Electronic Journal of Differential Equations, Vol. 2013 (2013), No. 226, pp. 1–11. ISSN: 1072-6691. URL: http://ejde.math.txstate.edu or http://ejde.math.unt.edu ftp ejde.math.txstate.edu EXISTENCE OF SOLUTIONS FOR (k, n − k − 2) CONJUGATE BOUNDARY-VALUE PROBLEMS AT RESONANCE WITH dim ker L = 2 WEIHUA JIANG Abstract. By constructing suitable project operators and using the coincidence degree theory due to Mawhin, the existence of solutions for (k, n − k − 2) conjugate boundary-value problems at resonance with dimkerL = 2 is obtained. 1. Introduction The existence of solutions for (k, n − k) conjugate boundary-value problems at nonresonance has been studied in many papers (see [1, 2, 3, 6, 7, 9, 10, 11, 16, 14, 21, 25, 27, 29, 30, 31, 32]). The solvability of boundary-value problems at resonance has been investigated by many authors (see [4, 5, 8, 12, 13, 15, 17, 18, 19, 20, 26, 22, 24, 28, 33]). In [12], the existence of solutions for (k, n − k) conjugate boundaryvalue problems at resonance with dim ker L = 1 has been studied. To the best of our knowledge, no paper discusses the existence of solutions for (k, n − k − 2) conjugate boundary-value problems at resonance with dim ker L = 2. We will fill this gap in the literature. In this article, we investigate the existence of solutions for the (k, n − k − 2) conjugate boundary-value problem at resonance (−1)n−k y (n) (t) = f t, y(t), y 0 (t), . . . , y (n−1) (t) + ε(t), a.e. t ∈ [0, 1], (1.1) y (i) (0) = y (j) (1) = 0, y (n−2) (1) = l X 0 ≤ i ≤ k − 1, 0 ≤ j ≤ n − k − 3, βj y (n−2) (ηj ), y (n−1) (1) = j=1 m X αi y (n−1) (ξi ), i=1 where 1 ≤ k ≤ n − 3, 0 < η1 < η2 < · · · < ηl < 1, 0 < ξ1 < ξ2 < · · · < ξm < 1. In this article, we assume that the following conditions hold. Pl Pl Pm (H1) i=1 αi = 1, j=1 βj = 1, j=1 βj ηj = 1. 2000 Mathematics Subject Classification. 35B34, 34B10. Key words and phrases. Resonance; Fredholm operator; boundary value problem. c 2013 Texas State University - San Marcos. Submitted July 24, 2012. Published October 11, 2013. 1 (1.2) 2 W. JIANG e (H2) e = 1 e3 EJDE-2013/226 e2 6= 0, where e4 e1 = 1 − m X a i ξi , e2 = i=1 e3 = 1 2 1− m X ai ξi2 , i=1 l X 1 1− βj ηj2 , 2 j=1 e4 = l X 1 1− βj ηj3 . 6 j=1 ∞ (H3) ε(t) ∈ L [0, 1], f : [0, 1] × Rn → R satisfies Carathéodory conditions; i.e., f (·, x) is measurable for each fixed x ∈ Rn , f (t, ·) is continuous for a.e. t ∈ [0, 1], and for each r > 0, there exists Φr ∈ L∞ [0, 1] such that |f (t, x1 , x2 , . . . , xn )| ≤ Φr (t) for all |xi | ≤ r, i = 1, 2, . . . , n, a.e. t ∈ [0, 1]. 