Electronic Journal of Differential Equations, Vol. 2025 (2025), No. 114, pp. 1–14. ISSN: 1072-6691. URL: https://ejde.math.txstate.edu, DOI: 10.58997/ejde.2025.114 NORMALIZED GROUND STATE SOLUTIONS FOR KIRCHHOFF EQUATION WITH SUBCRITICAL OR CRITICAL PERTURBATION ZIAN FAN Abstract. This article concerns the Kirchhoff equation with subcritical or critical perturbation. We establish the existence of normalized ground state solutions by using Pohozaev manifold and subcritical approximation methods. 1. Introduction and main results In this article, we study the Kirchhoff equation with subcritical or critical perturbation −(a+ b ∫ R3 |∇u|2dx)∆u+ λu = η|u|p−2u+ |u|q−2u in R3,∫ R3 |u|2dx = c, u ∈ H1(R3), (1.1) where a, b > 0 are two constants, 2 < p < q ≤ 2∗ = 6, c, η > 0, λ ∈ R. In the previous two decades, a large number of scholars have studied the existence of nontrivial solutions of the following Kirchhoff type equation −(a+ b ∫ RN |∇u|2dx)∆u+ V (x)u = f(x, u), see [1, 16, 6, 7, 2, 24, 4]. In these references, Alves, Perera and He proved the existence results of the nontrivial solutions by the variational methods. Zhang [24] considered one Kirchhoff equation with critical Sobolev exponent. By Nehari manifold, Chen [4] established the existence of positive solutions to (1.1) for 1 < p < 2 < q < 2∗ in a bounded domain. Recently, more attention is paid to the existence of solutions to nonlinear Schrödinger (NLS) equation with prescribed mass, ∫ RN |u|2dx = c. Such solution is usually called a normalized solution. Soave [17, 18] proved the existence of normalized ground states and properties of ground states for NLS equation −∆u− λu = µ|u|q−2u+ |u|p−2u in RN ,∫ RN |u|2dx = a2, u ∈ H1(RN ), where 2 < q < p ≤ 2∗. Yao [21] studied normalized solutions for the Choquard equations with lower critical exponent −∆u+ λu = γ(Iα ∗ |u| α N +1)|u| α N −1u+ µ|u|q−2u in RN ,∫ RN |u|2dx = c, u ∈ H1(RN ), 2020 Mathematics Subject Classification. 35J15, 35J20, 35J60, 35B33. Key words and phrases. Normalized solutions; Kirchhoff equation; critical growth; Pohozaev manifold. ©2025. This work is licensed under a CC BY 4.0 license. Submitted June 4, 2025. Published December 9, 2025. 1 2 Z. FAN EJDE-2025/114 where α ∈ (0, N), 2 < q ≤ 2N/(N − 2). By employing the Sobolev subcritical approximation method, Li, Nie and Zhang [10] studied the problem (1.1) for η sufficiently large and obtained the existence of normalized ground states. Kong and Chen [8] studied (1.1) in for the case N = 4. By decomposing Pohozaev manifold and constructing fiber map, they proved the existence of a positive normalized ground state. For more references on normalized solution of Kirchhoff equation and Schrödinger equation, we refer to [5, 9, 11, 12, 22, 23, 25, 26]. Motivated by the above papers, we examine the existence of normalized solutions for Kirchhoff equation in the subcritical case 2 < q < 2∗ and the critical case q = 2∗. For subcritical case, by using the constrained minimization method on a suitable submanifold and using Schwartz symmetrization rearrangements we obtain the existence of