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BY 4.0 license Open Access Published by De Gruyter September 4, 2021

Compact Sobolev-Slobodeckij embeddings and positive solutions to fractional Laplacian equations

  • Qi Han EMAIL logo

Abstract

In this work, we study the existence of a positive solution to an elliptic equation involving the fractional Laplacian (−Δ)s in ℝn, for n ≥ 2, such as

(0.1) (Δ)su+E(x)u+V(x)uq1=K(x)f(u)+u2s1.

Here, s ∈ (0, 1), q2,2s with 2s:=2nn2s being the fractional critical Sobolev exponent, E(x), K(x), V(x) > 0 : ℝn → ℝ are measurable functions which satisfy joint “vanishing at infinity” conditions in a measure-theoretic sense, and f (u) is a continuous function on ℝ of quasi-critical, super-q-linear growth with f (u) ≥ 0 if u ≥ 0. Besides, we study the existence of multiple positive solutions to an elliptic equation in ℝn such as

(0.2) (Δ)su+E(x)u+V(x)uq1=λK(x)ur1,

where 2 < r < q < ∞(both possibly (super-)critical), E(x), K(x), V(x) > 0 : ℝn → ℝ are measurable functions satisfying joint integrability conditions, and λ > 0 is a parameter. To study (0.1)-(0.2), we first describe a family of general fractional Sobolev-Slobodeckij spaces Ms;q,p(ℝn) as well as their associated compact embedding results.

1 Introduction

In this paper, we are interested in seeking a positive solution to

(1.1) (Δ)su+E(x)u+V(x)uq1=K(x)f(u)+u21

in ℝn when n ≥ 2. Here, and henceforth, (−Δ)s denotes the fractional Laplace operator that, up to a normalization constant and for 0 < s < 1, is defined to be

(1.2) (Δ)su(x):=12Rnu(x+y)+u(xy)2u(x)|y|n+2sdy,

2q<2s with 2s:=2nn2s the fractional critical Sobolev index, while E(x), K(x), V(x) > 0 : ℝn → ℝ and f (u) : ℝ → ℝ are functions satisfying the conditions below.

(EKV1) K(x)LRn,infBRV(x)VBR>0 for each R > 0, while for all c > 0 and some ϑq,2s,L({x Rn:K(x)E2s92s2τ2sq2s2(x)Vτ(x)c<withτ0,2sϑ2sq.

(f1) f (u) is continuous and satisfies limu0+f(u)uq1=limuf(u)u2s1=0.

(f2) f (u) ≥ Aϑuϑ−1 ≥ 0 when u ≥ 0, Aϑ>max2,2θ2sϑn(92)RnKv09dxSn2s292 > 0 is a constant, v0 > 0 is a mountain pass solution to

(1.3) (Δ)su+E(x)u+V(x)uq1=K(x)uϑ1,

and 𝒮 represents the best fractional critical Sobolev embedding constant.

(f3) There is some θq,2s such that, for F(u):=0uf(v)dv with u, v ≥ 0,

(1.4) K(x)(uf(u)θF(u))η1K1(x)ur1η2K2(x)ur2,

where r11,2s and r2 [1, 2), K1(x), K2(x) > 0 : ℝn → ℝ are functions satisfying K12s2sr1(x) L1(ℝn) and K22s+κ2sq2sr2(x)Vκ(x)L1Rn with κ0,r2qr2, while 0η122sr1sθ3n2sr1Sn2s2sr12s2sθr12s6r1CK1 and 0η2min4r2sθ3n2r2Sn2s2r22(θ2)r226r2CK2,qr2sθ9nqr2Sn2sqr2q(θq)r2qr2CK2 are some constants with CK1:= RnK12s2sr1(x)dx2sr12s>0 and C K2 > 0 a constant that depends on some embedding constants (see Section 5 for details).

Note the hypothesis Aϑ > 2 in condition (f2) guarantees that

(1.5) 0supt0t22+tqqAϑtθϑ=sup0t1t22+tqqA9tθϑsupt0t2Aϑtϑϑ.

