Electronic Journal of Differential Equations, Vol. 2022 (2022), No. 75, pp. 1–13. ISSN: 1072-6691. URL: http://ejde.math.txstate.edu or http://ejde.math.unt.edu POSITIVE SOLUTIONS FOR KIRCHHOFF-SCHRÖDINGER EQUATIONS VIA POHOZAEV MANIFOLD XIAN HU, YONG-YI LAN Abstract. In this article we consider the Kirchhoff-Schrödinger equation − ( (a+ b ∫ R3 |∇u|2 dx ) ∆u+ λu = k(x)f(u), x ∈ R3, where u ∈ H1(R3), λ > 0, a > 0, b ≥ 0 are real constants, k : R3 → R and f ∈ C(R,R). To overcome the difficulties that k is non-symmetric and the non-linear, and that f is non-homogeneous, we prove the existence a positive solution using projections on a general Pohozaev type manifold, and the linking theorem. 1. Introduction and main results This article concerns the Kirchhoff-Schrödinger equation − ( (a+ b ∫ R3 |∇u|2 dx ) ∆u+ λu = k(x)f(u), x ∈ R3, (1.1) where u ∈ H1(R3), λ > 0, a > 0, b ≥ 0 real constants, k : R3 → R and f : R→ R. We use the following assumptions: (H1) k ∈ C1(R3, [0,∞]), with k0 = infx∈R3 k(x) > 0; (H2) k∞ = lim|y|→∞ k(y) <∞; (H3) t 7→ k(tx) + 1 3∇k(tx) · (tx) is nondecreasing on (0,∞) for all x ∈ R3; (H4) ∇k(x) · x ≥ 0 and k(x) + 1 3∇k(x) · x ≤ ( 6≡)k∞, for all x ∈ R3; (H5) supR3 |k∞ − k(x)| ≤ β0( ∫ R3 F (w) dx)−1, where β0 is the unique positive root of the equation t2/3 + 2(m∞)1/3t = (m∞)2/3; (H6) f ∈ C(R,R), tf(t) ≥ 0, and there exist q ∈ (2, 6) such that lim|t|→∞ f(t)/|t|q−1 = 0; (H7) limt→0 f(t)/t = 0; (H8) f(t)t− 4F (t) ≥ 0 for all t ∈ R\{0}, where F (t) = ∫ t 0 f(s) ds. We look for the weak solutions of (1.1) which are the same as the critical points of the functional defined in H1(R3) by I(u) = 1 2 ∫ R3 (a|∇u|2 + λu2) dx+ b 4 (∫ R3 |∇u|2 dx )2 − ∫ R3 k(x)F (u) dx. (1.2) 2020 Mathematics Subject Classification. 35J35, 35B38, 35J92. Key words and phrases. Kirchhoff-Schrödinger equation; Pohozaev manifold; Cerami sequence; linking theorem. ©2022. This work is licensed under a CC BY 4.0 license. Submitted March 21, 2022. Published November 17, 2022. 1 2 X. HU, Y. LAN EJDE-2022/75 If k(x) ≡ k∞, then (1.1) reduces to the autonomous form − ( (a+ b ∫ R3 |∇u|2 dx ) ∆u+ λu = k∞f(u), x ∈ R3, (1.3) with u ∈ H1(R3). Its energy functional is I∞(u) = 1 2 ∫ R3 (a|∇u|2 + λu2) dx+ b 4 ( ∫ R3 |∇u|2 dx)2 − k∞ ∫ R3 F (u) dx. (1.4) Problem (1.1) is related to the stationary analogue of the equation utt − (a+ b ∫ R3 |∇u|2 dx)4u = 0 which was proposed by Kirchhoff [8] as an extension of classical D’Alembert’s wave equation. It has been applied widely to model various physics