normalized ground state solutions. For critical case, the main difficulty in solving the problem (1.1) is to study the estimate of Mountain pass Level and prove inf Iq(u) is attained in a suitable submanifold. Firstly we compare the zeros of some functions and study the Mountain pass Level, then we construct an increasing sequence to get the properties of inf Iq(u). Lately in the aid of subcritical approximation method, we prove the existence of normalized ground state solutions for q = 2∗ for any η > 0 . Let E = H1(R3) be the usual Sobolev space equipped with the norm ∥u∥ = (∫ R3 (|∇u|2 + u2)dx )1/2 . The norm of the space Lj(R3)(1 < j ≤ 2∗) is defined as ∥u∥j = (∫ R3 |u|jdx )1/j . Moreover, Er = H1 rad(R3) denotes the subspace of radial functions Er = H1 rad(R3) = {u ∈ H1(R3) : u(x) = u(|x|)}. From [20] we know that the embedding Er → Lj(R3)(2 < j ≤ 2∗) is continuous and compact for 2 < j < 2∗. For 0 ̸= u ∈ D1,2(R3), we define S0 = inf ∫ R3 |∇u|2dx(∫ R3 |u|2∗dx )2/2∗ . We now introduce the main results in this article. Theorem 1.1. Assume that c > 0, 14 3 ≤ p < q < 2∗, then problem (1.1) admits at least a couple of ground state solution (u, λ) ∈ H1(R3)× R for any η > 0. Moreover, the solution is real-valued positive and radially symmetric non-increasing function with λ > 0. Theorem 1.2. Assume that c > 0, 14 3 ≤ p < q, q = 2∗, then problem (1.1) admits at least a couple of ground state solution (u, λ) ∈ H1(R3) × R for any η > 0. Moreover, the solution is real-valued positive and radially symmetric non-increasing function with λ > 0. We set γp = 3(p− 2) 2p , γq = 3(q − 2) 2q . Remark 1.3. Direct calculations show that under the assumption of Theorem 1.1 or Theorem 1.2, it results that p > 2, q > 2, qγq > pγp ≥ 4. 2. Variational framework and technical lemmas In this section, we assume p, q satisfy the conditions of Theorem 1.1 or Theorem 1.2. By Remark 1.3 we know that q > p > 2 and qγq > pγp ≥ 4. The functional associated to (1.1) is Iq(u) = a 2 ∫ R3 |∇u|2dx+ b 4 (∫ R3 |∇u|2dx )2 − η 1 p ∫ R3 |u|pdx− 1 q ∫ R3 |u|qdx EJDE-2025/114 KIRCHHOFF EQUATION WITH SUBCRITICAL OR CRITICAL PERTURBATION 3 = 1 2 A(u) + 1 4 D(u)− 1 p L(u)− 1 q K(u) with the constrain Sc = {u ∈ E : ∫ R3 |u|2dx = c}. Where A(u) = a ∫ R3 |∇u|2dx, D(u) = b (∫ R3 |∇u|2dx )2 , L(u) = η ∫ R3 |u|pdx, K(u) = ∫ R3 |u|qdx. The Gagliardo-Nirenberg inequality can be founded in [19]: ∥u∥q ≤ C(q)∥∇u∥γq 2 ∥u∥1−γq 2 , 2 < q < 2∗. (2.1) If q = 2∗, by using the definition of S0 we obtain∫ R3 |u|2 ∗ dx ≤ S −2∗/2 0 ∥∇u∥2 ∗ 2 . (2.2) Since the embedding H1(R3) → Lj(R3)(2 < j ≤ 2∗) is continuous, then we deduce that Iq ∈ C1(E,R). For u ∈ E, we define Gq(u) = A(u) +D(u)− γpL(u)− γqK(u). If u ∈ E is a solution to the first equation of (1.1), −(a+ b ∫ R3 |∇u|2dx)∆u+ λu = η|u|p−2u+ |u|q−2u in R3, (2.3) then A(u) + λB(u) +D(u) = L(u) +K(u), where B(u) = ∫ R3 u2dx. Moreover, by using an argument similar to [15, 14] we have the identity 1 2 A(u) + λ 3 2 B(u) + 1 2 D(u)− 3 p L(u)− 3 q K(u) = 0. Hence if u ∈ E is a solution to (2.3), then u satisfies the Pohozaev equality Gq(u) = A(u) +D(u)− γpL(u)− γqK(u) = 