Electronic Journal of Differential Equations, Vol. 2025 (2025), No. 110, pp. 1–11. ISSN: 1072-6691. URL: https://ejde.math.txstate.edu, DOI: 10.58997/ejde.2025.110 SOLUTIONS TO MAGNETIC SCHRÖDINGER EQUATIONS WITH ARBITRARY GROWTH AT INFINITY WENDY F. ALMEIDA, GIOVANY M. FIGUEIREDO Abstract. This work addresses the existence of at least one radial solution to the nonlinear magnetic Schrödinger equation( ε i ∇−A(x) )2 u+ V (x)u = f(|u|2)u in RN , where both the magnetic potential A and the electric potential V are continuous, radial func- tions. Our main tool is the penalization method developed by del Pino and Felmer [17], which we adapt to the complex-valued setting under magnetic effects. By using the small parameter ε and radial symmetry, we handle nonlinearities with arbitrary growth. 1. Introduction The purpose of this article is to investigate the magnetic Schrödinger equation(ε i ∇−A(x) )2 u+ V (x)u = f(|u|2)u in RN , (1.1) LE1 where u : RN → C is an unknown function, N ≥ 3, i represents the imaginary unit, A = (A1, . . . , AN ) : RN → RN denotes the magnetic (or vector) potential, V : RN → R+ a potential continuous and the nonlinear term f :R+ → R is a regular function that satisfies appropriate conditions with arbitrary growth. A standing wave solution for (1.1) is a solution of the form ψ(x, t) = eiωtu(x), (1.2) where ω ∈ R is a real frequency, and u : RN → C is a spatial function to be determined. Rewriting (1.1) in terms of ψ(x, t), we have(ε i ∇−A(x) )2 ψ + V (x)ψ = f(|ψ|2)ψ − i ∂ψ ∂t in RN . (1.3) Thus, the function ψ satisfies the time-dependent Schrödinger equation with a frequency ω. The parameter ε in (1.1) represents the Planck constant, typically denoted by ℏ in quantum mechanics. This constant plays a fundamental role in distinguishing quantum mechanics from classical mechanics. In the limit as ε → 0, the quantum effects vanish, and the equation transi- tions to a classical regime, where the motion of particles follows Newtonian mechanics. Conversely, for nonzero values of ε, wave-particle duality emerges, and solutions of the equation exhibit inter- ference and localization effects characteristic of quantum systems. The presence of the magnetic potential A(x) further highlights the influence of the electromagnetic field on the quantum behav- ior of particles, modifying their trajectories according to the principles of gauge theory. For more details on the physical motivations, see [21, 22, 24]. Recently, the study of magnetic Schrödinger equations has been approached from various per- spectives, however only a limited number of works have addressed this topic. For instance, in [15], the authors investigate the existence of standing waves for a class of nonlinear Schrödinger equations in RN , incorporating both electric and magnetic fields. Under suitable non-degeneracy 2020 Mathematics Subject Classification. 35B33, 35J20, 35Q55. Key words and phrases. Magnetic Schrödinger equations; arbitrary growth at infinity. ©2025. This work is licensed under a CC BY 4.0 license. Submitted September 27, 2025. Published November 24, 2025. 