It may be helpful to demonstrate f (u) using an example. For ε > 0 small, set

f(u):={c1(q+ε)uq+ε1+c22su2s1ln(1+u)+2su2sln(1+u)u2s(1+u)ln2(1+u)0ifu00otherwise

for appropriate constants c1, c2 > 0 to observe F(u)={c1uq+ε+c2u2sln(1+u)ifu00otherwise. So, one derives

uf(u)θF(u)=c1(θqε)uq+ε+c22sθu2ln(1+u)c2u2s+1(1+u)ln2(1+u)

for u ≥ 0. When u is small, one has ln(1 + u) u and thus

uf(u)θF(u)c1(θqε)uq+ε+c22sθ1u2s1η2ur2

for some small η2 > 0 if 2s1q+ε , since q ≥ 2 > r2 ≥ 1; when u is large, one has

uf(u)θF(u)c1(θqε)uq+ε+c22sθ1u2sεη1ur1

for some small η1 > 0 if 2sq max{1, 2ε}, provided that q+ε< r1<2S in the case where 2sθ10 and 2sε< r1<2s in the case where 2sθ1<0. As a consequence, our condition (1.4) is fulfilled upon the introduction of K1(x), K2(x) ≥ K(x) > 0.

Since the seminal work by Brézis and Nirenberg [17], there has been a lot of research on the existence of positive solutions to elliptic problems involving the critical Sobolev exponent; see also the renowned papers of Ambrosetti, García-Azorero and Peral [5], and Benci and Cerami [12]. Problem (1.1) is motivated by the recent paper of do Ó, Miyagaki and Squassina [26], but our approach applies the insightful idea from García-Azorero and Peral [27] using the profound concentration-compactness principle of Lions [35]; see Palatucci and Pisante [39], and Bonder, Saintier and Silva [14] in the nonlocal setting. The authors in [26] used the ingenious approach of Caffarelli and Silvestre [18] which transfers a fractional Laplacian problem on ℝn to a locally possibly degenerate Laplacian problem on ℝn × ℝ+ via the s-harmonic extension; the relations of K (x), V(x) in [26] depend essentially on those of Alves and Souto [2], but ours are different. Finally, our condition (1.4) utilizes the embedding results and we have

uf(u)θF(u)η1K1(x)K1(x)ur1η2K2(x)K1(x)ur2;

noting that the right-hand side term is nonpositive, (1.4) is indeed weaker than the well-known condition of Ambrosetti-Rabinowitz that demands uf (u) ≥ θF(u) > 0.

Now, our first main result can be formulated as follows.

Theorem 1.1

Suppose n ≥ 2, 0 < s < 1, 2 ≤ q<2s,E(x), K(x), V(x) > 0 : ℝn → ℝ satisfy condition (EKV1), and f (u) : ℝ → ℝ satisfies conditions (f1)-(f3). Then, equation (1.1) has a positive solution.

Below, we proceed to discuss the existence of multiple positive solutions to

(1.6) (Δ)su+E(x)u+V(x)uq1=λK(x)ur1,

where 2 < r < q < ∞ both possibly being (super-)critical, E(x), K(x), V(x) > 0 : ℝn → ℝ are functions satisfying the subsequent conditions, and λ > 0 is a parameter.

(EKV2-1) 2< r<min{2s,q},K(x)Lloc,infBRV(x)VBR>0 for each R > 0, while for some β ∈ [0,∞) and κβ(r2)qr+r2qrn2s,β(r2)qr+rqr,Kψ2s(β,κ)(x)Eβ(x)Vκ(x)L1Rn with ψ2s(β,κ):=2s+β2s2+κ2sq2sr. (EKV2-2) 2sr< q,K(x)LlocRn,infBRV(x)VBR>0 for each R > 0, while for some β ∈ [0,∞) and κβ(r2)qr+rqr,β(r2)qr+r2qrn2s,Kψ2s(β,κ)(x)Eβ(x)Vk(x)L1Rn.

(EK) 2< r<min2s,q,infBRE(x)EBR>0 for each R > 0, K(x) ∈ L(Ω) for every subset ΩRn with 𝔏(Ω) < ∞, and LxRn:K(x)E2sr2s2(x)c< for all c > 0.

