t ) + μ 0 h ( α y 0 β ϕ 1 ( λ 0 m δ ( b a ) ) ) e ( t ) + μ 0 α h e ( t ) ( α y 0 + μ 0 h β ϕ 1 ( λ 0 m δ ( b a ) ) e ( t ) = ( α u 0 β ϕ 1 ( λ 0 m δ ) ( b a ) ) e ( t ) ,
so u 0 Q λ 0 . For λ 0 [ λ , 1 ] , we have
u 0 ( t ) ( α u 0 β ϕ 1 ( λ 0 m δ ( b a ) ) ) e ( t ) m 0 ,
for t ( 3 a + b 4 , a + b 2 ) . Therefore, let u 0 = u ( t u 0 ) , t u 0 ( 3 a + b 4 , a + b 2 ) , assume that t u 0 5 a + 3 b 8 , then
u 0 = u ( t u 0 ) = 3 a + b 4 t u 0 ϕ 1 ( λ 0 p ( s ) s t u 0 p ( τ ) f ( t , u 0 ) d τ ) d s + μ 0 h α 3 a + b 4 t u 0 ϕ 1 ( λ 0 p 0 p 1 s t u 0 p ( τ ) ( f ( t 0 , u 0 ) + m ) d τ ) d s β 3 a + b 4 t u 0 ϕ 1 ( λ 0 p 1 m p 0 ( t u 0 s ) ) d s ,
where
3 a + b 4 t u 0 ϕ 1 ( λ 0 p 0 p 1 s t u 0 ( f ( τ , u 0 ) + m ) d τ ) d s 3 a + b 4 11 a + 5 b 16 ϕ 1 ( λ 0 p 0 p 1 s t u 0 ( f ( τ , u 0 ) + m ) d τ ) d s 3 a + b 4 11 a + 5 b 16 ϕ 1 ( λ 0 p 0 p 1 11 a + 5 b 16 5 a + 3 b 8 m 1 ϕ ( u 0 ) d τ ) d s = 3 a + b 4 11 a + 5 b 16 ϕ 1 ( m 1 λ 0 p 0 ( b a ) 4 p 1 ) u 0 d s = b a 16 ϕ 1 ( m 1 λ 0 p 0 ( b a ) 16 p 1 ) u 0 ,
and
3 a + b 4 t u 0 ϕ 1 ( λ 0 p 1 m p 0 ( t u 0 s ) ) d s 3 a + b 4 t u 0 ϕ 1 ( λ 0 p 1 m p 0 ( b a ) ) d s = ϕ 1 ( λ 0 p 1 m p 0 ( b a ) ) ( t u 0 3 a + b 4 ) ( b a ) 8 ϕ 1 ( λ 0 m δ ) .
Thus,
u 0 α ( b a ) 16 ϕ 1 ( m 1 λ 0 p 0 ( b a ) 16 p 1 ) u 0 β ( b a ) 8 ϕ 1 ( λ 0 m δ ) α ( b a ) 16 ϕ 1 ( m 1 λ 0 p 0 ( b a ) 16 p 1 ) u 0 α ( b a ) 8 u 0 = ( α ( b a ) 16 ϕ 1 ( m 1 λ 0 p 0 ( b a ) 16 p 1 ) α ( b a ) 8 ) u 0 ,

so α ( b a ) 16 ϕ 1 ( m 1 λ 0 p 0 ( b a ) 16 p 1 ) α ( b a ) 8 1 , which is a contradiction. Then (2.3) holds. The proof is complete. □

3 Main results

For convenience, let us introduce the following symbols. For any r,
M ( r ) = { ( λ ˜ , u ) [ 0 , 1 ] × E : u = r } , M [ r , + ) = { ( λ ˜ , u ) [ 0 , 1 ] × E : r u < + } , M [ 0 , r ) = { ( λ ˜ , u ) [ 0 , 1 ] × E : 0 u < r } .

Now we give our main results of this paper.

Theorem 3.1 Suppose (A1) to (A4) hold. Then L ( P ) ( [ 0 , 1 ] × P ) possesses an unbounded connected component D such that Proj λ D ( 0 , λ ] for some λ > 0 and
lim λ 0 + , ( λ , u ) D u = + ,

where Proj λ D denotes the projection of D onto the λ-axis.