problems and ap- pears in some biological systems. The nonlocal term ( ∫ R3 |∇u|2 dx)4u, arises in various models of physical and biological systems, and the research for related is- sues gives rise to more mathematical difficulties and challenges; for more details and backgrounds, we refer the reader to [1, 3, 6] and references therein. After the pioneer work of Lions [12], Kirchhoff type problems began to attract the attention of mathematicians, see for example [10, 11, 21]. Recently, a lots of interesting results for problem (1.1) or similar problems have been obtained, see for example [2, 12, 16, 17, 18, 20] for the radial symmetry case, and [4, 5, 9, 13, 14, 19, 22, 23] for the non-radial symmetry case. As we known, the radial symmetry plays a crucial role since which can restore the compactness of the (PS)-sequence for the energy functional I. Salvatore [16] established the existence of multiple radially symmetric solutions with the radially symmetric case where V depends on |x|. Wang et al [20] obtained a least-energy sign-changing (or nodal) solution by using constraint variational method and the quantitative deformation lemma. When b = 0, the existence of solution was obtain by Strauss [17] and Lions [12] if f is superlinear at infinity, also in [2, 18] if f is asymptotically linear at infinity. For non-radial symmetry case, problem (1.1) with k(x) > k∞ > 0 was also solved in [13] by constrained minimization and concentration-compactness argu- ments. There the role played by the inequality k(x) > k∞ in restoring compactness in RN is used. However, in case k(x) ≤ ( 6≡)k∞ and f is superlinear at infinity, nonsymmetric problem (1.1) cannot be solved by minimization [4]. Che and Chen [5] considered existence and multiplicity of positive solutions by using the Nehari manifold technique and the Ljusternik Schnirelmann category theory. Under proper assumptions, Wang and Zhang [23] obtained a ground state solution for the above problem with the help of Nehari manifold. In [14, 19], the authors studied the existence of ground state solutions of Nehari-Pohozaev type. When b = 0, [9, 22] studied a class of nonlinear Schrödinger equations by using concentration compact- ness arguments and projections on a general Pohozaev type manifold. Motivated by [9, 14, 19, 22], we investigate the existence of nontrivial solutions of problem (1.1). In this article, the main obstacle is that the geometrical hy- potheses on the potential k(x) does not allow us to use