1 2 W. F. ALMEIDA, G. M. FIGUEIREDO EJDE-2025/110 assumptions on the critical points of an auxiliary function associated with the electric field, they establish the existence and multiplicity of complex-valued solutions in the semiclassical limit. Moreover, they demonstrate that in this limit, while the presence of a magnetic field induces a phase shift in the complex wave, it does not affect the spatial localization of the wave’s modulus peaks. In [16], a magnetic Schrödinger equation was analyzed in the context of competition between electric potentials. In [7], the authors investigate the existence of infinitely many geometrically distinct solutions to problem (1.1), considering nonlinearities f with either subcritical or critical growth. Using a finite-dimensional reduction approach, [8] and [10] establish a multiplicity result for (1.1). Another multiplicity results can be seen in [4, 5, 6, 18, 23]. For further significant contributions to the study of the magnetic Schrödinger equation, we refer the reader to [3, 9, 11, 12, 14, 25, 28] and the references therein. Throughout this article, we use the following assumptions: (A1) A is a radial continuous function, that is A ∈ C(RN ,RN ) and if |x| = |y| then A(x) = A(y); (A2) The potential V is a radial continuous function and there are positive constants R1 < r1 < r2 < R2 such that: (i) A(x) = (0, . . . , 0) ∈ RN in the set Ω = {x ∈ RN : r1 < |x| < r2}, (ii) V (x) = 0 in the set Ω = {x ∈ RN : r1 < |x| < r2}, (iii) there exists V0 > 0 such that V (x) ≥ V0 in the set Λc = BR1 ⋃ Bc R2 ; (A3) f ∈ C(R+,R) and lims→0+ f(s) = 0 and f(s) = 0 for all s ≤ 0; (A4) There exists θ > 2 such that f(s)s − θF (s) > 0 for every s ∈ R with s > 0 where F (s) = ∫ s 0 f(t) dt; (A5) The function s→ f(s) is non-decreasing for s > 0. Now we give typical examples of functions A(x) and V (x) satisfying conditions (A1) and (A2). Let Ai(x) =  r1 − |x|, |x| < r1, 0, r1 ≤ |x| ≤ r2, |x| − r2, |x| > r2, for i = 1, . . . N . In this case A is radial and A(x) = (0, . . . , 0) if r1 < |x| < r2, satisfying condition (A2)(i). Let V (x)−  exp( 1 |x|2−r1 ), x ∈ Br1(0), 0, x ∈ Br2 ∩Bc r1 , |x|2 − 2r2x+ r22, x ∈ Bc r2 . This function is continuous and satisfies the conditions (ii) and (iii) in (A2). Both functions A and V are continuous and radial, ensuring symmetry with respect to the origin. Now we state the main result in this article. mainresult Theorem 1.1. Suppose that N ≥ 3 and (A1)–(A5) hold. Then, there exists ε0 > 0 such that for all ε ∈ (0, ε0) problem (1.1) admits a nontrivial complex solution uε with |uε(x)| → 0 as |x| → +∞ and |uε| ∈ L∞(RN ) ∩ C1,λ loc (RN ), for λ ∈ (0, 1). Elliptic problems with arbitrary growth can be found as partial differential equations where the growth term can be nonlinear and increase uncontrollably wit respect to the unknown variable or its derivatives. For example, the authors in [2], analyzed the problem −ε2∆u+ V (x)u = f(u) in