2. Preliminaries For convenience, we introduce some notation and a theorem. For more details see [23]. Let X and Y be real Banach spaces and L : dom L ⊂ X → Y be a Fredholm operator with index zero, P : X → X, Q : Y → Y be projectors such that Im P = ker L, ker Q = Im L, X = ker L ⊕ ker P, Y = Im L ⊕ Im Q. It follows that Ldom L∩ker P : dom L ∩ ker P → Im L is invertible. We denote its inverse by KP . Let Ω be an open bounded subset of X, dom L ∩ Ω 6= ∅, the map N : X → Y will be called L-compact on Ω if QN (Ω) is bounded and KP (I − Q)N : Ω → X is compact. Theorem 2.1 ([23]). Let L : dom L ⊂ X → Y be a Fredholm operator of index zero and N : X → Y L-compact on Ω. Assume that the following conditions are satisfied: (1) Lx 6= λN x for every (x, λ) ∈ [(dom L \ ker L) ∩ ∂Ω] × (0, 1); (2) N x ∈ / Im L for every x ∈ ker L ∩ ∂Ω; (3) deg(QN |ker L , Ω ∩ ker L, 0) 6= 0, where Q : Y → Y is a projection such that Im L = ker Q. Then the equation Lx = N x has at least one solution in dom L ∩ Ω. Take X = C n−1 [0, 1] with norm kuk = max{kuk∞ , ku0 k∞ , . . . , ku(n−1) k∞ }, R1 where kuk∞ = maxt∈[0,1] |u(t)|, Y = L1 [0, 1] with norm kxk1 = 0 |x(t)|dt. Define operator Ly(t) = (−1)n−k y (n) (t) with n dom L = y ∈ X : y (n) ∈ Y, y (i) (0) = y (j) (1) = 0, 0 ≤ i ≤ k − 1, 0 ≤ j ≤ n − k − 3, y (n−2) (1) = l X j=1 y (n−1) (1) = m X i=1 o αi y (n−1) (ξi ) . βj y (n−2) (ηj ), EJDE-2013/226 EXISTENCE OF SOLUTIONS Let N : X → Y be defined as N y(t) = f t, y(t), y 0 (t), . . . , y (n−1) (t) + ε(t), 3 t ∈ [0, 1]. Then problem (1.1), (1.2) becomes Ly = N y. We use convention that 1/k! = 0, for k = −1, −2, . . . . By simple calculation, we can get the following results. 1 1 1 ... k! (k+1)! (n−3)! 1 1 1 . . . k! (n−4)! (k−1)! ... ... 1 1 1 . . . [n−3−(n−k−3)]! [k−(n−k−3)]! [k+1−(n−k−3)]! = (n − k − 3)! (n − k − 4)! 1 · ... 6= 0. k! (k + 1)! (n − 3)! So, the following lemmas hold. Lemma 2.2. The system of linear equations xk xk+1 xn−3 1 + + ··· + + = 0, k! (k + 1)! (n − 3)! (n − 2)! xk+1 xn−3 1 xk + + ··· + + = 0, (k − 1)! k! (n − 4)! (n − 3)! ... xk xk+1 + + ... [k − (n − k − 3)]! [k + 1 − (n − k − 3)]! 1 xn−3 + =0 + [n − 3 − (n − k − 3)]! [n − 2 − (n − k − 3)]! has only one solution, its denoted by (ak , ak+1 , . . . , an−3 ). Lemma 2.3. The system of linear equations xk xk+1 xn−3 1 + + ··· + + = 0, k! (k + 1)! (n − 3)! (n − 1)! xk xk+1 xn−3 1 + + ··· + + = 0, (k − 1)! k! (n − 4)! (n − 2)! ... xk xk+1 + + ... [k − (n − k − 3)]! [k + 1 − (n − k − 3)]! xn−3 1 + + =0 [n − 3 − (n − k − 3)]! [n − 1 − (n − k − 3)]! has only one solution, it is denoted by (bk , bk+1 , . . . , bn−3 ). Lemma 2.4. For given u ∈ Y , the system of linear equations Z xk xk+1 xn−3 (−1)n−k 1 + + ··· + + (1 − s)n−1 u(s)ds = 0, k! (k + 1)! (n − 3)! (n − 1)! 0 Z xk xk+1 xn−3 (−1)n−k 1 + + ··· + + (1 − s)n−2 u(s)ds = 0, (k − 1)! k! (n − 4)! (n − 2)! 