concentration compactness arguments as in [4, 13]. In general, this difficulty is circumvented by assuming symmetry properties of k(x). Our objective is to prove the existence of a positive solution of (1.1) under k(x) ≤ (6≡)k∞ and k∞ = lim|x|→∞ k(x), but not requiring EJDE-2022/75 KIRCHHOFF-SCHRÖDINGER EQUATIONS 3 any symmetry properties. Another obstacle is that the nonlinear term in (1.1) is non-homogeneous and non-autonomous. Projections on Nehari manifold are not possible in general, thus one is motivated to use the more suitable projections on the set of points which satisfy the Pohozaev identity [15], the so-called the Pohozaev manifold of (1.1). Let a > 0 and b ≥ 0 be fixed. Throughout the paper we use the following notation: H1(R3) denotes the usual Sobolev space equipped with the norm ‖u‖2λ = ∫ R3 (a|∇u|2 + λu2) dx. Ls(R3) (1 ≤ s <∞) denotes the Lebesgue space with the norm ‖u‖ss = ∫ R3 |u|s dx. For u ∈ H1(R3)\{0}, ut(x) = u(x/t) for t > 0. For x ∈ R3 and r > 0, Br(x) = {y ∈ R3 : |y − x| < r}. We denote various positive constants as c, ci, C, Ci (i = 0, 1, 2, 3, . . . ). To state our results, we define two functionals on H1(R3) as follows: P (u) = a 2 ∫ R3 |∇u|2 dx+ 3λ 2 ∫ R3 λu2 dx+ b 2 (∫ R3 |∇u|2 dx )2 − ∫ R3 [3k(x) +∇k(x) · x]F (u) dx , (1.5) P∞(u) = a 2 ∫ R3 |∇u|2 dx+ 3λ 2 ∫ R3 u2 dx+ b 2 (∫ R3 |∇u|2 dx )2 − 3k∞ ∫ R3 F (u) dx. (1.6) We define the Pohozaev manifold associated with (1.1) and (1.3) by M = {u ∈ H1(R3)\{0} : P (u) = 0}, (1.7) M∞ = {u ∈ H1(R3)\{0} : P∞(u) = 0}. (1.8) We are now in position to state and prove our main result. Theorem 1.1. Under assumptions (H1)–(H8), problem (1.1) has a positive solu- tion u ∈ H1(R3)\{0}. 2. Proof of Theorem 1.1 Lemma 2.1. Suppose that ∫ R3 [λu 2 2 − k∞F (u)] dx < 0. Then there exists unique tu > 0 and tu∗ > 0 such that utu ∈M and utu∗ ∈M∞. Proof. First we define the function ψ(t) = I(ut) = at 2 ∫ R3 |∇u|2 dx+ λt3 2 ∫ R3 u2 dx+ bt2 4 (∫ R3 |∇u|2 dx )2 − t3 ∫ R3 k(tx)F (u) dx. 4 X. HU, Y. LAN EJDE-2022/75 Taking the derivative of ψ(t), we obtain ψ′(t) = a 2 ∫ R3 |∇u|2 dx+ 3λt2 2 ∫ R3 u2 dx+ bt 2 (∫ R3 |∇u|2 dx )2 − 3t2 ∫ R3 k(tx)F (u) dx− t3 ∫ R3 ∇k(tx) · xF (u) dx = a 2 ∫ R3 |∇u|2 dx+ bt 2 (∫ R3 |∇u|2 dx )2 + 3t2 ∫ R3 [ λu2 2 − k(tx)F (u)] dx − t3 ∫ R3 ∇k(tx) · xF (u) dx. By the Lebesgue Dominated Convergence Theorem, lim t→∞ ∫ R3 [ λu2 2 − k(tx)F (u)] dx = ∫ R3 [ λu2 2 − k∞F (u)] dx < 0. By (H2) and (H4), we have ∇k(x) · x→ 0, as |x| → ∞. (2.1) Using again the Lebesgue Dominated Convergence Theorem, lim