0. (2.4) Suppose that u ∈ E, by computations we obtain ⟨I ′q(u), ϕ⟩ = (a+ b ∫ R3 |∇u|2dx) ∫ R3 ∇u∇ϕdx− η ∫ R3 |u|p−2uϕdx− ∫ R3 |u|q−2uϕdx for every ϕ ∈ E. Hence the normalized solutions of problem (1.1) are the critical points of the energy functional Iq under the constrain Sc. We say that uc is a ground state of (1.1) on Sc if (uc, λc) ∈ E × R is a normalized solution to (1.1) and uc has the minimal energy among all nontrivial solutions belonging to Sc, that is, Iq(u) = inf{Iq(v) : v ∈ Sc, (Iq |Sc) ′(v) = 0}. Let u ∈ E, and ut = t3/2u(tx), t > 0. By computations we obtain h(t) = Iq(u t) = at2 2 ∫ R3 |∇u|2dx+ bt4 4 (∫ R3 |∇u|2dx )2 − η tpγp p ∫ R3 |u|pdx− tqγq q ∫ R3 |u|qdx. Then Iq(u t) → −∞ as t → +∞, Iq is not bounded from below. Consider the Pohozaev set Mc,q = { u ∈ Sc : Gq(u) = 0 } . 4 Z. FAN EJDE-2025/114 From (2.4) we deduce that if u ∈ E is a solution to (1.1), then u ∈ Mc,q, that is, any critical points of Iq |Sc stay in Mc,q. By computations we obtain h′(t) = tA(u) + t3D(u)− γpt pγp−1L(u)− γqt qγq−1K(u). It is clear that Gq(u) = 0 if and only if h′(1) = 0. Next, we claim that Mc,q is a natural constraint. Lemma 2.1. The following results hold: (i) Mc,q is a smooth manifold of codimension 1 in Sc; (ii) If u ∈ Mc,q is a critical point of Iq |Mc,q , then u is a critical point of Iq |Sc . Proof. (1) Note that Mc,q = {u ∈ E : Gq(u) = 0, G1(u) = 0} , where G1(u) = ∫ R3 |u|2dx− c. Then it is easy to see that Gq(u), G1(u) are of class C1 in E. If G′ q(u) = 0, then by the Lagrange multipliers rule there exists some λ1 ∈ R and u ∈ Mc,q such that G′ q(u) + λ1G1 ′(u) = 0, which implies that −2a∆u− 4b (∫ R3 |∇u|2dx ) ∆u+ 2λ1u = ηpγp|u|p−2u+ qγq|u|q−2u. By Pohozaev equality (2.4) we deduce that 2A(u) + 4D(u) = pγ2 pL(u) + qγ2 qK(u), then −2A(u) + γp(4− pγp)L(u) + γq(4− qγq)K(u) = 0. This contradicts Remark 1.3. Hence we obtain that G′ q(u) ̸= 0 and Mc,q is a smooth manifold of codimension 1 in Sc. (2) If u ∈ Mc,q is a critical point of Iq |Mc,q , by the Lagrange multipliers rule there exists some λ, λ2 ∈ R such that for any φ ∈ E, ⟨I ′q(u), φ⟩+ λ ∫ R3 uφdx+ λ2⟨G′ q(u), φ⟩ = 0, then u satisfies the equation − (2λ2 + 1)a∆u− (4λ2 + 1)b (∫ R3 |∇u|2dx ) ∆u+ λu = η(λ2pγp + 1)|u|p−2u+ (λ2qγq + 1)|u|q−2u. From Pohozaev equality (2.4) we deduce that (2λ2 + 1)A(u) + (4λ2 + 1)D(u) = γp(λ2pγp + 1)L(u) + γq(λ2qγq + 1)K(u). (2.5) Since Gq(u) = 0, then from (2.4) and (2.5) we obtain λ2(−2A(u)− (pγp − 4)γpL(u)− (qγq − 4)γqK(u)) = 0. Then we obtain that λ2 = 0, the proof is complete. □ Lemma 2.2. For any u ∈ Sc, there exists a unique t0 such that ut0 ∈ Mc,q and Iq(u t0) = max t>0 Iq(u t). Moreover, if Gq(u) ≤ 0, then 0 < t0 ≤ 1. EJDE-2025/114 KIRCHHOFF EQUATION WITH SUBCRITICAL OR CRITICAL PERTURBATION 5 Proof. Suppose that u ∈ Sc, then h(t) = Iq(u t) = t2 2 A(u) + t4 4 D(u)− tpγp p L(u)− tqγq q K(u), h′(t) = tA(u) + t3D(u)− γpt pγp−1L(u)− γqt qγq−1K(u), = t3(t−2A(u) +D(u)− γpt pγp−4L(u)− γqt qγq−4K(u)) = t3g(t). Then it is clear that h(0) = 0 and h(t) → −∞ as t → +∞. There exists t0 such that h′(t) > 0 for t ∈ (0, t0) and h′(t) < 0 for t ∈ [t0, t1), t1 > t0 > 0, it follows