Proof We divide our proof into four steps.

Step 1. Let
T ( λ , u ) = { A ( λ , u ) , ( [ 0 , 1 ] × E ) M [ 2 , + ) , θ , ( [ 0 , 1 ] × B ( θ , 1 ) ¯ ) ( { 0 } × E ) ,
(3.1)

where B ( θ , 1 ) ¯ = { u E : u 1 } . Obviously, T ( , ) is a completely continuous operator.

Note that T ( λ , u ) = A ( λ , u ) for all λ [ 0 , 1 ] and u E with u 2 . From Lemma 2.5, there exists R 1 > 2 large enough such that Fix T ( 1 , ) B ( θ , R 1 ) and
deg ( I T ( 1 , ) , B ( θ , R 1 ) , θ ) = 0 .
(3.2)
Obviously,
deg ( I T ( 1 , ) , B ( θ , 1 ) , θ ) = 1 .
(3.3)
Therefore,
deg ( I T ( 1 , ) , B ( θ , R 1 ) B ( θ , 1 ) ¯ , θ ) = deg ( I T ( 1 , ) , B ( θ , R 1 ) , θ ) deg ( I T ( 1 , ) , B ( θ , 1 ) , θ ) = 0 1 = 1 .
(3.4)

So, Fix T ( 1 , ) and Fix T ( 1 , ) U : = B ( θ , R 1 ) B ( θ , 1 ) ¯ .

Step 2. Let
S = { ( λ , u ) R + × E : u = T ( λ , u ) } .
From Lemma 2.6, we have
L ( P ) [ 0 , 1 ] × { u E : 0 < u 1 } = .
This implies that T has no bifurcation point on [ 0 , 1 ] . From step 1,we have L ( P ) ( { 1 } × E ) , then for each ( 1 , u ) L ( P ) ( { 1 } × E ) , denote by D u the connected component of the metric space L ( P ) ( { 1 } × E ) emitting from ( 1 , u ) . Now we will show that, there must exist ( 1 , u 0 ) L ( P ) ( { 1 } × E ) such that D u 0 is unbounded. Assume on the contrary that D u is bounded for each ( 1 , u ) L ( P ) ( { 1 } × E ) . Take a bounded open neighborhood U u 1 in L ( P ) ( { 1 } × E ) for each D u such that
C l ( { 1 } × E ) U u 1 ( [ 0 , 1 ] × { θ } ) =
(3.5)
and U u 1 ( { 0 } × E ) = , where C l ( { 1 } × E ) U u 1 denotes the closure of U u 1 in the metric space [ 0 , 1 ] × E . Let [ 0 , 1 ] × E U u 1 denote the boundary of U u 1 in the metric space [ 0 , 1 ] × E . Obviously, [ 0 , 1 ] × E U u 1 L ( P ) is a compact subset. Assume that [ 0 , 1 ] × E U u 1 L ( P ) . From the maximal connectedness of D u , there is no connected subset of [ 0 , 1 ] × E U u 1 L ( P ) meeting both [ 0 , 1 ] × E U u 1 L ( P ) and D u . From Lemma 2.4, there exist compact disjoint subsets Ω u ( 1 ) and Ω u ( 2 ) of C l [ 0 , 1 ] × E Ω u ( 1 ) L ( P ) such that D u Ω u ( 1 ) and [ 0 , 1 ] × E U u ( 1 ) L ( P ) Ω u ( 2 ) , and C l [ 0 , 1 ] × E U u ( 1 ) L ( P ) = Ω u ( 1 ) Ω u ( 2 ) . Let d = d ( Ω u ( 1 ) , Ω u ( 2 ) ) > 0 and U u ( 2 ) be the d 3 -neighborhood of Ω u ( 1 ) in the metric space [ 0 , 1 ] × E . Set
U u = { U u ( 1 ) U u ( 2 ) , when  [ 0 , 1 ] × E U u ( 1 ) L ( P ) , U u ( 1 ) , when  [ 0 , 1 ] × E U u ( 1 ) L ( P ) = .
(3.6)
Then we have D u U u and
[ 0 , 1 ] × E U u L ( P ) = .
(3.7)
Obviously, the collection of the subsets
{ U u { 1 } × E : ( 1 , u ) L ( P ) ( { 1 } × E ) }
is an open cover of L ( P ) ( { 1 } × E ) . Since L ( P ) ( { 1 } × E ) is compact, then there exist finite points, namely
( 1 , u 1 ) , ( 1 , u 2 ) , , ( 1 , u n ) ( { 1 } × E ) L ( P ) ,
such that
( { 1 } × E ) L ( P ) i = 1 n ( U u i ( { 1 } × E ) ) .
Let U = i = 1 n U u i . Then U is a bounded open subset of [ 0 , 1 ] × E . From (3.7), we have
[ 0 , 1 ] × E U L ( P ) i = i n ( ( [ 0 , 1 ] × E U u i ) L ( P ) ) = .
(3.8)
Thus,
[ 0 , 1 ] × E U L ( P ) = .
From (3.5) and (3.8), we have
[ 0 , 1 ] × E U S = .
Then from Lemma 2.5, we have
deg ( I T ( λ , ) , U ( 1 ) , θ ) = deg ( I T ( λ , ) , U ( 0 ) , θ ) .
(3.9)
Since U ( 0 ) = , then
deg ( I T ( λ , ) , U ( 0 ) , θ ) = 0 .
(3.10)
Since Fix T B ( θ , R ) , then from (3.4) we have
deg ( I T ( λ , ) , U ( 1 ) , θ ) = 1 ,
(3.11)