Since the celebrated paper of Ambrosetti, Brézis and Cerami [3] on the concave and convex model problem, there has been a lot of studies on this topic. In 1996, Alama and Tarantello [1] considered an elliptic problem of different type that is the origin of all the research on equation (1.6). It seems to the author that Chabrowski [20] was the first person extending a result in [1] to ℝn; ever since, other important results appeared such as the renowned papers of Pucci and Rădulescu [42, 44] where for the first time the multiplicity results were discussed; Autuori and Pucci [8] later extended this research to the nonlocal setting with the same equation as (1.6) here (see also the closely related paper [7]). In this sense, our study continues their work, as we further utilize the compact embedding results for the functions E (x), K (x), V(x), not merely those for K(x) and/or V(x). See [31] for more details and references.

Of course, the authors in [7, 8] used Hardy’s potential for E(x); here, we shall fully employ E (x) by inscribing it into the compact embedding results with K(x), V(x), which include the one where β=0,κ=rqr and ψ2s0,rqr=qqr in [7, 8] as a special case. Other two closely related important work are from Pucci and Zhang [43], and Rădulescu, Xiang and Zhang [45], where a weaker condition corresponding to β = 0, κ=r2qrn2sandψ2s0,r2qrn2s=q2qrn2s was used. Notice both conditions come from those in [1]. In addition, our condition (EK) here is broader than any of those appeared in the associated earlier work.

Now, our second main result can be formulated as follows.

Theorem 1.2

Assume that n ≥ 2, 0 < s < 1, 2 < r < q < ∞ both possibly being (super-)critical, and E(x), K(x), V(x) > 0 : ℝn → ℝ satisfy conditions (EKV2-1) or (EKV2-2). Then, there is a λ1 ≥ 0 such that equation (1.6) has at least a positive solution for all λ > λ1. In addition to condition (EKV2-1), when condition (EK) is true, then λ1 > 0 and equation (1.6) has at least a positive solution if and only if λλ1; moreover, there exists a λ2(≥ λ1 > 0) such that equation (1.6) has at least two distinct positive solutions for all λ > λ2.

Note in problems (1.1) and (1.6), we are interested in the situation where E(x), K(x), V(x) vanish at infinity, as initiated by Ambrosetti, Felli and Malchiodi in their celebrated work [4].

The paper is organized as follows: Section 2 analyzes a family of general fractional Sobolev-Slobodeckij spaces Ms;q,p(ℝn), Section 3 describes a version of the fractional Moser-Trudinger inequality when sp = n, Section 4 discusses some compact embedding results that are particularly useful for our studies here of equations (1.1) and (1.2), while Sections 5 and 6 are devoted to the detailed proofs of Theorems 1.1 and 1.2 respectively.

An excellent reference for the approaches involved in this paper is the recent monograph of Papageorgiou, Rădulescu and Repovš [40] for nonlinear analysis in large.

It is worthwhile to remark finally that our conditions fully utilize the (compact) embedding results both in the upper-triangle case and the lower-triangle case (see Section 4 for definition) in each individual problem, which seems new even in the Laplacian setting.

2 Function space analysis

Recently, nonlocal equations and the associated fractional Sobolev function spaces Ws,p(ℝn) attracted great attentions due to their impressive applications to real-world problems in various disciplines as briefed, for example, in the introduction from Di Nezza, Palatucci and Valdinoci [23]; see also Demengel and Demengel [22, Chapter 4], or Molica Bisci, Rădulescu and Servadei [37, Chapters 1-2] for some concise, self-contained treatment of this matter.

In his classical monograph [36, Section 5.1.1], Maz’ya defined a class of general Sobolev function spaces Wp,q1Rn; using the symbol Mq,p(ℝn), the author analyzed some relations among those spaces and their compact embedding results in [28, 29, 30, 31] hoping to provide a complement to Lemma I.1 of Lions [34] in the function space setting.