RN , which exhibits superlinear growth at infinity, without imposing any constraints on the growth of the function f . Utilizing the force of the parameter ε, the space of radial functions, and the penalization method introduced by Del Pino and Felmer [17], they establish the existence of solutions. The particular case f(t) = tp with p > 1 was studied in [1]. Additionally, an extension of [2] to a Hamiltonian system was investigated in [13]. EJDE-2025/110 MAGNETIC SCHRÖDINGER EQUATIONS 3 Other approaches have been used. For instance, in [30], the existence of infinitely many so- lutions was demonstrated for various elliptic problems under Dirichlet and Neumann boundary conditions. this was also done for a Hamiltonian system, considering nonlinearities exhibiting sub- linear behavior at the origin. The methodology involved modifying the nonlinearity and obtaining solutions with small L∞ norms, ensuring that each solution of the modified problem corresponded to a solution of the original problem. The case studied in [30], where the nonlinearity could change sign, was explored in [20]. In [19], a Kirchhoff problem was analyzed, considering nonlinearities that exhibit both sublinear and linear behavior at the origin, employing the strategy introduced in [30]. The main contributions of this article are as follows: (1) When the growth of the nonlinearity is not bounded by a polynomial function of controlled order, classical methods such as Sobolev embeddings may not directly apply. To overcome this difficulty we are adapting to our case the arguments that can be found in [1, 2, 13]. However, with respect to [1, 2, 13], due to the presence of the magnetic potential A and the fact that the solutions assume complex values, a more careful analysis will be needed and some refined estimates will be given in Lemmas 3.3, 4.1, and 4.2. (2) Proving the existence of weak solutions can be challenging, especially if the growth of the nonlinearity does not satisfy suitable structural conditions. For this reason, it was necessary to put forward appropriate hypotheses on the magnetic potential A that were compatible with the existing hypotheses about the electrical potential V . This is another point that differs our article from the articles [1], [2] and [13] that consider solutions that assume real values and A = 0. (3) Even if existence is guaranteed, proving sufficient regularity for the solutions can be com- plicated, as arbitrary growth may generate instabilities or singularities. Once again, due to the presence of the magnetic potential A and the fact that the solutions assume complex values, it was necessary to use Moser’s iteration method in Lemma 4.2. This article is organized as follows. In Section 2 we introduce the Banach space where we will look for the solution to the problem and we recall an important inequality called the diamagnetic inequality. In Section 3 we use the Del Pino Felmer Penalization [17]. With this penalty and the fact that we are in the space of