t→∞ ∫ R3 ∇k(tx) · (tx)F (u) dx = 0. where we have used (H6) and (H7). Therefore, if t > 0 is sufficiently large, then ψ′(t) < 0. On the other hand, taking t > 0 sufficiently small in the expression of ψ′(t), we obtain ψ′(t) > 0. Since ψ′ is continuous, there exists at least one tu > 0 such that ψ′(tu) = 0. Then P (utu) = tψ′(tu) = 0 so that utu ∈M. Moreover (H3) implies that 3t3[k(x)− k(tx)] + (t3 − 1)∇k(x) · x ≤ 0, ∀t ≥ 0, x ∈ R3. (2.2) By this inequality, (H6) and (H7), for any u ∈ H1(R3), t > 0, one has I(u)− I(ut) = a(1− t) 2 ‖∇u‖22 + λ(1− t3) 2 ‖u‖22 + b(1− t2) 4 ‖∇u‖42 − ∫ R3 [k(x)− t3k(tx)]F (u) dx = 1− t3 3 P (u) + a(t3 − 3t+ 2) 6 ‖∇u‖22 + b(2t3 − 3t2 + 1) 12 ‖∇u‖42 − 1 3 ∫ R3 [3t3(k(x)− k(tx)) + (t3 − 1)∇k(x) · x]F (u) dx ≥ 1− t3 3 P (u) + a(t3 − 3t+ 2) 6 ‖∇u‖22 + b(2t3 − 3t2 + 1) 12 ‖∇u‖42. (2.3) Next we claim that tu is unique. In fact, for any given u satisfies ∫ R3 [λu 2 2 − k∞F (u)] dx < 0. Let t1, t2 > 0 such that ut1 , ut2 ∈M. Then P (ut1) = P (ut2) = 0. From this and (2.3), we have I(ut1) ≥ I(ut2) + t31 − t32 3t31 P (ut1) + a(2t31 − 3t21t2 + t32) 6t31 ‖∇ut1‖22 + b(3t41 − 3t21t 2 2 − 2t31 + 2t32) 12t21 ‖∇ut1‖42 EJDE-2022/75 KIRCHHOFF-SCHRÖDINGER EQUATIONS 5 = I(ut2) + a(2t31 − 3t21t2 + t32) 6t31 ‖∇ut1‖22 + b(3t41 − 3t21t 2 2 − 2t31 + 2t32) 12t21 ‖∇ut1‖42 and I(ut2) ≥ I(ut1) + t32 − t31 3t32 P (ut2) + a(2t32 − 3t22t1 + t31) 6t32 ‖∇ut2‖22 + b(3t42 − 3t22t 2 1 − 2t32 + 2t31) 12t22 ‖∇ut2‖42 = I(ut1) + a(2t32 − 3t22t1 + t31) 6t32 ‖∇ut2‖22 + b(3t42 − 3t22t 2 1 − 2t32 + 2t31) 12t22 ‖∇ut2‖42. These inequalities above imply t1 = t2. Therefore, tu > 0 is unique. Similarly, we define the function ϕ(t) = I∞(ut) = at 2 ∫ R3 |∇u|2 dx+ λt3 2 ∫ R3 u2 dx+ bt2 4 (∫ R3 |∇u|2 dx )2 − k∞t3 ∫ R3 F (u) dx. Taking the derivative of ψ(t), we obtain ϕ′(t) = a 2 ∫ R3 |∇u|2 dx+ 3λt2 2 ∫ R3 u2 dx+ bt 2 (∫ R3 |∇u|2 dx )2 − 3t2k∞ ∫ R3 F (u) dx = a 2 ∫ R3 |∇u|2 dx+ bt 2 (∫ R3 |∇u|2 dx )2 + 3t2 ∫ R3 [ λu2 2 − k∞F (u)] dx. Therefore, if t > 0 is sufficiently large, then ϕ′(t) < 0. Taking t > 0 sufficiently small, we obtain ϕ′(t) > 0. Since ϕ′ is continuous, there exists at least one tu∗ > 0 such that ϕ′(tu∗) = 0. Then P∞(utu∗ ) = tϕ′(tu∗) = 0 so that utu∗ ∈M∞. For any u ∈ H1(R3), t > 0, one has I∞(u)− I∞(ut) = a(1− t) 2 ‖∇u‖22 + λ(1− t3) 2 ‖u‖22 + b(1− t2) 4 ‖∇u‖42 − k∞(1− t3) ∫ R3 F (u) dx = 1− t3 3 P∞(u) + a(t3 − 3t+ 2) 6 ‖∇u‖22 + b(2t3 − 3t2 + 1) 12 ‖∇u‖42 = 1− t3 3 P∞(u) + a(t3 − 3t+ 2) 6 ‖∇u‖22 + b(2t3 − 3t2 + 1) 12 ‖∇u‖42. (2.4) Now we claim that tu∗ is unique. In