0 ... 4 W. JIANG EJDE-2013/226 xk xk+1 xn−3 + + ··· + [k − (n − k − 3)]! [k + 1 − (n − k − 3)]! [n − 3 − (n − k − 3)]! Z 1 (−1)n−k (1 − s)n−1−(n−k−3) u(s)ds = 0 + [n − 1 − (n − k − 3)]! 0 has only one solution, its denoted by (Bk (u), Bk+1 (u), . . . , Bn−3 (u)). Define the operators T1 , T2 , Q1 , Q2 : Y → R as follows: Z 1 m X T1 u(t) = αi u(s)ds, i=1 T2 u(t) = l X j=1 βj hZ ξi 1 Z (1 − s)u(s)ds + (1 − ηj ) ηj 1 (e4 T1 u − e3 T2 u), Q2 u = e Obviously, e1 = T1 (1), e2 = T2 (1), e3 = T1 (t), e4 Q1 u = ηj u(s)ds , 0 1 (−e2 T1 u + e1 T2 u). e = T2 (t). Lemma 2.5. Assume that (H1) holds, then L : dom L ⊂ X → Y is a Fredholm operator of index zero and the linear continuous projector Q : Y → Y can be defined as Qu = Q1 u + t · Q2 u, and the linear operator KP : Im L → dom L ∩ ker P can be written as Z n−3 X Bi (u) (−1)n−k t ti + KP u = (t − s)n−1 u(s)ds. i! (n − 1)! 0 i=k Pn−1 Proof. Take y ∈ ker L. We obtain y = i=k xi!i ti satisfying xk xk+1 xn−2 xn−1 + + ··· + + = 0, k! (k + 1)! (n − 2)! (n − 1)! xk+1 xn−2 xn−1 xk + + ··· + + = 0, (k − 1)! k! (n − 3)! (n − 2)! ... xk xk+1 + + ... [k − (n − k − 3)]! [k + 1 − (n − k − 3)]! xn−2 xn−1 + + = 0. [n − 2 − (n − k − 3)]! [n − 1 − (n − k − 3)]! Setting xn−2 = 1, xn−1 = 0, and xn−2 = 0, xn−1 = 1, respectively, by Lemmas 2.2, 2.3, we have y= n−3 X i=k cai + dbi i c d t + tn−2 + tn−1 , c, d ∈ R. i! (n − 2)! (n − 1)! Therefore, n−3 X cai + dbi c d ti + tn−2 + tn−1 , c, d ∈ R . ker L = y : y = i! (n − 2)! (n − 1)! i=k Define the linear operator P : X → X as follows P y(t) = n−3 X i=k y (n−2) (0)ai + y (n−1) (0)bi i y (n−2) (0) n−2 y (n−1) (0) n−1 t + t + t . i! (n − 2)! (n − 1)! EJDE-2013/226 EXISTENCE OF SOLUTIONS 5 Obviously, Im P = ker L and P 2 y = P y. For any y ∈ X, it follows from y = (y − P y) + P y that X = ker P + ker L. By simple calculation, we can get that ker L ∩ ker P = {0}. So, we have X = ker L ⊕ ker P. We will show that Z m X Im L = u ∈ Y : αi βj hZ 1 u(s)ds = 0, ξi i=1 l X (2.1) 1 Z ηj j=1 ηj (1 − s)u(s)ds + (1 − ηj ) i u(s)ds = 0 . 0 In fact, if u ∈ Im L, there exists y ∈ dom L such that u = Ly ∈ Y . This, together with y i (0) = 0, 0 ≤ i ≤ k − 1, implies that Z n−1 X ci (−1)n−k t ti + (t − s)n−1 u(s)ds. y(t) = i! (n − 1)! 0 i=k Pm Pm (n−1) Since i=1 αi = 1 and y (1) = i=1 αi y (n−1) (ξi ), we obtain Z 1 m X αi u(s)ds = 0. (2.2) i=1 Since Pl j=1 ξi Pl βj ηj = 1 and y (n−2) (1) = Z l hZ 1 X βj (1 − s)u(s)ds + (1 − ηj ) βj = 1, j=1 j=1 ηj Pl j=1 ηj βj y (n−2) (ηj ), we obtain i u(s)ds = 0. (2.3) 0 On the other hand, if u ∈ Y satisfies (2.2) and (2.3), take Z n−3 X Bi (u) (−1)n−k t ti + (t − s)n−1 u(s)ds. y= i! (n − 1)! 