In the desire of furnishing a bit more insight regarding the similarity between W1,p(ℝn) and Ws,p(ℝn) as seen in [22, 23, 37], Sections 2-4 here are devoted to the description of a family of general fractional Sobolev-Slobodeckij spaces Ms;q,p(ℝn) when n ≥ 2, their relations and their compact embedding results that are akin to those observed for Mq,p(ℝn).

In the sequel, we always assume n ≥ 2, 1 ≤ p, q ≤ ∞and 0 < s < 1.

Denote by Ω a bounded domain in ℝn having a compact, Lipschitz boundary Ω, or Ω = ℝn. Define Ms;q,p(Ω) to be the Banach space as the completion of the set C1(Ω)ifΩ is bounded, or as that of the set CC1RnforΩ=Rn, with respect to the norm

(2.1) uMs;q,p(Ω):=[u]S,p,Ω+uq,Ω,

where [u]s,p,Ωp:=ΩΩ|u(x)u(y)|p|xy|n+spdxdyanduq,Ωq:=Ω|u|qdx.

Note Ws,p(Ω)=Ms;p,p(Ω),andMs;q,(Ω)=C0,s(Ω) independent of q. From now on, we shall write both continuous embedding of function spaces and convergence of functions by “→”, compact embedding of function spaces by “↦”, and weak convergence of functions by “”. Other notations will be clarified when appropriate.

Below, we will embark on our detailed analysis for the spaces Ms;q,p(Ω).

2.1 Ω is a bounded domain having a compact, Lipschitz boundary ∂Ω

In this case, it is trivial to see Ms;q,p(Ω) → L1(Ω); so, via the fractional Poincaré’s inequality of Bellido and Mora-Corral [11, Lemma 3.1], we have Ms;q,p(Ω) → Ws,p(Ω) through Minkowski’s inequality. This, together with [22, Corollary 4.53], leads to the conclusions as follows.

(1) When sp < n, we have, with ps:=npnsp,

(2.2) Ms;q,p(Ω)=Ws,p(Ω) for 1qps,Ms;q1,p(Ω)Ms;q2,p(Ω) for psq2q1.

Also, there exists a constant Cp,q > 0, depending on n, p, q, s, Ω, such that

(2.3) uWs,p(Ω)Cp,quMs;q,p(Ω),uMs;q,p(Ω)andq[1,].

(2) When sp = n, we have

(2.4) Ms;,p(Ω)Ms;q,p(Ω)=Ws,p(Ω)for1q<,

and Ms;q,p(Ω) in general cannot be a proper subspace of L(Ω) unless q = ∞. The fractional Moser-Trudinger inequality of Parini and Ruf [41] says

(2.5) sup[u]s,p,Rn1Ωeα|u|nnsdxCΩ,uW˜0s,p(Ω) and α0,α,

Here, α*, C Ω > 0 are constants of n, p, s, Ω, and W˜0S,p(Ω), as a proper subspace of Ws,p(Ω), is the completion of CC1(Ω) with respect to the Gagliardo semi-norm [u]s,p,Rn which is equivalent to (2.1) on ℝn for CC1(Ω) by Brasco, Lindgren and Parini [16, Remark 2.5].

(3) When sp > n, we have, with γs:=spnp,

(2.6) Ms;q,p(Ω)=Ws,p(Ω)C0,γ(Ω) for 0γγs and 1q.

Next, by [22, Theorem 4.54] or [23, Theorem 7.1], one easily verifies the result below.

Proposition 2.1

Assume n ≥ 2,1 ≤ p, q ≤ ∞ and 0 < s < 1. When sp < n, the embedding Ms;q,p(Ω) → Lr(Ω) is continuous if 1rmaxps,q and compact if 1r<maxps,q . When spn, the embedding Ms;q,p(Ω) ➨ Lr(Ω) is compact if 1 ≤ r < ∞.

Proof. Viewing (2.2)-(2.4) and (2.6), we only need to consider the case sp < n following almost identically the proofs of [22, Theorem 4.54] or [23, Theorem 7.1]. Actually, noticing that Ω is an extension domain, for any cube Q ( Ω ) and each u ∈ Ms;q,p(Ω), denote the extension of u to Ws,p(ℝn) by u˜; then, for some constants CΩ,Cp,q>0 depending on n, p, q, s, Ω,

u˜Ws,p(Q)u˜Ws,pRnCΩuWs,p(Ω)Cp,quMs;q,p(Ω)

holds. So, our proof is finished using [22, Theorem 4.54] or [23, Theorem 7.1].