that h(t) achieves its local maximum at t = t0 and h′(t0) = 0. Since pγp ≥ 4 and qγq > 4, then g(t) is strictly decreasing. On the other hand, we have {t > 0 : h′(t) = 0} = {t > 0 : g(t) = 0}, which implies that h(t) has a positive unique critical point which corresponds to its maximum. By computations we have Gq(u t0) = t0[at0 ∫ R3 |∇u|2dx+ bt30 (∫ R3 |∇u|2dx )2 − γpt pγp−1 0 L(u)− γqt qγq−1 0 K(u)] = t0h ′(t0). From h′(t0) = 0, we obtain that Gq(u t0) = 0 and ut0 ∈ Mc,q. Suppose Gq(u) ≤ 0, we claim that 0 < t0 ≤ 1. Assume by contradiction that t0 > 1, using that Gq(u t0) = 0 we obtain 0 = Gq(u t0) = t40[t −2 0 A(u) +D(u)− γpt pγp−4 0 L(u)− γqt qγq−4 0 K(u)] < t40[A(u) +D(u)− γpL(u)− γqK(u)] = t40Gq(u) ≤ 0, which is a contradiction, then 0 < t0 ≤ 1. This completes the proof. □ Let u ∈ Mc,q, we obtain Iq(u) = Iq(u)− 1 4 Gq(u) = 1 4 A(u) + ( γp 4 − 1 p )L(u) + ( γq 4 − 1 q )K(u). (2.6) In view of Remark 1.3, we deduce that Iq(u) > 0 and Iq(u) is bounded below on Mc,q. Since that Iq(u) is bounded below on Mc,q, we may define m(c, q) = inf u∈Mc,q Iq(u). Lemma 2.3. There exists C1 = C1(a, p, q, η) > 0 such that m(c, q) > C1. Proof. Let u ∈ Mc,q. Then A(u) +D(u) = γpL(u) + γqK(u) ≥ a0∥∇u∥22, (2.7) where a0 = min{1, a}. Using (2.1)-(2.2) and (2.7) we can deduce that a0 ≤ ηC(p)γp∥∇u∥pγp−2 2 c p(1−γp) 2 + C(q)γq∥∇u∥qγq−2 2 c q(1−γq) 2 , 2 < q < 2∗, a0 ≤ ηC(p)γp∥∇u∥pγp−2 2 c p(1−γp) 2 + γqS −2∗ 2 0 ∥∇u∥2 ∗−2 2 , q = 2∗. Then there exists C > 0 such that ∥∇u∥22 > C > 0. It follows from (2.6)-(2.7) that Iq(u) ≥ 1 4 A(u) = a 4 ∥∇u∥22. (2.8) Then there exists C1 = C1(a, p, q, η) > 0 such that m(c, q) > C1. □ 6 Z. FAN EJDE-2025/114 3. Proof of Theorem 1.1 In this section, we study the subcritical case 14 3 ≤ p < q < 2∗. From Remark 1.3 we have q > p > 2, qγq > pγp ≥ 4. Let {un} ⊂ Mc,q be a minimizing sequence for Iq(u), that is lim n→∞ Iq(un) = inf u∈Mc,q Iq(u) = m(c, q). Then we have the following Lemma. Lemma 3.1. Under the assumption of Theorem 1.1, m(c, q) is attained by a real- valued positive and radially symmetric non-increasing function. Proof. Let vn = |un|∗ be the Schwartz symmetrization rearrangement of |un|. Then by [13] we obtain A(vn) ≤ A(un), D(vn) ≤ D(un), B(vn) = B(un) = c, (3.1) K(vn) = K(un), L(vn) = L(un). (3.2) Therefore, Iq(vn) ≤ Iq(un), Gq(vn) ≤ Gq(un) = 0. Since vn ∈ Sc, then by Lemma 2.2 there exists a unique 0 < tn ≤ 1 such that {vtnn } ⊂ Mc,q, where vtnn = t 3/2 n vn(tnx). From (3.1) and (3.2) we deduce that m(c, q) ≤ Iq(v tn n ) = Iq(v tn n )− 1 pγp Gq(v tn n ) = ( 1 2 − 1 pγp )t2nA(vn) + ( 1 4 − 1 pγp )t4nD(vn) + ( γq pγp − 1 q )tqγq n K(vn) ≤ ( 1 2 − 1 pγp )A(un) + ( 1 4 − 1 pγp )D(un) + ( γq pγp − 1 q )K(un) = Iq(un)− 1 pγp Gq(un) = Iq(un) → m(c, q) as n → ∞. Then we obtain that Iq(v tn n ) → m(c, q), n → ∞. Hence {vtnn } is a minimizing sequence for Iq(u). We claim {vtnn } is bounded in E. Otherwise, if ∥vtnn ∥ → ∞ as n → ∞, then by (2.8) we have that Iq(v tn n ) → ∞, that is a contradiction. Therefore {vtnn } is bounded in E. We can extract a subsequence(still denoted {vtnn }) and v ∈ E such that vtnn ⇀ v in Er; vtnn → v in