fact, each u satisfies ∫ R3 [λu 2 2 −k∞F (u)] dx < 0. Let t3, t4 > 0 such that ut3 , ut4 ∈ M∞. Then P∞(ut3) = P∞(ut4) = 0. From this and (2.4), we have I∞(ut3) = I∞(ut4) + t33 − t34 3t33 P∞(ut3) + a(2t33 − 3t23t4 + t34) 6t33 ‖∇ut3‖22 + b(3t43 − 3t23t 2 4 − 2t33 + 2t34) 12t23 ‖∇ut3‖42 = I∞(ut4) + a(2t33 − 3t23t4 + t34) 6t33 ‖∇ut3‖22 + b(3t43 − 3t23t 2 4 − 2t33 + 2t34) 12t23 ‖∇ut3‖42 6 X. HU, Y. LAN EJDE-2022/75 and I∞(ut4) = I∞(ut3) + t34 − t33 3t34 P∞(ut4) + a(2t34 − 3t24t3 + t33) 6t34 ‖∇ut4‖22 + b(3t44 − 3t24t 2 3 − 2t34 + 2t33) 12t24 ‖∇ut4‖42 = I∞(ut3) + a(2t34 − 3t24t3 + t33) 6t34 ‖∇ut4‖22 + b(3t44 − 3t24t 2 3 − 2t34 + 2t33) 12t24 ‖∇ut4‖42. The two inequalities above imply t3 = t4. Therefore, tu∗ > 0 is unique. � Lemma 2.2. If u ∈M∞, then there exists tu ≥ 1 such that utu ∈M. Proof. Since u ∈M∞, we have P∞(u) = a 2 ‖∇u‖22 + 3λ 2 ‖u‖22 + b 2 ‖∇u‖42 − 3k∞ ∫ R3 F (u) dx = 0. (2.5) In view of Lemma 2.1, there exists tu > 0 such that utu ∈ M. From (H4), (H6), and (H7), one has 0 = P (utu) = atu 2 ‖∇u‖22 + 3λt3u 2 ‖u‖22 + bt2u 2 ‖∇u‖42 − ∫ R3 [3k(tux) +∇k(tux) · (tux)]F (u) dx = atu 2 ‖∇u‖22 + t3u(−a 2 ‖∇u‖22 − b 2 ‖∇u‖42 + 3k∞ ∫ R3 F (u) dx) + bt2u 2 ‖∇u‖42 − ∫ R3 [3k(tux) +∇k(tux) · (tux)]F (u) dx = a(tu − t3u) 2 ‖∇u‖22 + b(t2u − t3u) 2 ‖∇u‖42 + t3u ∫ R3 [3(k∞ − k(tux))−∇k(tux) · (tux)]F (u) dx ≥ a(tu − t3u) 2 ‖∇u‖22 + b(t2u − t3u) 2 ‖∇u‖42, which implies tu ≥ 1. � Lemma 2.3. If u ∈M, then there exists tu ∈ (0, 1] such that utu ∈M∞. Proof. Since u ∈M, we have P (u) = a 2 ‖∇u‖22 + 3λ 2 ‖u‖22 + b 2 ‖∇u‖42 − ∫ R3 [3k(x) +∇k(x) · x]F (u) dx = 0. In view of Lemma 2.1, there exists tu > 0 such that utu ∈ M∞. From (H4), (H6) and (H7), one has 0 = P∞(utu) = atu 2 ‖∇u‖22 + 3λt3u 2 ‖u‖22 + bt2u 2 ‖∇u‖42 − 3k∞ ∫ R3 F (u) dx = atu 2 ‖∇u‖22 + t3u(−a 2 ‖∇u‖22 − b 2 ‖∇u‖42 + ∫ R3 [3k(x) +∇k(x) · x]F (u) dx) EJDE-2022/75 KIRCHHOFF-SCHRÖDINGER EQUATIONS 7 + bt2u 2 ‖∇u‖42 − 3k∞ ∫ R3 F (u) dx = a(tu − t3u) 2 ‖∇u‖22 + b(t2u − t3u) 2 ‖∇u‖42 + t3u ∫ R3 [3(k(x)− k∞) +∇k(x) · x]F (u) dx ≤ a(tu − t3u) 2 ‖∇u‖22 + b(t2u − t3u) 2 ‖∇u‖42 which implies tu ≤ 1. Therefore tu ∈ (0, 1]. � Lemma 2.4. If u ∈M∞, then u(·− y) ∈M∞ for all y ∈ R3. Moreover, for every y ∈ R3, there exists ty ≥ 1 such that uty (· − y) ∈M and lim|y|→∞ ty = 1. Proof. If u ∈ M∞, then from the translation invariance of I∞ it follows that u(· − y) ∈ M∞ for all y ∈ R3. Furthermore, from Lemma 2.2 there exists ty ≥ 1 such that uty (· − y) ∈ M. By (2.1) and the Lebesgue Dominated Convergence Theorem, we have 0 = lim