radial functions, we get around the difficulty of having an arbitrary growth. In fact, it is possible to obtain a functional associated to the penalized problem. In this section we show that this functional has the Geometry of the Mountain Pass Theorem and that Palais-Smale sequences have strongly convergent subsequences. In Section 4, using the strength of the parameter ε and the fact that we obtain a radial solution to the penalized problem, we show that the solution to the penalized problem is a solution to the original problem. 2. Notation and variational tools tools To introduce the variational structure of the problem, we define the Hilbert space H1 A,ε(RN ,C) obtained by the closure of C∞ 0 (RN ,C) under the scalar product (u, v)A,ε = Re ∫ RN ( ∇A,εu · ∇A,εv + V (x)uv ) dx for all u, v ∈ H1 A,ε(RN ,C) where ∇A,εu = (Dε 1u, . . . ,D ε Nu), D ε j = ε i ∂j − Aj(x), and Re and the bar denote the real part of a complex number and the complex conjugation respectively. The norm induced by this inner product is ∥u∥A,ε = (∫ RN (|∇A,εu|2 + V (x)|u|2) dx )1/2 for u ∈ H1 A,ε(RN ,C). Since there is no relationship between H1 A,ε(RN ,C) and H1(RN ,R); that is, H1 A,ε(RN ,C) ̸⊂ H1(RN ,R) and H1(RN ,C) ̸⊂ H1 A,ε(RN ,C), we will frequently use in this paper the following diamagnetic inequality (see [25, Theorem 7.21]) ε|∇|u|(x)| ≤ |∇A,εu(x)| for almost every x ∈ RN . (2.1) diam 4 W. F. ALMEIDA, G. M. FIGUEIREDO EJDE-2025/110 This implies that, if u ∈ H1 A,ε(RN ,C) then |u| ∈ H1(RN ,R). Therefore, u ∈ Lp(RN ,C) for any p ∈ [2, 2∗]. We denote by H1 A,ε,rad(RN ,C) the subspace of H1 A,ε(RN ,C) formed by the radial functions, that is H1 A,ε,rad(RN ,C) = {u ∈ H1 A,ε(RN ,C) : u(x) = u(|x|) for x ∈ RN}. 3. Auxiliary problems Auxiliary Note that, since the functional has arbitrary growth, it is not possible to obtain a functional directly associated to this problem. To overcome this difficulty, we will use the Del Pino and Felmer prenalization method [17] and make strong use of the radiality of the problem to obtain a functional that satisfies the Mountain Pass Geometry and that has compactness. We choose k > θ/(θ−2), where θ is given by (A4), and using (A5), take a > 0 to be the unique number such that f(a) = V0/k, with V0 given by (A2). We set f̂(s) := { f(s), if s ≤ a, V0/k, if s > a. Let χΛ denotes the characteristic function of the set Λ. We introduce the penalized nonlinearity g : RN × R → R by setting g(x, s) := χΛ(x)f(s) + (1− χΛ(x))f̂(s). (3.1) def_g Now, we shall consider the modified problem ( ε i ∇−A(x))2u+ V (x)u = g(x, |u|2)u, x ∈ RN , u ∈ H1 A,ε(RN ,C). (3.2) tDea Notice that if uε is a solution of the above problem such that |uε(x)| < a1/2 in Λc ,then, in view of the definition of g, there holds g(x, |u|2)u = f(|u|2)u for each x ∈ RN . Thus, the function u is also a solution of the original problem (1.1). In view of the above comment, in the sequel we study the modified problem (3.2). In the next result we prove that some properties on the continuous function g(x, s). lem3.1 