Li(R3)(2 < i < 2∗), vtnn → v a.e. in R3 as n → ∞. Therefore we obtain K(vtnn ) → K(v), L(vtnn ) → L(v). On the other hand, by Lemma 2.3, we have 0 < C1 < m(c, q) ≤ Iq(v tn n ) = Iq(v tn n )− 1 2 Gq(v tn n ) = −1 4 t4nD(vtnn ) + ( γp 2 − 1 p )tpγp n L(vtnn ) + ( γq 2 − 1 q )tqγq n K(vtnn ) ≤ ( γp 2 − 1 p )L(vtnn ) + ( γq 2 − 1 q )K(vtnn ) EJDE-2025/114 KIRCHHOFF EQUATION WITH SUBCRITICAL OR CRITICAL PERTURBATION 7 → ( γp 2 − 1 p )L(v) + ( γq 2 − 1 q )K(v), which implies that v ̸= 0. Moreover, by Fatou’s Lemma, Gq(v) = A(v) +D(v)− γpL(v)− γqK(v) ≤ lim inf n→∞ [A(vtnn ) +D(vtnn )]− γp lim n→∞ L(vtnn )− γq lim n→∞ K(vtnn ) = lim inf n→∞ Gq(v tn n ) = 0, which implies that Gq(v) ≤ 0. (3.3) Next we shall prove that ∫ R3 |v|2dx = c. Set 0 < ∫ R3 |v|2dx = c1 ≤ c, ξ = c1 c , v1(x) = ξ 1 q−2 v(ξ q 3q−6x). Note that 2 < p < q < 6. Then A(v1) = ξ 6−q 3q−6A(v) ≤ A(v), B(v1) = c, D(v1) ≤ D(v), (3.4) L(v1) = ξ p−q q−2L(v) ≥ L(v), K(v1) = K(v). (3.5) It follows from (3.3)-(3.5) that Gq(v1) ≤ Gq(v) ≤ 0. From Lemma 2.2, there exists a unique 0 < τ ≤ 1 such that Gq(v τ 1 ) = 0 and vτ1 ∈ Mc,q. Then by using (3.4) and (3.5) we deduce that m(c, q) ≤ Iq(v τ 1 ) = Iq(v τ 1 )− 1 pγp G(vτ1 ) = ( 1 2 − 1 pγp )τ2A(v1) + ( 1 4 − 1 pγp )τ4D(v1) + ( γq pγp − 1 q )τ qγqK(v1) ≤ ( 1 2 − 1 pγp )A(v) + ( 1 4 − 1 pγp )D(v) + ( γq pγp − 1 q )K(v) ≤ ( 1 2 − 1 pγp ) lim inf n→∞ A(vtnn ) + ( 1 4 − 1 pγp ) lim inf n→∞ D(vtnn ) + ( γq pγp − 1 q ) lim n→∞ K(vtnn ) = lim inf n→∞ [Iq(v tn n )− 1 pγp Gq(v tn n )] = m(c, q). (3.6) Which implies that Iq(v τ 1 ) = m(c, q). We claim that τ = 1, ξ = 1. Otherwise, if 0 < τ < 1 or 0 < ξ < 1, we replace ≤ with < in (3.6) and get a contradiction. Therefore we deduce that Iq(v τ 1 ) = m(c, q), τ = 1, v1 = v, c = c1. We deduce that m(c, q) is attained by a real-valued nonnegative and radially symmetric non- increasing function. By strong maximum principle v > 0, then v is positive. □ Proof of Theorem 1.1. From Lemma 3.1 we know that v is a critical point of Iq |Mc,q and v ∈ Mc,q is a real-valued positive and radially symmetric non-increasing function. It follows from Lemma 2.1 that v is a critical point of Iq |Sc . By using the Lagrange multipliers rule there exists some λ ∈ R such that for any φ ∈ E ⟨I ′q(v), φ⟩+ λ ∫ R3 vφdx = 0, then v satisfies the equation −(a+ b ∫ R3 |∇v|2dx)∆v + λv = η|v|p−2v + |v|q−2v. 8 Z. FAN EJDE-2025/114 Since γp < 1, γq < 1, then from Pohozaev equality (2.4) we obtain λ ∫ R3 v2dx = (1− γp)L(v) + (1− γq)K(v) > 0, consequently, λ > 0. The proof is complete. □ 4. Proof of Theorem 1.2 Now we turn to the critical case 14 3 ≤ p < q, q = 2∗. In this case, we have m(c, 2∗) = inf u∈Mc,2∗ I2∗(u). We define qn = 2∗ − 1 n > 2, n = 1, 2..., then {qn} is increasing and qn → 2∗ as n → ∞. We first give the following properties of m(c, qn). Lemma 4.1. The following results hold: (i) lim infn→∞ m(c, qn) > 0; (ii) lim supn→∞ m(c, qn) ≤ m(c, 2∗). Proof. Item (i) follows from Lemma 2.3. (ii) From the definition of m(c, 2∗) there exists u ∈ Mc,2∗ such that I2∗(u) < m(c, 2∗) + ε, 0 < ε < 1. (4.1) Let ut = t3/2u(tx), t > 0. It is clear that h1(t) = Iqn(u