0 i=k It follows from (2.2), (2.3) and Lemma 2.4 that y ∈ dom L. Obviously, Ly = u. So, we get u ∈ Im L. Now we will prove that Q : Y → Y is a projector such that ker Q = Im L, Y = Im L ⊕ Im Q. For u ∈ Y , since 1 1 Q1 (1) = [e4 T1 (1) − e3 T2 (1)] = 1, Q1 (t) = [e4 T1 (t) − e3 T2 (t)] = 0, e e 1 1 Q2 (1) = [−e2 T1 (1) + e1 T2 (1)] = 0, Q2 (t) = [−e2 T1 (t) + e1 T2 (t)] = 1, e e we have Q1 (Qu) = Q1 (Q1 u + t · Q2 u) = Q1 u · Q1 (1) + Q2 u · Q1 (t) = Q1 u, Q2 (Qu) = Q2 (Q1 u + t · Q2 u) = Q1 u · Q2 (1) + Q2 u · Q2 (t) = Q2 u. Thus, Q2 u = Q1 (Qu) + t · Q2 (Qu) = Q1 u + t · Q2 u = Qu. Since u ∈ ker Q, we have e4 T1 u − e3 T2 u = 0, −e2 T1 u + e1 T2 u = 0. 6 W. JIANG EJDE-2013/226 It follows from (H2) that T1 u = T2 u = 0. So, u ∈ Im L; i.e., ker Q ⊂ Im L. Clearly, Im L ⊂ ker Q. So, Im L = ker Q. This, together with Q2 y = Qy, means that Im L ∩ Im Q = {0}. Thus, we have Y = Im L ⊕ Im Q. Considering (2.1), we know that L is a Frdholm operator of index zero. Define the operator KP : Y → X as follows Z n−3 X Bi (u) (−1)n−k t (t − s)n−1 u(s)ds. KP u = ti + i! (n − 1)! 0 i=k For u ∈ Im L, by Lemma 2.4, we have KP u ∈ dom L. Clearly, KP u ∈ ker P . So, we get that KP (Im L) ⊂ dom L ∩ ker P . Now we will prove that KP is the inverse of L|dom L∩ker P . Obviously, LKP u = u, for u ∈ Im L. On the other hand, for y ∈ dom L ∩ ker P , we have Z n−3 X Bi (Ly) (−1)n−k t ti + (t − s)n−1 (−1)n−k y (n) (s)ds KP Ly(t) = i! (n − 1)! 0 i=k = n−3 X i=k Bi (Ly) − y (i) (0) i t + y(t). i! Since KP (Ly) ∈ dom L and y ∈ dom L, we obtain (KP Ly)(j) (1) = y (j) (1) = 0, 0 ≤ j ≤ n − k − 3. Thus (Bk (Ly) − y (k) (0), Bk+1 (Ly) − y (k+1) (0), . . . , Bn−3 (Ly) − y (n−3) (0)) is the only zero solution of the system of linear equations xk xk+1 xn−3 + + ··· + = 0, k! (k + 1)! (n − 3)! xk xk+1 xn−3 + + ··· + = 0, (k − 1)! k! (n − 4)! ... xk xk+1 + + ... [k − (n − k − 2)]! [k + 1 − (n − k − 2)]! xn−3 = 0. + [n − 3 − (n − k − 3)]! So, we have KP Ly = y, for y ∈ dom L ∩ ker P . Thus, KP = (L|dom L∩ker P )−1 . The proof is complete. 3. Main results Lemma 3.1. Assume Ω ⊂ X is an open bounded subset and dom L ∩ Ω 6= ∅, then N is L-compact on Ω. Proof. By (H3), we have that QN (Ω) is bounded. Now we will show that KP (I − Q)N : Ω → X is compact. It follows from (H3) that there exists constant M0 > 0 such that |(I − Q)N y| ≤ M0 , a.e. t ∈ [0, 1], y ∈ Ω. Thus, KP (I −Q)N (Ω) is bounded. By (H3) and Lebesgue Dominated Convergence theorem, we get that KP (I − Q)N : Ω → X is continuous. Rt Since { 0 (t − s)j (I − Q)N y(s)ds, y ∈ Ω}, j = 0, 1 . . . , n − 1 are equi-continuous, and tj , j = 0, 1 . . . , n−1 are uniformly continuous on [0,1], using Ascoli-Arzela theorem, we obtain that KP (I − Q)N : Ω → X is compact. The proof is complete. To obtain our main results, we need the following assumptions. EJDE-2013/226 EXISTENCE OF SOLUTIONS 7 (H4) There exist constants M1 > 0, M2 > 0 such that if |y (n−1) (t)| > M1 , t ∈ [ξm , 1] then Z 1 m X αi N y(s)ds 6= 0, i=1 and if |y ξi (n−2) (t)| > M2 , t ∈ [0, η1 ] then Z l hZ 1 X βj (1 − s)N y(s)ds + (1 − ηj ) ηj j=1 ηj i N y(s)ds 6= 0. 