which contradicts to (3.10) and (3.11). Therefore, there must exist ( 1 , u 0 ) ( { 1 } × E ) L ( P ) such that D u 0 is bounded.

Step 3. Obviously, the projection of D u is a interval, denote it by [ 0 , λ ] , then λ 1 . Then D u is a bounded connected component of ( [ 0 , λ ] × E ) . Take r 0 = β ( b a ) α ϕ ( λ m δ ) + 2 , let
Y 1 = ( { 1 } × E ) M [ r 0 , + ) , Y 2 = ( [ 0 , 1 ] × E ) M ( r 0 ) , Y = ( [ 0 , 1 ] × E ) M [ r 0 , + ) .
Obviously, D u ( Y 1 Y 2 ) . For each p D u ( Y 1 Y 2 ) , denote by E ( p ) the connected component of the metric space D u Y , which passes the point p. Now we shall prove that there must exist a p 0 D u ( Y 1 Y 2 ) such that E ( p 0 ) is an unbounded connected component of the metric space D u Y . On the contrary, assume that E ( p ) is bounded for each p D u ( Y 1 Y 2 ) . Then, for each p D u ( Y 1 Y 2 ) , in the same way as in the construction of U in (3.6) we can show that there exists a neighborhood U ( p ) of E ( p ) in Y such that
Y U ( p ) D u = .
(3.12)
Obviously, the set of { U ( p ) ( Y 1 Y 2 ) | p D u ( Y 1 Y 2 ) } is an open cover of the set D u ( Y 1 Y 2 ) and D u ( Y 1 Y 2 ) is a compact set. Thus, there exist finite subsets of { U ( p ) ( Y 1 Y 2 ) | p D u ( Y 1 Y 2 ) } , say
U ( p 1 ) ( Y 1 Y 2 ) , U ( p 2 ) ( Y 1 Y 2 ) , , U ( p n ) ( Y 1 Y 2 ) ,
which is also an open cover of D u ( Y 1 Y 2 ) , that is,
i = 1 n ( U ( p i ) ( Y 1 Y 2 ) ) D u ( Y 1 Y 2 ) .
(3.13)
Let U 0 = i = 1 n U ( p i ) , then U 0 is a bounded open subset of Y . Since
Y U 0 i = 1 n Y U ( p i ) ,
then by (3.12) we have
Y U 0 D u = .
(3.14)
Let
W 1 = ( ( [ 0 , 1 ] × E ) M [ 0 , r 0 ) ) U 0 ,
and W 2 = ( [ 0 , 1 ] × E ) C l [ 0 , 1 ] × E W 1 . It is easy to see that
[ 0 , 1 ] × E W 1 Y U 0 [ ( M ( r 0 ) ( [ 0 , 1 ] × E ) ) ( U 0 ( Y 1 Y 2 ) ) ] .