Lemma 3.1. The continuous function g(x, s) satisfies the following properties uniformly in x ∈ RN : (1) g(x, s) = 0 for each s ≤ 0; (2) lims→0+ g(x, s) = 0, g and G(s) = ∫ s 0 g(t)dt are radials in x; (3) (i) 0 ≤ θ 2G(x, s) < g(x, s)s, for each x ∈ Λ, s > 0, (ii) 0 ≤ G(x, s) ≤ V (x) k s and 0 ≤ g(x, s) ≤ V (x) k , for each x ∈ Λc, s > 0; (4) the function s 7→ g(x, s) is non-decreasing for s > 0; (5) for all u ∈ H1 A,ε,rad(RN ,C), we have ∫ RN G(x, |u|2)dx <∞ and ∫ RN g(x, |u|2)|u|2dx <∞. Proof. Note that from (1)–(4) follow by the definition of g. Now, for u ∈ H1 A,ε,rad(RN ,C), from [27], there exists CN > 0, which depends just the dimension N such that |u(x)| ≤ CN∥u∥A,ε |x|(N−1)/2 . (3.3) Decaimento Then ∫ RN G(x, |u|2)dx ≤ ∫ Λ G ( x, C2 N∥u∥2A,ε R1 ) dx+ ∫ Λc G(x, |u|2)dx ≤ max Λ G ( ·, C2 N∥u∥2A,ε R1 ) |Λ|+ V0 k ∫ Λc |u|2dx <∞. (3.4) calhou Using the same argument we can conclude that ∫ RN g(x, |u|2)|u|2dx <∞. □ EJDE-2025/110 MAGNETIC SCHRÖDINGER EQUATIONS 5 By Lemma 3.1(5), the functional associated with (3.2), namely Jε(u) := 1 2 ∫ RN |∇A,εu|2dx+ 1 2 ∫ RN V (x)|u|2dx− 1 2 ∫ RN G(x, |u|2)dx, u ∈ H1 A,ε,rad(RN ,C) belongs to C1(H1 A,ε,rad(RN ,C),R) with Gâteaux differential given by J ′ ε(u)v := Re (∫ RN ∇A,εu∇A,εvdx+ ∫ RN V (x)uvdx− ∫ RN g(x, |u|2)uvdx ) , u, v ∈ H1 A,ε,rad(RN ,C). Moreover, its critical points are the weak solutions of the modified problem (3.2). Now we prove that the associated functional Jε satisfies the Mountain Pass Geometry. mountpassIA Lemma 3.2. Suppose (1)–(5) of Lemma 3.1 hold. Then, the functional Jε has a Mountain Pass Geometry, that is (i) Jε(0) = 0; (ii) there exist ρ, δ > 0 such that Jε(u) ≥ δ for all u ∈ H1 A,ε,(RN ,C) with ∥u∥A,ε = ρ; (iii) there exists u0 ∈ H1 A,ε,rad(RN ,C) such that ∥u∥A,ε > ρ0 and Jε(u0) ≤ 0. Proof. Note that by (2) of Lemma 3.1, given Υ > 0, there exists δ > 0 such that for all 0 ≤ s < δ. Then we have G(s) = F (s) ≤ Υ 2 |s|2. Considering (3.3) and ∥u∥A,ε = ρ with ρ enough small such that |u(x)| ≤ CN∥u∥A,ε R 1/2 1 ≤ δ, there exists C > 0 such that Jε(u) = 1 2 ∫ RN |∇A,εu|2dx+ 1 2 ∫ RN V (x)|u|2dx− 1 2 ∫ Λ G(x, |u|2)dx− 1 2 ∫ Λc G(x, |u|2)dx ≥ 1 2 ∥u∥2A,ε − Υ 4 ∫ RN |u|2dx− 1 2k ∫ RN V (x)|u|2dx ≥ C∥u∥2A,ε, and the proof of (ii) is complete, decreasing ρ if necessary. (iii) Note that, for all x ∈ Λ , from (G3), there exist C > 0 and s0 > 0 such that G(x, s) ≤ Csθ for all s ≥ s0. Now consider v0 ∈ C∞ 0 (Λ) and note that Jε(sv0) ≤ s2 2 ∥v0∥2A,ε − sθ 2 ∫ Λ |v0|θ dx. Since θ > 2, we obtain Jε(sv0) → −∞ as s → +∞ thus, taken u0 = sv0 for s sufficiently large (iii) is proved. □ By [29, Theorem 1.15] we assert the existence of a Palais-Smale sequence (un) inH 1 A,ε,rad(RN ,C) at level dε, that is, a sequence with the property Jε(un) → dε and J ′ ε(un) → 0, where dε is the minimax level of the mountain pass theorem related to Jε, namely dε = inf ς∈J max t∈[0,1] Jε(ς(t)), (3.5) beta0 where J = { ς ∈ C([0, 1], H1 A,ε,rad(RN ,C) : ς(0) = 0 and Jε(ς(1)) < 0 } . By a reasoning similar to the one in [29, Theorem 