0 (H5) There exist functions g, h, ψi ∈ L1 [0, 1], i = 1, 2, . . . , n, with kψn k1 := r1 < Pn−1 1 1/2, i=1 kψi k1 := r2 < 1−2r 4 , θ ∈ [0, 1), and some 1 ≤ j ≤ n − 1 such that n X ψi (t)|xi | + h(t)|xj |θ . |f (t, x1 , x2 , . . . , xn )| ≤ g(t) + i=1 (H6) There exist constants c0 > 0, d0 > 0 such that, for y= n−3 X i=k cai + dbi i c d t + tn−2 + tn−1 ∈ ker L, i! (n − 2)! (n − 1)! one of the following two conditions holds (1) c · T1 N y < 0, if |c| > c0 , d · T2 N y < 0, if |d| > d0 , (2) c · T1 N y > 0, if |c| > c0 , d · T2 N y > 0, if |d| > d0 , Lemma 3.2. Suppose (H1)–(H5) hold, then the set Ω1 = {y ∈ dom L \ ker L : Ly = λN y, λ ∈ (0, 1)} is bounded. Proof. Take y ∈ Ω1 . By N y ∈ Im L, we have Z 1 m X αi N y(s)ds = 0, i=1 l X βj hZ 1 Z (1 − s)N y(s)ds + (1 − ηj ) ηj j=1 (3.1) ξi ηj i N y(s)ds = 0. (3.2) 0 Since Ly = λN y and y ∈ dom L, we obtain y(t) = n−1 X i=k ci i (−1)n−k t + λ i! (n − 1)! t Z (t − s)n−1 N y(s)ds, 0 where ck , ck+1 , . . . , cn−1 satisfy n−1 X i=k n−1 X i=k ci (−1)n−k =− λ i! (n − 1)! Z 1 (1 − s)n−1 N y(s)ds, 0 n−k ci (−1) =− λ (i − 1)! (n − 2)! ... Z 0 1 (1 − s)n−2 N y(s)ds, (3.3) 8 W. JIANG n−1 X i=k ci (−1)n−k =− λ [i − (n − k − 3)]! [i − (n − k − 3)]! EJDE-2013/226 Z 1 (1 − s)i−(n−k−3) N y(s)ds. 0 It follows from y (i) (0) = y (j) (1) = 0, 0 ≤ i ≤ k − 1, 0 ≤ j ≤ n − k − 3 that there exist points δi ∈ [0, 1] such that y (i) (δi ) = 0, i = 0, 1, . . . , n − 3. So, we have Z t y (i+1) (s)ds, i = 0, 1, . . . , n − 3. y (i) (t) = δi Therefore, ky (i) k∞ ≤ ky (i+1) k1 ≤ ky (i+1) k∞ , i = 0, 1, . . . , n − 3. (3.4) (n−1) By (3.1) and (H4), there exists t0 ∈ [ξm , 1] such that |y (t0 )| ≤ M1 . This, together with (3.3), implies that Z 1 f (s, y(s), y 0 (s), . . . , y (n−1) (s))ds + kεk1 . |cn−1 | ≤ M1 + 0 By (3.2) and (H4), we get that there exists t1 ∈ [0, η1 ] such that |y (n−2) (t1 )| ≤ M2 . It follows from (3.3) that Z 1 f (s, y(s), y 0 (s), . . . , y (n−1) (s))ds + kεk1 |cn−2 | ≤ M2 + |cn−1 | + 0 1 Z f (s, y(s), y 0 (s), . . . , y (n−1) (s))ds + 2kεk1 . ≤ M1 + M2 + 2 0 Thus, ky (n−1) k∞ ≤ M1 + 2 Z 1 f (s, y(s), y 0 (s), . . . , y (n−1) (s))ds + 2kεk1 , 0 ky (n−2) k∞ ≤ 2M1 + M2 + 4 Z 1 f (s, y(s), y 0 (s), . . . , y (n−1) (s))ds + 4kεk1 . 0 By (H5) and (3.4) we have ky (n−1) k∞ ≤ r3 + 2r2 ky (n−2) k∞ + 2r1 ky (n−1) k∞ + 2khk1 ky (n−2) kθ∞ and ky (n−2) k∞ ≤ 2r3 + M2 + 4r2 ky (n−2) k∞ + 4r1 ky (n−1) k∞ + 4khk1 ky (n−2) kθ∞ , (3.5) where r3 = M1 + 2kgk1 + 2kεk1 . So, we obtain ky (n−1) k∞ ≤ 1 [r3 + 2r2 ky (n−2) k∞ + 2khk1 ky (n−2) kθ∞ ]. 