Finally, recall for sp > n, in view of (2.6), one actually has

Ms;q,p(Ω)C0,γ(Ω) for 0γ<γs and 1q.

On the other hand, from our preceding analysis and the remark at page 197 of [22], we have an equivalent definition of the space Ms;q,p(Ω), when p, q ≠ ∞, such as

Ms;q,p(Ω):=u:ΩR measurable with [u]s,p,Ω+uq,Ω<.

2.2 Ω =n

Recall Ms;q,p(ℝn) denotes the Banach space as the completion of the set Cc1Rn in terms of the norm (2.1). Now, following Lieb and Loss [33, Sections 3.2 and 4.3], a function uLloc1Rn is said to vanish at infinity provided 𝔏({x ∈n : |u(x)|c}) < ∞ for all positive constants c > 0, where 𝔏 represents the Lebesgue measure.

(1) When sp < n, denote by Ds,p(ℝn) the space of functions uLloc1Rn where u vanish at infinity and [u]s,p,Rn < ∞. Then, a careful check for [23, Lemma 6.3 and Theorem 6.5] implies that uLpsRn, and the fractional Sobolev inequality reads as follows

(2.7) Rn|u|psdxnspnC1RnRn|u(x)u(y)|p|Xy|n+spdxdy,uDs,pRn.

Here, C1 > 0 is an absolute constant depending on n, p, s for 1 ≤ p < ∞.

By virtue of Dipierro and Valdinoci [24] with a = 0, Ds,p(ℝn) can be equivalently defined to be the completion of Cc1Rn through [u]s,p,Rn; so, Ds,pRn=Ms;ps,pRn and one recognizes an equivalent definition of the space Ms;q,p(ℝn), for q ≠ ∞, such as

Ms;q,pRn:=u:RnR measurable with [u]s,p,Rn+uq,Rn<.

From Chebyshev’s inequality and the standard interpolation inequality, one has

(2.8) either 1q1q2psMs;q1,pRnMs;q2,pRnDs,pRnfor or psq2q1<.

If one would like to include q = ∞, then u needs to be compactly supported.

The best fractional critical Sobolev embedding constant 𝒮p is defined to be

(2.9) Sp:=infuDs,pRn{0}[u]s,p,Rnpups,RnpC11>0.

As common practice, we write Ds(ℝn) := Ds,2(ℝn) and 𝒮 := 𝒮2 in the sequel.

(2) When sp = n, the fractional Gagliardo-Nirenberg inequality of Nguyen and Squassina [38, Lemma 2.1] says

(2.10) ur,RnC2uq,Rnς[u]s,p,Rn1ς,uMs;q,pRn.

Here, we only write a tailored version for our purpose with 1 ≤ qr < ∞and ς:=qr (0, 1], and C2 > 0 is an absolute constant depending on n, p, q, r, s. Thus, we have

(2.11) Ms;q1,pRnMs;q2,pRn for 1q1q2<.

Notice here q = ∞does not contribute to this continuous embedding (2.11).

(3) When sp > n, a careful check for Theorem 8.2 in [23], especially their estimates (8.3) and (8.9), suggests that Ms;q,pRnC0,γsRnLRn. Therefore, one has

(2.12) Ms;q1,pRnMs;q2,pRnC0,γsRn for 1q1q2.

Note Ms;q,∞(ℝn)→ C0,s(ℝn) which is consistent with the observation at page 565 of [23], and Ms;∞,p(ℝn) is the largest possible function space for fixed p, s in (2.12).

Summarizing all the preceding analysis yields the result below.

Proposition 2.2

Assume n ≥ 2,1 ≤ p, q < ∞and0 < s < 1.When sp < n, the embedding Ms;q,p(ℝn)→ Lr(ℝn) is continuous if minps,qrmaxps,q. When sp = n or sp > n, the embedding Ms;q,p(ℝn)→ Lr(ℝn) is continuous if qr < ∞or qr ≤ ∞.