t) = t2 2 A(u) + t4 4 D(u)− tpγp p L(u)− tqnγqn qn Kn(u), where Kn(u) = ∫ R3 |u|qndx. Note that |u|qn ≤ |u|2 + |u|2∗ and |u|qn → |u|2∗ as n → ∞, then from Lebesgue dominated convergence theorem we obtain tqnγqn qn ∫ R3 |u|qndx = t 3qn−6 2 qn ∫ R3 |u|qndx → t2 ∗ 2∗ ∫ R3 |u|2 ∗ dx. Which implies that |Iqn(ut)− I2∗(u t)| < ε. (4.2) On the other hand, it is easy to see that h1(0) = 0 and h1(t) → −∞ as t → +∞. By the proof of Lemma 2.2, we deduce that h1(t) achieves its unique maximum at t = t0 for t0 ∈ [0, t1), t1 > t0 > 0. Moreover, we have ut0 ∈ Mc,qn . Since u ∈ Mc,2∗ , it follows that I2∗(u) = max t>0 I2∗(u t). From (4.1) and (4.2), we obtain m(c, qn) ≤ Iqn(u t0) ≤ I2∗(u t0) + ε ≤ I2∗(u) + ε < m(c, 2∗) + 2ε, which implies that lim sup n→∞ m(c, qn) ≤ m(c, 2∗). The proof is complete. □ Let Bδ(0) be a ball centered at the origin with radius δ > 0. Let ρ(x) ∈ C∞ 0 (R3) be a radial cut-off function such that ρ(x) = 1 for |x| ≤ δ and ρ(x) = 0 for |x| ≥ 2δ, where |∇ρ(x)| ≤ C,B2δ(0) ⊂ R3. Let 0 < ε < 1, we choose the function uε(x) as follows uε(x) = ρ(x)Uε(x), EJDE-2025/114 KIRCHHOFF EQUATION WITH SUBCRITICAL OR CRITICAL PERTURBATION 9 where Uε(x) = (3ε2)1/4 (ε2 + |x|2)1/2 . If ε > 0 is small enough, by using [14] we have that the function uε(x) satisfies∫ R3 |∇uε|2dx = S 3/2 0 +O(ε); (4.3)∫ R3 |uε|2 ∗ dx = S 3/2 0 +O(ε3); (4.4)∫ R3 |uε|2dx = C2ε+O(ε2). (4.5) Where C2 is a positive constant independent of ε. By computations we have∫ Ω |uε|pdx ≥  C3ε 3− p 2 , p > 3, C3ε 3/2|ln ε|, p = 3, C3ε p/2, p < 3, (4.6) where C3 is a positive constant independent of ε. We set 0 < ∫ R3 |uε|2dx = c2, ξ1 = c2 c , vε(x) = ξ 1/4 1 uε(ξ 1/2 1 x). By computations we have A(vε) = A(uε), B(vε) = c, D(vε) = D(uε), (4.7) L(vε) = ξ p−6 4 1 L(uε), K(vε) = K(uε). (4.8) Lemma 4.2. Under the assumption of Theorem 1.2, we have 0 < m(c, 2∗) < ( 1 2 − 1 2∗ )ay1 + ( 1 4 − 1 2∗ )by21 = c∗, where y1 is given in the following discussion. Proof. From Lemma 2.3, we obtain m(c, 2∗) > 0. We will show m(c, 2∗) < c∗. Since B(vε) = c, from Lemma 2.2, there exists a unique τ0 such that vτ0ε ∈ Mc,2∗ and I2∗(v τ0 ε ) = max t>0 I2∗(v t ε). Consider the function H(t) = I2∗(v t ε) = at2 2 ∫ R3 |∇vε|2dx+ bt4 4 (∫ R3 |∇vε|2dx )2 − η tpγp p ∫ R3 |vε|pdx− t2 ∗ 2∗ ∫ R3 |vε|2 ∗ dx. By using (4.7) and (4.8) we deduce H(t) = t2 2 A(uε) + t4 4 D(uε)− tpγp p ξ p−6 4 1 L(uε)− t2 ∗ 2∗ K(uε). We set H1(t) = 1 2 at2∥∇uε∥22 + bt4 4 ∥∇uε∥42 − t2 ∗ 2∗ ∫ R3 |uε|2 ∗ dx. Then from (4.3) and (4.4) we have H1(t) ≤ H2(t) + C3(t)ε 3 + C4(t)ε, (4.9) and H2(t) = a 2 t2Sβ 0 + bt4 4 S2β 0 − t2 ∗ 2∗ Sβ 0 , β = 3 2 . By the same argument as in Lemma 2.2, we deduce that H2(t) achieves its maximum at t = t2 > 0 and aSβ 0 + bt22S 2β 0 − t2 ∗−2 2 Sβ 0 = 0. (4.10) 10 Z. FAN EJDE-2025/114 We consider the function F (t) = a+ bt− S −2∗ 2 0 t 2∗−2 2 , t > 0. Suppose y1 is the unique zero of F (t), then by (β − 1) 2 ∗ 2 = β, we know that y1 and t22S β are both zeros of the function F (t). Since the zero of the function F (t) is unique for some t > 0, then we deduce that y1 = t22S β 0 . From (4.10) we obtain H2(t) ≤ H2(t2) = a 2 t22S β 