1 − 2r1 (3.6) By (3.5) and (3.6), we have ky (n−2) k∞ ≤ 2r3 4r2 4khk1 (n−2) θ + M2 + ky (n−2) k∞ + ky k∞ . 1 − 2r1 1 − 2r1 1 − 2r1 Therefore, ky (n−2) k∞ ≤ 1 [2r3 + (1 − 2r1 )M2 + 4khk1 ky (n−2) kθ∞ ]. 1 − 2r1 − 4r2 It follows from θ ∈ [0, 1) that {ky (n−2) k∞ : y ∈ Ω1 } is bounded. By (3.4) and (3.6), we get that Ω1 is bounded. EJDE-2013/226 EXISTENCE OF SOLUTIONS 9 Lemma 3.3. Suppose (H1)–(H3), (H6) hold. Then the set Ω2 = {y ∈ ker L : N y ∈ Im L} is bounded. Proof. Take y ∈ Ω2 , then y(t) = n−3 X i=k c d cai + dbi i t + tn−2 + tn−1 . i! (n − 2)! (n − 1)! By N y ∈ Im L, we have T1 N y = 0, T2 N y = 0. By (H6), we get that |c| ≤ c0 , |d| ≤ d0 . This means that Ω2 is bounded. Lemma 3.4. Suppose (H1)–(H3), (H6) hold. Then the set Ω3 = {y ∈ ker L : λJy + (1 − λ)ωQN y = 0, λ ∈ [0, 1]} is bounded, where J : ker L → Im Q is a linear isomorphism given by J n−3 1 X cai + dbi c d 1 ti + tn−2 + tn−1 = (e4 c − e3 d) + (−e2 c + e1 d)t, i! (n − 2)! (n − 1)! e e i=k where c, d ∈ R and ( −1, ω= 1, if (H6)(1) holds, if (H6)(2) holds. Proof. Take y ∈ Ω3 . y ∈ ker L implies that y= n−3 X i=k c d cai + dbi i t + tn−2 + tn−1 , c, d ∈ R. i! (n − 2)! (n − 1)! Since λJy + (1 − λ)ωQN y = 0, we obtain λc = −(1 − λ)ωT1 N y, λd = −(1 − λ)ωT2 N y. If λ = 0, by (H6), we get |c| ≤ c0 , |d| ≤ d0 . If λ = 1, then c = d = 0. For λ ∈ (0, 1), if |c| > c0 or |d| > d0 , then λc2 = −(1 − λ)ωc · T1 N y < 0 or λd2 = −(1 − λ)ωd · T2 N y < 0. A contradiction. So, Ω3 is bounded. Theorem 3.5. Suppose (H1)–(H6) hold. Then (1.1)–(1.2) has at least one solution in X. Proof. Let Ω ⊃ ∪3i=1 Ωi ∪ {0} be a bounded open subset of X. It follows from Lemma 3.1 that N is L-compact on Ω. By Lemmas 3.2 and 3.3, we obtain (1) Ly 6= λN y for every (y, λ) ∈ [(dom L \ ker L) ∩ ∂Ω] × (0, 1); (2) N y ∈ / Im L for every y ∈ ker L ∩ ∂Ω. 10 W. JIANG EJDE-2013/226 We need to prove only that: deg(QN |ker L , Ω ∩ ker L, 0) 6= 0. Take H(y, λ) = λJy + ω(1 − λ)QN y. According to Lemma 3.4, we know that H(y, λ) 6= 0 for y ∈ ∂Ω ∩ ker L, λ ∈ [0, 1]. By the homotopy of degree, we obtain deg(QN |ker L , Ω ∩ ker L, 0) = deg(ωH(·, 0), Ω ∩ ker L, 0) = deg(ωH(·, 1), Ω ∩ ker L, 0) = deg(ωJ, Ω ∩ ker L, 0) 6= 0. By Theorem 2.1, we can obtain that Ly = N y has at least one solution in dom L∩Ω; i.e., (1.1)–(1.2) has at least one solution in X. The prove is complete. Acknowledgments. The author is grateful to anonymous referees for their constructive comments and suggestions which led to improvement of the original manuscript. 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