4.2], we have dε = inf u∈H1 A,ε,rad(RN ,C),u̸=0 sup t≥0 Φε(tu). (3.6) beta-e The main feature of the modified functional is that it satisfies the Palais-Smale condition, as we can see from the next result. vit5 Lemma 3.3. The functional Jε satisfies the (PS)dε condition for any level dε ∈ R. 6 W. F. ALMEIDA, G. M. FIGUEIREDO EJDE-2025/110 Proof. Suppose that (un) ⊂ H1 A,ε,rad(RN ,C) is a (PS)dε sequence for Jε, that is, Jε(un) → dε and J ′ ε(un) → 0. We first prove that (un) is bounded in H1 A,ε(RN ,C). Indeed, by using (3) of lemma 3.1 we obtain dε + on(1)∥un∥A,ε ≥ Jε(un)− 1 θ J ′ ε(un)un ≥ (1 2 − 1 θ ) ∥un∥2A,ε + 1 θ ∫ Λc ε g(x, |un|2)|un|2dx− 1 2 ∫ Λc ε G(x, |un|2)dx ≥ 1 2 (θ − 2 θ − 1 k ) ∥un∥2A,ε, where on(1) denotes a quantity approaching zero as n → ∞. Since k > θ/(θ − 2) we conclude from the above inequality that (un) is bounded in H1 A,ε(RN ,C). Claim. For any given ζ > 0, there exists R = R(ζ) > 0 such that R > 4R2 and lim sup n→∞ ∫ BR(0)c (|∇A,εun|2 + V (x)|un|2)dx ≤ ζ. (3.7) Crucial To prove the claim we consider ηR ∈ C∞(RN ,R) such that 0 ≤ ηR ≤ 1, ηR ≡ 0 in BR/2(0), ηR ≡ 1 in BR(0) c and |∇ηR| ≤ C/R, where C > 0 is a constant independent of R. Since the sequence (ηRun) is bounded in H1 A,ε(RN ,C), we have that J ′ ε(un)(ηRun) = on(1), that is, Re (∫ RN ∇A,εun∇A,ε(unηR)dx ) + ∫ RN V (x)|un|2ηRdx = ∫ RN g(x, |un|2)|un|2ηRdx+ on(1). Since ηR take values in R, a direct calculation shows that ∇A,ε(unηR) = iun∇ηR + ηR∇A,εun. The two above equalities and Lemma 3.1(3)(ii) imply that∫ RN ( |∇A,εun|2 + V (x)|un|2 ) ηRdx ≤ 1 k ∫ RN V (x)|un|2ηRdx+Re (∫ RN −iun∇A,εun∇ηR ) dx+ on(1). By using the definition of ηR, Hölder’s inequality and the boundedness of (un) we obtain( 1− 1 k )∫ BR(0)c ( |∇A,εun|2 + V (x)|un|2 ) dx ≤ C R ∥un∥L2∥∇A,εun∥L2 + on(1) ≤ C1 R + on(1). So, for any fixed ζ > 0, we can choose R > 0 large enough, such that lim sup n→∞ ∫ BR(0)c (|∇A,εun|2 + V (x)|un|2) ≤ ζ. This completes the proof of the claim. Now note that∫ RN ( g ( x, |un|2 ) |un|2 − g(x, |u|2)|u|2 ) dx = ∫ BR1 ( g ( x, |un|2 ) |un|2 − g(x, |u|2)|u|2 ) dx + ∫ BR\BR1 ( g ( x, |un|2 ) |un|2 − g(x, |u|2)|u|2 ) dx + ∫ Bc R ( g ( x, |un|2 ) |un|2 − g(x, |u|2)|u|2 ) dx. We shall prove that each of these terms approaches zero as n → ∞. From the boundedness of BR1 ⊂ Λc, we have un → u in L2 (BR1 ). By Lemma 3.1(3) it follows that∫ BR1 ( g ( x, |un|2 ) |un|2 − g(x, |u|2)|u|2 ) dx = on(1). EJDE-2025/110 MAGNETIC SCHRÖDINGER EQUATIONS 7 Using the proof of lemma 3.1(5) and Lebesgue’s Dominated Convergence Theorem, we conclude that ∫ BR\BR1 ( g ( x, |un|2 ) |un|2 − g(x, |u|2)|u|2 ) dx = on(1). Now note that ∣∣ ∫ Bc R g ( x, |un|2 ) |un|2 − g(x, |u|2)|u|2dx ∣∣ ≤ ∫ Bc R g ( x, |un|2 ) |un|2dx+ ∫ Bc R g(x, |u|2)|u|2dx ≤ ∫ Bc R (|∇A,εun|2 + V (x)|un|2) + ∫ Bc R g ( x, |un|2 ) |un|2dx. Since ∫ Bc R g ( x, |un|2 ) |un|2dx is integrable and using (3.7), we obtain∫ Bc R ( g ( x, |un|2 ) |un|2 − g(x, |u|2)|u|2 ) dx = on(1). Observe that J ′ ε(un)u = on(1), which implies that ∥u∥2A,ε = ∫ RN g(x, |u|2)|u|2dx. Then