3 A fractional Moser-Trudinger inequality

In this section, we utilize [41] to provide an extension of the inequality (2.5) to ℝn for functions in M s;q,p(ℝn) when sp = n. The proof presented here follows essentially from do Ó [25, Lemma 1] and Ruf [46, Proposition 2.1]. Consult also Li and Ruf [32], Han [30, Section 2.2], and several other important contributions in ℝn that cannot be exhaustively listed here.

Below, we review some fundamental facts about Schwarz symmetrization based on Berestycki and Lions [13, Appendix III], and Lieb and Loss [33, Section 3.3]. Assume f (x) is a measurable function vanishing at infinity in the measure-theoretic sense of Lieb and Loss, and let f*(x) ≥ 0 be its Schwarz symmetrization or spherical rearrangement through LχRn:f(x)c=LxRn:|f(x)|c for all positive constants c > 0. Then, f* is unique, radial, decreasing in |x|, and lower semi-continuous (and therefore, measurable). Also, we have

(3.1) RnΦfdx=RnΦ(|f|)dx

for all continuous functions Φ with Φ(|f |) integrable; so, fq,Rn=fq,RniffLqRnfor1q. We recall the important Theorem 3 of Beckner [10] and observe

(3.2) RnRnf(x)f(y)p|Xy|n+spdxdyRnRn|f(x)f(y)|p|Xy|n+spdxdy,

while moreover the Berestycki-Lions’ radial lemma [13, Lemma A.IV] leads to

(3.3) f(x)|x|nqnωn11qfq,Rn,fLqRn,

with x ≠0, where ωn−1 represents the surface area of the unit sphere in ℝn.

It is notable that neither in [13, Appendix III] or [34, Lemma I.1], nor in [33, Section 3.3] or [10, Theorem 3] was the condition f being integrable needed.

Now, we characterize an inequality of fractional Moser-Trudinger type in the function space Ms;q,p(ℝn) using its full norm, instead of the Gagliardo semi-norm [u]s,p,Rn.

Theorem 3.1

Let n ≥ 2, 1 ≤ p, q < ∞, 0 < s < 1, sp = n, 0 ≤ α < α*, and u ∈ Ms;q,p(ℝn). Then, we have

(3.4) supuMs;q,p(Rn1RnΨα,q,s(|u|)dxC(α,q,s).

Here, C(α, q, s) > 0 is an absolute constant that depends on α, n, p, q, s, and for v ≥ 0 and the least positive integer l0 with l0nnsq1, we set Ψα,q,s(v):=l=l0αll!vlnns.

Proof. To save notation, without loss of generality, take u ≥ 0. Recalling (3.1) and (3.2), and noticing that Ψα,q,su0 for u*, we may simply consider u = u* and decompose

RnΨα,q,s(u)dx=BR0Ψα,q,s(u)dx+BR0cΨα,q,s(u)dx.

Here, and hereafter, BRRn is the ball of radius R centered at the origin and BRc:=RnBR, while R0 > 0 is a sufficiently large absolute constant to be determined later.

To estimate the integral over BR0, write v(x) := max{u(x) − u0, 0} for u0 := u(R0) > 0, a constant. Then, v0onBR0c and vW˜0s,pBR0. In fact, as in [16, Lemma 2.4], for the ball BR0x0BR0c of radius R0 centered at a point x0 with |x0| = 4R0, one has

vp(x)=|v(x)v(y)|p|Xy|2n|xy|2n for xBR0 and yBR0x0,

which further yields

ωn1R0nnvp(x)diamBR0x0BR02nBR0x0|v(x)v(y)|p|χy|2ndy.