From (3.12) and (3.13), we see that [ 0 , 1 ] × E W 1 D u = . Obviously, W 1 D u and W 1 W 2 = . Note the unboundedness of D u , then W 2 D u . Now we have D u = ( W 1 D u ) ( W 2 D u ) , which is a contradiction of the connectedness of D u . Therefore, there must exist p 0 D u ( Y 1 Y 2 ) such that E ( p 0 ) is an unbounded connected component of D u Y .

Step 4. Since u = T ( λ , u ) Q λ for each ( λ , u ) E ( p 0 ) , we have
u ( α u β ϕ 1 ( λ m δ ) ) e ( t ) > θ .
So, u = A ( λ , u ) for each ( λ , u ) E ( p 0 ) . This implies E ( p 0 ) L ( P ) is an unbounded subset. Let D be the connected component of L ( P ) containing E ( p 0 ) . Obviously, there exists λ > 0 such that Proj D ( 0 , λ ] . As D is unbounded, we easily see that
lim λ 0 + , ( λ , u ) D u = + .

The proof is complete. □

Corollary 3.1 Let (A1) to (A4) hold. Then there exists λ > 0 such that problem (1.1) has a positive solution u λ for 0 < λ < λ with u λ as λ 0 .

Declarations

Acknowledgements

This paper is supported by Innovation Project of Jiangsu Province postgraduate training project (CXLX12_0979).

Authors’ Affiliations

(1)
Department of Mathematics, Jiangsu Normal University

References

  1. Manasevich R, Schmitt K: Boundary value problems for quasilinear second order differential equations. CISM Lecture Notes. In Nonlinear Analysis and Boundary Value Problems. Springer, Berlin; 1996:79-119.
  2. Castro A, Shivaji R: Semipositone Problems, Semigroups of Linear and Nonlinear Operators and Applications. Kluwer Academic, Dordrecht; 1993:109-119.View Article
  3. Lions PL: On the existence of positive solutions of semilinear elliptic equations. SIAM Rev. 1982, 24: 441-467. 10.1137/1024101MathSciNetView Article
  4. Xian X, Jingxian S: Unbounded connected component of the positive solutions set of some semi-position problems. Topol. Methods Nonlinear Anal. 2011, 37: 283-302.MathSciNet
  5. Jingxian S, Xian X: Positive fixed points of semi-positone nonlinear operator and its applications. Acta Math. Sin. 2012, 55: 55-64. in Chinese
  6. Anuradha V, Hai DD, Shivaji R: Existence results for superlinear semipositone BVPs. Proc. Am. Math. Soc. 1996, 124: 757-763. 10.1090/S0002-9939-96-03256-XMathSciNetView Article
  7. Xian X, O’Regan D, Yanfeng C: Structure of positive solution sets of simi-positon singular boundary value problems. Nonlinear Anal. 2010, 72: 3535-3550. 10.1016/j.na.2009.12.035MathSciNetView Article
  8. Haisen LU: Existence and multiplicity of positive solutions for semiposition p -Laplacian equations. Acta Math. Appl. Sin. 2006, 19(3):546-553.
  9. Hai DD, Schmitt K, Shivaji R: Positive solutions of quasilinear boundary value problems. J. Math. Anal. Appl. 1998, 217: 672-686. 10.1006/jmaa.1997.5762MathSciNetView Article
  10. Rabinowitz PH: Some global results for nonlinear eigenvalues. J. Funct. Anal. 1971, 7: 487-513. 10.1016/0022-1236(71)90030-9MathSciNetView Article
  11. Amann H: Fixed point equations and nonlinear eigenvalue problems in ordered Banach spaces. SIAM Rev. 1976, 18: 620-709. 10.1137/1018114MathSciNetView Article
  12. Dancer EN: Solution branches for mappings in cones and applications. Bull. Aust. Math. Soc. 1974, 11: 133-145.MathSciNetView Article
  13. Rabinowitz PH: On bifurcation from infinity. J. Differ. Equ. 1973, 14: 462-475. 10.1016/0022-0396(73)90061-2MathSciNetView Article
  14. Xiyu L:Some existence principles for the singular second order differential equation ( ϕ ( x ) ) + f ( t , x ) = 0 . Acta Math. Sin. 1996, 39(3):366-375.
  15. Deimling K: Nonlinear Functional Analysis. Springer, Berlin; 1985.View Article

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© Xian and Xunxia; licensee Springer. 2013

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