0 + bt42 4 S2β 0 − t2 ∗ 2 2∗ Sβ 0 = (1 2 − 1 2∗ ) at22S β 0 + (1 4 − 1 2∗ ) bt42S 2β 0 = ( 1 2 − 1 2∗ )ay1 + ( 1 4 − 1 2∗ )by21 = c∗. (4.11) By using (4.5), (4.6) and (4.9)-(4.11) we deduce that H(t) ≤ H2(t2) + C4ε 3 + C4ε− C5τ pγp 0 ξ p−6 4 1 L(uε) ≤ c∗ + C4ε 3 + C4ε− C5ητ pγp 0 c 6−p 4 c p−6 4 2 L(uε) ≤ c∗ + C4ε 3 + C4ε− C5ητ pγp 0 c 6−p 4 ε 6−p 4 , (4.12) where Ci (i = 4, 5) are positive constants independent of ε. We claim that there exists a constant M1 independent of ε such that τ0 ≤ M1. If τ0 → ∞ as ε → 0, then H(τ0) → −∞ and m(c, 2∗) ≤ 0, which contradicts m(c, 2∗) > 0. On the other hand, since 0 is a local minimum of H(t), there exists a constant M2 independent of ε such that H(τ0) ≥ M2 > 0. This implies that there exists a constant M3 independent of ε such that τ0 ≥ M3 > 0. Note that p > 2, then 6− p 4 < 1. (4.13) By (4.12) and (4.13) we deduce that m(c, 2∗) ≤ sup t>0 H(t) < c∗. The proof is complete. □ The proof of the following Lemma can be founded in [3]. Lemma 4.3. Let N ≥ 3 and 1 ≤ t < +∞. If u ∈ Lt(RN ) is a radial non-increasing function, then one has |u(x)| ≤ |x|−N/t( N |SN−1| )∥u∥t, x ̸= 0, where |SN−1| is the area of the unit sphere in RN . Lemma 4.4. Under the assumption of Theorem 1.2, m(c, 2∗) is attained by a real-valued positive and radially symmetric non-increasing function. Proof. For qn = 2∗ − 1 n , by Lemma 3.1, m(c, qn) is attained by a sequence of real-valued positive and radially symmetric non-increasing functions {un}, and {un} ⊂ Mc,qn , Iqn(un) = m(c, qn). From the proof of Theorem 1.1 we know that there exists λn > 0 such that un satisfies −(a+ b ∫ R3 |∇un|2dx)∆un + λnun = η|un|p−2un + |un|qn−2un. (4.14) From Pohozaev equality (2.4) we obtain λn ∫ R3 u2 ndx = (1− γp)L(un) + (1− γqn)K(un), which implies that {λn} is bounded. Then there exists λ > 0 such that up to a subsequence, limn→∞ λn = λ. EJDE-2025/114 KIRCHHOFF EQUATION WITH SUBCRITICAL OR CRITICAL PERTURBATION 11 From the proof of Lemma 3.1 we deduce that {un} is bounded in Er. We can extract a subsequence (still denoted un) and w ∈ Er such that un ⇀ w in Er, un → w in Li(R3)(2 < i < 2∗), un → w a.e. in R3a as n → ∞. Then {|un|p−2un} is bounded in L p p−1 (R3), which implies that∫ R3 |un|p−2unφdx → ∫ R3 |u|p−2uφdx for φ ∈ C∞ 0 (R3). Note that For ϕ ∈ Lt(R3), t > 1, by the Young inequality, the Hölder inequality and Lemma 4.3 there exists a constant C > 0 independent of n such that ||un|qn−2unϕ| ≤ C(|un|2−1|ϕ|+ |un|2 ∗−1|ϕ|) ≤ C(|x|− 1 2 |ϕ|+ |x| −(2∗−1) 2 |ϕ|) ∈ L1(R3). By using the Lebesgue dominated convergence theorem and passing to the limit in (4.14) we obtain for φ ∈ C∞ 0 (R3), 0 = ⟨I ′qn(un), φ⟩ → ⟨I ′2∗(w), φ⟩. Therefore w is a solution of the equation −(a+ b ∫ R3 |∇w|2dx)∆w + λw = η|w|p−2u+ |w|2 ∗−2w. Then G2∗(w) = 0. We claim that w ̸= 0. Otherwise, we assume that un ⇀ w = 0, then from (3.3) we have L(un) → 0. (4.15) From Young inequality we obtain |un|qn ≤ 2∗ − qn 2∗ − θ |un|θ + qn − θ 2∗ − θ |un|2 ∗ , 2 < θ < qn < 2∗. On the other hand, by using the definition of S0 we obtain∫ R3 |u|2 ∗ dx ≤ S −2∗ 2 0 (∫ R3 |∇un|2dx )2∗/2 . Hence we deduce that