Thus, it follows that

ω n 1 n 36 R 0 n B R 0 v p ( x ) d x B R 0 B R 0 x 0 | v ( x ) v ( y ) | p | x y | 2 n d y d x B R 0 B R 0 | v ( x ) v ( y ) | p | x y | 2 n d x d y + 2 B R 0 B R 0 c | v ( x ) v ( y ) | p | x y | 2 n d x d y = B R 0 B R 0 | u ( x ) u ( y ) | p | x y | 2 n d x d y + 2 B R 0 B R 0 c 0 u ( x ) u 0 p | X y | 2 n d x d y ;

in view of u(y)u0onBR0c, we have

ωn1n36R0nvp,BR0p[v]S,p,Rnp[u]S,p,Rnp1.

Recall [25, Estimate (5)] says (1+t)nnstnns+C3tsns+1 for all t (0,∞) with C3 > 0 an absolute constant. Actually, for

f(t):=(1+t)nnstnns1tsns

continuous on (0,∞), one observes limt0+f(t)=0 as n2>2s and limf(t)=nnsthrought˜:=1t. Hence, for t=v(x)u0, it follows that

unnsv+u0nnsvnns+C3vsnsu0+u0nns.

Apply Young’s inequality to C3vsnsu0 to get, for an absolute constant C3>0,

(3.5) unnsvnns1+u0ns+C3+u0nns.

Set u˜:=v1+u0nsnsnW˜0s,pBR0 and recall [v]S,p,Rnp[u]S,p,Rnp to see

[u˜]s,p,Rnp1+u0nsnss[u]s,p,Rnp1+u0nsnss1uq,Rnns.

From (3.3), one has u0nsσuq,Rnns for σ:=nωn1R0nnqs. Define

g(t):=1+σtnsnss(1t)ns1

with g(0) = 0 and g(1) = −1, and note

g(t)=nS1+σtnsn2ss(1t)nssnssσtnssnsσtns1.

Write

h(t):=nsSσtnssnSσtns1

with ht0=0att0:=nsn2. Thus, when R0 is so large that σnnS2nss, one deduces h(t) ≤ 0 and hence g(t) ≤ 0 on [0, 1]. That is, g(t) ≤ 0 for 0 ≤ t ≤ 1, which clearly implies that [u˜]s,p,Rn1 provided R0nnωn1nsnq(2ns)n.

Thus, one may combine the preceding analysis with (2.5) and (3.5) to derive

BR0Ψα,q,s(u)dxBR0eαunnsdxeαC3+αu0nnsBR0eαu˜nnsdxC1(α,q,s).

Here, C1(α, q, s) > 0 is an absolute constant depending on α, n, p, q, s.

To estimate the integral over BR0C, we use (3.3) with uMs;q,pRn1 to see

B R 0 c u ln n s d x ω n 1 n ω n 1 ln q ( n s ) R 0 t ln 2 q ( n s ) + n 1 d t R 0 n ω n 1 n ω n 1 R 0 n l n q ( n s ) q ( n s ) ln 2 n q ( n s ) = R 0 n ω n 1 σ 1 s n s q ( n s ) ln 2 n q ( n s ) .

As l0nnSq, we apply Proposition 2.2 to the first term of Ψα,q,s(u) and observe

BR0cΨα,q,s(u)dxαl0l0!BR0cul0nnsdx+q(ns)n2R0nωn1eασsnsC2(α,q,s).

Here, C2(α, q, s) > 0 is an absolute constant depending on α, n, p, q, s.

Therefore, (3.4) follows with C(α, q, s) := C1(α, q, s) + C2(α, q, s) > 0.

It is worth to remark that Parini and Ruf [41] found an upper bound

αs,n:=n2ωn12Γ(p+1)n!k=0(n+k1)!(n+2k)pk!sns

for α* utilizing renowned functions in analytic number theory with sophisticated calculations. Following Proposition 5.2 of [41], one observes a similar result as follows.

Proposition 3.2

Assume that n ≥ 2, 1 ≤ p, q < ∞, 0 < s < 1, sp = n, and αs,n<α<. Then, we have

(3.6) supuMs;q,pRn1RnΨα,q,s(|u|)dx=.