inf |y|→∞ t−3 y P (uty (· − y)) = lim inf |y|→∞ [ at−2 y 2 ‖∇u‖22 + 3λ 2 ‖u‖22 + bt−1 y 2 ‖∇u‖42] − lim inf |y|→∞ ∫ R3 [3k(tyx+ y) +∇k(tyx+ y) · (tyx+ y)]F (u) dx = lim inf |y|→∞ [ at−2 y 2 ‖∇u‖22 + bt−1 y 2 ‖∇u‖42 − a 2 ‖∇u‖22 − b 2 ‖∇u‖42 + 3 ∫ R3 k∞(x)F (u) dx] − lim inf |y|→∞ ∫ R3 [3k(tyx+ y) +∇k(tyx+ y) · (tyx+ y)]F (u) dx = lim inf |y|→∞ [ a(t−2 y − 1) 2 ‖∇u‖22 + b(t−1 y − 1) 2 ‖∇u‖42] + lim inf |y|→∞ ∫ R3 3[k∞ − k(tyx+ y)− 1 3 ∇k(tyx+ y) · (tyx+ y)]F (u) dx = a 2 (lim inf |y|→∞ t−2 y − 1)‖∇u‖22 + b 2 (lim inf |y|→∞ t−1 y − 1)‖∇u‖42 which implies lim sup|y|→∞ ty = 1, and so lim|y|→∞ ty = 1. � From Jeanjean and Tanaka [7] have that inf u∈M∞ I∞(u) = m∞. Lemma 2.5. m = m∞. Proof. Let u ∈ H1(R3) be the ground state solution (which is positive and radially symmetric) of the problem at infinity, u ∈ M∞ and I∞(u) = m∞. From the translation invariance of the integrals, given any y ∈ R3 such that u(· − y) ∈M∞, I∞(u(· − y)) = m∞. From Lemma 2.4, for any y ∈ R3, there exists a ty ≥ 1 such that uty (· − y) ∈M. Therefore, |I(uty · (−y))−m∞| 8 X. HU, Y. LAN EJDE-2022/75 = |I(uty · (−y))− I∞(u · (−y))| = |a(ty − 1) 2 ‖∇u‖22 + b(t2y − 1) 4 ‖∇u‖42 + λ(t3y − 1) 2 ∫ R3 u2 dx + ∫ R3 (k∞ − t3yk(tyx+ y))F (u) dx| ≤ |a(ty − 1) 2 ‖∇u‖22|+ | λ(t3y − 1) 2 ∫ R3 u2 dx|+ ∫ R3 |k∞ − t3yk(tyx+ y)||F (u)|dx. Since ty → 1 as |y| → ∞, it follows that |I(uty · (−y))−m∞| ≤ oy(1) + oy(1) + ∫ R3 |k∞ − k(x+ y)||F (u)|dx. and since k(x+ y)→ k∞ as |y| → ∞, it follows that lim |y|→∞ I(uty · (−y)) = m∞. Therefore, m = infu∈M I(u) ≤ m∞. On the other hand, we consider u ∈ M and 0 < ty ≤ 1 such that uty ∈ M∞. Since u ∈M, then P (u) = 0 and u satisfies m = I(u) = a 2 ‖∇u‖22 + λ 2 ‖u‖22 + b 4 ‖∇u‖42 − ∫ R3 k(x)F (u) dx = 1 3 P (u) + a 3 ‖∇u‖22 + b 12 ‖∇u‖42 + 1 3 ∫ R3 ∇k(x) · xF (u) dx ≥ aty 3 ‖∇u‖22 + bt2y 12 ‖∇u‖42 ≥ I∞(uty )− 1 3 P∞(uty ) = I∞(uty ) ≥ m∞ where we have used (H4) and (H6). Thus, for any u ∈ M, I(u) ≥ m∞ and hence infu∈M I(u) ≥ m∞. We conclude that m = m∞. � Lemma 2.6. The functional I satisfies condition (Ce) at level d ∈ (m∞, 2m∞). Proof. Since {un} ⊂ H1(R3) is a Cerami sequence (Ce)d, by (H8), we have d+ o(1) = I(un)− 1 4 〈I ′(un), un〉 = 1 4 ∫ R3 a|∇un|2 + λu2 n dx+ 1 4 ∫ R3 a(f(un)un − 4F (un)) dx ≥ 1 4 ‖un‖2λ. This shows {un} is bounded in H1(R3). Applying the splitting lemma cite[Lemma 4.6]l1, up to subsequences, we have un − k∑ j=1 uj(x− yjn)→ u in H1(R3), EJDE-2022/75 KIRCHHOFF-SCHRÖDINGER EQUATIONS 9 where uj is a weak solution of the problem at infinity, |yjn| → ∞ and u