Kn(un) = ∫ R3 |un|qndx ≤ qn − θ 2∗ − θ S −2∗ 2 0 (∫ R3 |∇un|2dx )2∗/2 + o(1). (4.16) Note that un ∈ Mc,qn , then 0 = Gqn(un) = A(un) +D(un)− γpL(un)− γqnKn(un). (4.17) From the proof of Lemma 2.3, there exists a constant C > 0 such that ∥∇un∥22 ≥ C > 0, then we may therefore assume that lim inf n→∞ ∫ R3 |∇un|2dx = l, l > 0. Let n → ∞, from (4.15)-(4.17) we have a+ bl − S −2∗ 2 0 l 2∗−2 2 ≤ 0, l > 0. (4.18) We set F (y) = a+ by − S −2∗ 2 0 y 2∗−2 2 , y > 0, where F (y) has been defined in the proof of Lemma 4.2. From F ′(y) = 0 we obtain y = y0 > 0 and F (0) = a > 0. it is easy to see that F (y) → −∞ as y → +∞. Moreover we have F ′(y) > 0 12 Z. FAN EJDE-2025/114 for y ∈ [0, y0) and F ′(y) < 0 for y ∈ [y0,∞). It follows that F (y) achieves its maximum at y = y0. If y > 0, then F (y) have only one zero point y = y1 > 0. Since F (y1) = 0, we deduce that a+ by1 − S −2∗ 2 0 y 2∗−2 2 1 = 0. (4.19) From (4.18) and (4.19) we deduce that l ≥ y1. By using Lemma 4.1 and (4.15) we obtain m(c, 2∗) ≥ lim sup n→∞ m(c, qn) = lim sup n→∞ Iqn(un) = lim sup n→∞ [Iqn(un)− 1 qnγqn Gqn(un)] = lim sup n→∞ [( 1 2 − 1 qnγqn )A(un) + ( 1 4 − 1 qnγqn )D(un)] ≥ lim inf n→∞ [( 1 2 − 1 qnγqn )A(un) + ( 1 4 − 1 qnγqn )D(un)] = a( 1 2 − 1 2∗ )l + b( 1 4 − 1 2∗ )l2 ≥ a( 1 2 − 1 2∗ )y1 + b( 1 4 − 1 2∗ )y21 = c∗. Which contradicts Lemma 4.2, so we obtain w ̸= 0. We set 0 < ∫ R3 |w|2dx = c3 ≤ c, ξ2 = c3 c , w1(x) = ξ 1/4 2 w(ξ 1/2 2 x). Then by computation we have A(w1) = A(w), B(w1) = c, D(w1) = D(w). (4.20) L(w1) = ξ p−6 4 2 L(w) ≥ L(w), K(w1) = K(w), (4.21) which implies that G2∗(w1) ≤ G2∗(w) ≤ 0. From Lemma 2.2, there exists a unique 0 < σ ≤ 1 such that G2∗(w σ 1 ) = 0 and wσ 1 ∈ Mc,2∗ . Then by Lemma 4.1, (4.20), and (4.21), we deduce that m(c, 2∗) ≤ I2∗(w σ 1 ) = I2∗(w σ 1 )− 1 pγp G2∗(w σ 1 ) = ( 1 2 − 1 pγp )σ2A(w1) + ( 1 4 − 1 pγp )σ4D(w1) + ( γ2∗ pγp − 1 2∗ )σ2∗ ∫ R3 |w1|2 ∗ dx ≤ ( 1 2 − 1 pγp )A(w) + ( 1 4 − 1 pγp )D(w) + ( γ2∗ pγp − 1 2∗ ) ∫ R3 |w|2 ∗ dx ≤ lim inf n→∞ [( 1 2 − 1 pγp )A(un) + ( 1 4 − 1 pγp )D(un) + ( γqn pγp − 1 qn ) ∫ R3 |un|qndx] ≤ lim inf n→∞ [Iqn(un)− 1 pγp Gqn(un)] = lim inf n→∞ Iqn(un) = lim inf n→∞ m(c, qn) ≤ lim sup n→∞ m(c, qn) ≤ m(c, 2∗). By a similar method to that of Lemma 3.1, we have I2∗w σ 1 ) = m(c, 2∗), σ = 1, w1 = w, c = c3, then we deduce that m(c, 2∗) is attained by a real-valued nonnegative and radially symmetric non-increasing function. By strong maximum principle v > 0, then v is positive. □ EJDE-2025/114 KIRCHHOFF EQUATION WITH SUBCRITICAL OR CRITICAL PERTURBATION 13 Proof of Theorem 1.2. From Lemma 4.4 we know that w is a critical point of I2∗ |Mc,2∗ and w ∈ Mc,2∗ is a real-valued positive and radially symmetric non-increasing function. It follows from Lemma 2.1 that w is a critical point of I2∗ |Sc . By using the Lagrange multipliers rule there exists some λ ∈ R such that for any φ ∈ E, ⟨I ′2∗(w), φ⟩+ λ ∫ R3 wφdx = 0. Then w satisfies −(a+ b ∫ R3 |∇u|2dx)∆u+ λu = η|u|p−2u+ |u|2 ∗−2u. Similarly to the proof of Theorem 1.1, we have λ > 0, The proof is complete. □ Acknowledgements. 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