lim n→∞ ∥un∥2A,ε = lim n→∞ ∫ RN g(x, |un|2)|un|2dx = ∫ RN g(x, |u|2)|u|2dx = ∥u∥2A,ε. □ 4. Proof of Theorem 1.1 From Lemmas 3.2 and 3.3, for each ε > 0, there exists uε ∈ H1 A,ε,rad(RN ,C) weak solution of problem (3.2). That is, Jε (uε) = dε and J ′ ε (uϵ) v = 0,∀v ∈ H1 A,ε,rad(RN ,C). Note that, by the Principle of Symmetric Criticality [29, Theorem 1.28], we have that uε is in fact a critical point of Jε in the space H1 A,ε(RN ,C). The next result is crucial for this section. vit55 Lemma 4.1. ∥uε∥2A,ε → 0 as ε→ 0. Proof. Taking ψ ∈ C∞ 0, rad (Ω,R), a nonnegative function with suppψ ⊂ Ω, there is a unique tϵ ∈ R+ such that Jϵ (tϵψ) = max t≥0 Jϵ(tψ). Then, from (A2), ϵ2 ∫ Ω |∇ψ|2dx = ∫ Ω f ( |tϵψ|2 ) |ψ|2dx, and choosing Ω1 ⊂ Ω such that ψ(x) ≥ ψ0 > 0 for all x ∈ Ω1, it follows that ϵ2 ∫ Ω |∇ψ|2dx ≥ ∫ Ω1 f ( |tϵψ|2 ) |ψ|2 ≥ ψ2 0 ∫ Ω1 f ( |tϵψ|2 ) dx. Thus, from (A5), we conclude that tε → 0 as ε→ 0. Furthermore, 0 < dε ≤ Jϵ (tεψ) ≤ t2ε 2 ∫ Ω ϵ2|∇ψ|2dx, which implies that dε → 0 as ε→ 0. On the other hand, there exists C > 0 such that dε = Jϵ (uϵ) = Jϵ (uϵ)− 1 θ J ′ ϵ (uϵ)uϵ ≥ (1 2 − 1 θ )( ∫ RN ( |∇A,εuε|2 + ( 1− 1 k ) V (x)|uϵ|2 ) dx ) ≥ C∥uε∥2A,ε. 8 W. F. ALMEIDA, G. M. FIGUEIREDO EJDE-2025/110 The proof is complete. □ Now we prove a regularity result. Its proof follows the argument found in [5, Lemma 4.1.]. We will give the proof here for completeness of this work. leminha1 Lemma 4.2. Let (εn) be a sequence of positive numbers with εn → 0+ and un ∈ H1 A,εn,rad (RN ,C) be a solution of (3.2). Then |un| ∈ L∞(RN ) ∩ C1,λ loc (RN ), for λ ∈ (0, 1). Moreover, there exists a constant C > 0, independent on n, such that |un| ≤ C∥un∥A,εn . Proof. We define uL,n ∈ H1 A,εn,rad (RN ,C) and zL,n ∈ H1 A,εn,rad (RN ,C) by setting uL,n(x) := min{|un(x)|, L}, zL,n := u 2(β−1) L,n un, with β > 1 to be determined later. By using the calculation performed in [14, equation (2.2)] and the diamagnetic inequality we obtain Re ( ∇A,εnun∇A,εnzL,n ) ≥ u 2(β−1) L,n |∇A,εnun|2 ≥ u 2(β−1) L,n ε2n ∣∣∇|un| ∣∣2. This inequality, the definition of zL,n and J ′ εn(un)zL,n = 0 imply that∫ RN u 2(β−1) L,n |∇|un||2dx ≤ ∫ RN ( g(x, |un|2)− V (x) ) |un|2u2(β−1) L,n dx. (4.1) moser1 Arguing as in (3.4), using Lemma 4.1 and Lemma 3.1(1), we obtain C1 > 0 such that g(x, s) ≤ V0 2 + C1|s|(2 ∗−2)/2, for all (x, s) ∈ RN × R. This, (4.1), and V (x) ≥ V0 provide∫ RN u 2(β−1) L,n ε2n ∣∣∇|un| ∣∣2dx ≤ ∫ RN (V0 2 + C1|un|2 ∗−2 − V (x) ) |un|2u2(β−1) L,n dx ≤ C1 ∫ RN |un|2 ∗ u 2(β−1) L,n dx. (4.2) 2moser Let S be the best constant of the embedding D1,2(RN ,R) ↪→ L2∗(RN ,R) and define ûL,n := |un|uβ−1 L,n . We have that S−1∥ûL,n∥2L2∗ ≤ ∫ RN ∣∣∇( |un|uβ−1 L,n )∣∣2dx. But ∫ RN ∣∣∇( |un|uβ−1 L,n )∣∣2dx = ∫ {|un|≤L} ∣∣∇( |un|uβ−1 L,n )∣∣2dx+ ∫ {|un|>L} ∣∣∇( |un|uβ−1 L,n )∣∣2dx = ∫ {|un|≤L} ∣∣∇|un|β ∣∣2 dx+ ∫ {|un|>L} L2(β−1) |∇|un||2 dx ≤ β2 ∫ RN u 2(β−1) L,n ε2n ∣∣∇|un| ∣∣2dx, and therefore ∥ûL,n∥2L2∗ ≤ C3β 2 ∫ RN u 2(β−1) L,n ε2n ∣∣∇|un| ∣∣2dx. This and (4.2) yield ∥ûL,n∥2L2∗ ≤ C4β 2 ∫ RN |un|2 ∗ u 2(β−1) L,n