is a weak solution of (1.1). Moreover, I(un) = I(u) + k∑ j=1 I∞(uj) + on(1). Since d < 2m∞, it follows that k < 2. If k = 1, we have two cases to distinguish: (1) u 6= 0, which implies I(u) ≥ m∞ and hence I(un) ≥ 2m∞. (2) u = 0, which yields I(un)→ I∞(u1). In both cases we arrive at a contradiction with the fact that d ∈ (m∞, 2m∞). Therefore, we must have k = 0 and the convergence un → u follows. � Definition 2.7. Define the barycenter function of a given function u ∈ H1(R3)\{0} as follows: let µ(u)(x) = 1 |B1| ∫ B1(x) |u(y)|dy, with µ(u) ∈ L∞(R3)) and µ is a continuous function. Subsequently, take µ̂(u)(x) = [µ(u)(x)− 1 2 maxµ(u)]+. It follows that û ∈ C0(R3). Now define the barycenter of u by β(u)(x) = 1 ‖û‖ ∫ R3 xû(x) dx ∈ R3. Since û has compact support, by definition, β(u) is well defined. Now we define b = inf{I(u) : u ∈M, β(u) = 0}. It is clear that b ≥ m∞. Lemma 2.8. b > m∞. Proof. By contradiction, suppose that b = m∞. By the definition of b, there exists a (minimizing) sequence {un} ∈ {u ∈ M, β(u) = 0} such that I(u n ) → b. By Lemma 2.8, the sequence {un} is bounded. Since m = m∞ by Lemma 2.6, then {un} is also a minimizing sequence of I on M. By Ekeland Variational Principle [24, Theorem 8.5] there exists another sequence {ũn} ∈ M such that: (i) I(ũn)→ m; (ii) I ′(ũn)→ 0; (iii) ‖ũn − un‖ → 0. Moreover, {un} is bounded, β(un) = 0 and ‖ũn−un‖ → 0 imply that the sequence {ũn} is bounded and |β(ũn)− β(un)| → 0, since β is a continuous function. So we have that β(ũn) is bounded. Therefore, the sequence {ũn} satisfies the assumptions of [9, Corollary 4.8] and since m = m∞ and is not attained, then the splitting lemma holds with k = 1. This yields ũn(x)→ u1(x− yn), where yn ∈ R3, |y| → ∞, and u1 is a solution of the problem at infinity. By making a translation, we obtain ũn(x+ yn) = u1(x) + on(1). 10 X. HU, Y. LAN EJDE-2022/75 Calculating the barycenter function on both sides, we have β(ũn(x+ yn)) = β(ũn)− yn, where β(ũn) is bounded and β(u1(x) + on(1))→ β(u1(x)), since β is a continuous function. On one side, β(u1(x)) is a fixed real value and, on the other, |yn| → ∞ so we arrive at a contradiction. Therefore, we must have b > m∞. � Inspired by [9], let w ∈ H1(R3) be the positive, radially symmetric, ground state solution of (1.3). We define the operator Π : R3 →M by Π[y](x) = w( x− y ty ) = wty (x− y). Proof of Theorem 1.1. By Lemma 2.2, for any w ∈ M∞, then there exists ty ≥ 1 such that wty = Π[y] ∈M. Therefore P (Π[y]) = 0 for any y ∈ R3, and we