dx, (4.3) 4moser for all β > 1. The above expression and uL,n ≤ |un|, imply that ∥ûL,n∥2L2∗ ≤ C4β 2 ∫ RN |un|2 ∗−2|un|2βdx. (4.4) 5moser Now, setting t := 2∗2∗ 2(2∗ − 2) > 1, α := 2t t− 1 < 2∗, (4.5) def_t EJDE-2025/110 MAGNETIC SCHRÖDINGER EQUATIONS 9 we can apply Hölder’s inequality with exponents t/(t− 1) and t in (4.4), to obtain ∥ûL,n∥2L2∗ ≤ C4β 2∥un∥2βLβα (∫ RN |un|2 ∗(2∗/2)dx )1/t . (4.6) 6moser Claim. There exist n0 ∈ N and K > 0 such that, for any n ≥ n0, it holds∫ RN |un|2 ∗(2∗/2)dx ≤ K. Assuming the claim is true, we can use (4.6) to conclude that ∥ûL,n∥2L2∗ ≤ C6β 2∥un∥2βLβα . Since ∥uL,n∥2βLβ2∗ = (∫ RN uβ2 ∗ L,ndx )2/2∗ ≤ (∫ RN |un|2 ∗ u 2∗(β−1) L,n dx )2/2∗ = ∥ûL,n∥2L2∗ ≤ C6β 2∥un∥2βLβα , we can apply Fatou’s lemma in the variable L to obtain ∥|un|∥Lβ2∗ ≤ C 1/β 7 β1/β∥|un|∥Lβα . We now set β := 2∗/α > 1 and note that, since |un| ∈ L2∗(RN ), the above inequality holds for this choice of β. Moreover, since β2α = β2∗, it follows that the inequality also holds with β replaced by β2. Hence, ∥|un|∥Lβ22∗ ≤ C 1/β2 7 β2/β2 ∥|un|∥Lβ2α . By iterating this process and recalling that βα = 2∗ we obtain, for k ∈ N, ∥|un|∥Lβk2∗ ≤ C ∑k i=1 β−i 7 β ∑m i=1 iβ−i ∥|un|∥L2∗ . Since β > 1 we can take the limit as k → ∞ to obtain ∥|un|∥L∞ ≤ C8∥|un|∥L2∗ . From the Sobolev imbedding, there exists a constant positive C, independent on n such that ∥|un|∥L∞ ≤ C∥|un|∥A,εn . (4.7) Wendy By the elliptic regularity |un| ∈ L∞(RN ) ∩ C1,λ loc (RN ), for λ ∈ (0, 1). It remains to prove the claim. In fact, let β = 2∗/2. From (4.3), we have |ûL,n|22∗ ≤ Cβ2 ∫ RN u2 ∗ n u (2∗−2) L,n dx, or equivalently |ûL,n|22∗ ≤ Cβ2 ∫ RN u2nu (2∗−2) L,n u(2 ∗−2) n dx. Using the Hölder inequality with exponents 2∗ 2 and 2∗ 2∗−2 |ûL,n|22∗ ≤ Cβ2 (∫ RN [ unu (2∗−2) 2 L,n ]2∗ dx )2/2∗(∫ RN u2 ∗ n dx ) 2∗−2 2∗ . From definition of ûL,n, we have(∫ RN [ unu (2∗−2) 2 L,n ]2∗ dx )2/2∗ ≤ Cβ2 (∫ RN [ unu (2∗−2) 2 L,n ]2∗ dx )2/2∗(∫ RN u2 ∗ n dx ) 2∗−2 2∗ . From Lemma 4.1, we conclude that(∫ RN [ unu (2∗−2) 2 L,n ]2∗ dx )2/2∗ ≤ Cβp ∫ RN u2nu (2∗−2) L,n dx, or equivalently (∫ RN [ unu (2∗−2) 2 L,n ]2∗ dx )2/2∗ ≤ Cβp ∫ RN u2 ∗ n dx ≤ K <∞. 10 W. F. ALMEIDA, G. M. FIGUEIREDO EJDE-2025/110 Using the Fatou’s lemma in the variable L, we have∫ RN u2 ∗(2∗/2) n dx ≤ K <∞, and therefore the claim holds. □ 4.1. Proof of Theorem 1.1. From (4.7) in Lemma 4.2, we have |uε| ≤ C∥uε∥A,ϵ. From Lemma 4.1, for ε > 0 sufficiently small, we have that |uε| < a1/2 and this completes the proof. Acknowledgments. W. F. 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Almeida Universidade de Braśılia, Departamento de Matemática, Campus Darcy Ribeiro, 01, CEP 70910-900, Braśılia, DF, Brazil Email address: wendy fda@hotmail.com Giovany M. Figueiredo Universidade de Braśılia, Departamento de Matemática, Campus Darcy Ribeiro, 01, CEP 70910-900, Braśılia, DF, Brazil Email address: giovany@unb.br 1. Introduction 2. Notation and variational tools 3. Auxiliary problems 4. Proof of Theorem 1.1 4.1. Proof of Theorem 1.1 Acknowledgments References