have I(Π[y]) = a 2 ‖∇Π[y]‖22 + λ 2 ‖Π[y]‖22 + b 4 ‖∇Π[y]‖42 − ∫ R3 k(x)F (Π[y]) dx = 1 3 P (Π[y]) + a 3 ‖∇Π[y]‖22 + b 12 ‖∇Π[y]‖42 + 1 3 ∫ R3 ∇k(x) · xF (Π[y]) dx = a 3 ‖∇Π[y]‖22 + b 12 ‖∇Π[y]‖42 + 1 3 ∫ R3 ∇k(x) · xF (Π[y]) dx = aty 3 ‖∇w‖22 + bt2y 12 ‖∇w‖42 + t3y 3 ∫ R3 ∇k(tyx+ y) · (tyx+ y)F (w) dx. (2.6) Moreover, since w ∈M∞, we have I∞ = 1 3 P∞(w) + aty 3 ‖∇w‖22 + bt2y 12 ‖∇w‖42 = aty 3 ‖∇w‖22 + bt2y 12 ‖∇w‖42. Combing (2.6) and the above equality yields I(Π[y]) = I∞ + t3y 3 ∫ R3 ∇k(tyx+ y) · (tyx+ y)F (w) dx. By (2.2), it follows that I(Π[y]) → m∞, as |y| → ∞. In view of Lemma 2.8, we have b > m∞. Then there exists ρ̄ > 0 such that for every ρ ≥ ρ̄, m∞ < max |y|=ρ I(Π[y]) < b. To apply the Linking Theorem, we take Q = Π(Bρ̄(0)) and S = {u ∈ M : β(u) = 0}. From [9, Lemma 4.13], we have β(Π[y](x)) = y, ∀y ∈ R3. If u ∈ S, then β(u) = 0, and if u ∈ ∂Q, then β(u) = y 6= 0, because of equality |y| = ρ̄; therefore ∂Q ∩ S = ∅. For any h ∈ H = {h ∈ C(Q,M) : h|∂Q = id}, we define T : Bρ̄(0) → R3 as T [y] = β ◦ h ◦ Π[y]. The function T is continuous. Moreover, for any |y| = ρ̄, we EJDE-2022/75 KIRCHHOFF-SCHRÖDINGER EQUATIONS 11 have Π[y] ∈ ∂Q, thus h ◦ Π[y] = Π[y], T (y) = β(Π[y]) = y. By Brouwer’s Fixed Point Theorem we conclude that there exists ỹ ∈ Bρ̄(0) such that T (ỹ) = 0, which implies h(Π[ỹ]) ∈ S. Therefore h(Q) ∩ S 6= ∅ and S and ∂Q link. If h is fixed, then there exists z ∈ S such that z also belongs to h(Q), which means that z = h(v) form some v ∈ Π(Bρ̄(0)). Therefore, I(z) ≥ inf u∈S I(u) and max u∈Q I(h(u)) ≥ I(h(v)). This gives max u∈Q I(h(u)) ≥ I(h(v)) = I(z) ≥ inf u∈S I(u) = b, and hence d = inf h∈H max u∈Q I(h(u)) ≥ b > m∞. Since w ∈M∞ and m∞ = I∞(w), it follows that m∞ = a 3‖∇w‖ 2 2 + b 12‖∇w‖ 4 2, and P∞(w) = a 2 ‖∇w‖22 + 3λ 2 ‖w‖22 + b 2 ‖∇w‖42 − 3k∞ ∫ R3 F (w) dx = 0. We set t∗ = [ m∞ m∞ − 2β0 ]1/2. Since β0 is the unique positive root of (H5), then 1 < t∗ <∞. Hence I(Π[y]) = aty 2 ‖∇w‖22 + λt3y 2 + bt2y 4 ‖∇w‖42 − t3y ∫ R3 k(tyx+ y)F (w) dx = t3yP ∞(w) + a(3ty − t3y) 6 ‖∇w‖22 + b(3t2y − 2t3y) 12 ‖∇w‖42 + t3y ∫ R3 [k∞ − k(tyx+ y)]F (w) dx ≤ a(3ty − t3y) 6 ‖∇w‖22 + b(3t2y − 2t3y) 12 ‖∇w‖42 + β0t 3 y ≤ a(3t∗ − t3∗) 6 ‖∇w‖22 + b(3t2∗ − 2t3∗) 12 ‖∇w‖42 + β0t 3 ∗ < a 3 ‖∇w‖22 + b 12 ‖∇w‖42 + β0[ m∞ m∞ − 2β0 ]3/2 = 2m∞. Furthermore, if we take h = id, then d = inf h∈H max u∈Q I(h(u)) < max u∈Q I(u) < 2m∞. Then we have d ∈ (m∞, 2m∞), thus from Lemma 2.6, (Ce) condition is satisfied at level d. 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