Proof. Define the nonlocal/modified Moser function uε by |lnε|1snif|x|ε,|ln|x|||lnε|snifε|x|1, and 0 if |x| ≥ 1. Then, limε0+uεS,p,Rnp=αs,nnnss as shown in Proposition 5.1 of [41] through delicate computations, and uεq,Rnq=O|lnε|sqn which is infinitesimal when ε0+. Set accordingly Vε:=uεuεMs;q,p(Rn0 with vεMs;q,pRn=1. When α>αs,n and ε is sufficiently small, αuεMs;q,pRnnnsαuεS,p,Rnnnsαnαs,n> n. So, one derives

RnΨα,q,s(vε)dxBεΨα,q,s(vε)dx=BεeαuεMs;q,p(Rn)nns|lnε|dxl=0l01αll!BεuεMs;q,p(Rn)lnns|lnε|ldxωn1n(εnαnαs,nO(εn|lnε)|l0)asε0+,

which certainly implies the desired estimate (3.6) and thus finishes the proof.

Not like in the local case, it is not clear if αS,n is optimal, yet, as pointed out in Remark 5.4 of [41], at least αs.2 coincides with the optimal exponent α1,2 up to the multiplicative constant appeared in the asymptotic behaviour of the Gagliardo semi-norm as s → 1.

4 Some compact embedding results

In this section, we describe some compact embedding results from subspaces of Ms;q,p(ℝn) or Ds,p(ℝn) to LKrRn that are useful when studying problems (1.1) and (1.6).

Some closely related results on1,p(ℝn)may be found in Bartsch and Wang [9, Theorem2.1], Chiappinelli [21, Theorem 1], Schneider [47, Theorem 2.3], Bonheure and Van Schaftingen [15, Theorem 4], and Han [30, Section 4.1] and [31, Propositions 2.3-2.4]; note nevertheless the results presented below seem not known in the literature, even on W1,pRn.

Let n2,1p,q<,1p˜ps, and 0 < s < 1 with sp < n. Suppose E(x), V(x) > 0 with infBRV(x) VBR>0 for each R > 0 in the sequel. Denote by ME,Vs;q,pRn the Banach space as the completion of functions uLloc1(Rn) that vanish at infinity (measure-theoretically) with [u]s,p,Rn<, or equivalently as that of uCc1Rn, with respect to the norm

(4.1) uME,vs;a,pRn:=[u]s,p,Rn+uLEp˜Rn+uLVqRn

for uLEp˜Rnp˜:=RnE|u|p˜dx and uLVqRnq:=RnV|u|qdx;so,ME,Vs;q,pRnDs,pRn.

Theorem 4.1

Assume that n ≥ 2,1 ≤ p < ∞,0 < s < 1with sp < n, and1p˜,qr< ps. Let E(x), K(x), V(x) > 0 : ℝn → ℝ be Lebesgue measurable functions such that K(x) ∈ Lt(Ω) for some tpspsr, on each set Ω ofn having L(Ω)< while K(x)Eϕps(τ)(x)Vτ(x) vanishes at infinity with ϕps(τ):=psrpsp˜τpsqpsp˜ for some τ0,psrpsq;so, ϕps(τ)0,psrpsp˜. Then, the embedding ME,Vs;q,pRnLKrRn is compact.

Proof. Without loss of generality, assume {ul : l ≥ 1} is a sequence of functions in ME.Vs;q,pRn with ul 0 when l → ∞and ulME.Vs;q,pRn uniformly bounded. For each ε > 0, setWε:=xRn:K(x)Eϕps(τ)(x)Vτ(x) ε} andWεC:=RnWε to decompose

RnKulrdx=WεKulrdx+WεcKulrdx.

For the integral overWec, noting that ps=rp˜ϕps(τ)qτ1ϕps(τ)τ, it is easy to get

(4.2) WεcK|ul|rdx=WεcKEϕps(τ)Vτ(E|ul)|p˜ϕps(τ)(V|ul)|qτ|ul|rp˜ϕps(τ)qτdxε(WεcE|ul|p˜dx)ϕps(τ)(WεcV|ul|qdx)τ(Wεc|ul|psdx)1ϕps(τ)τεC1ulLEp˜(Rn)p˜ϕps(τ)ulLVq(Rn)qτ[ul]s,p,Rnrp˜ϕps(τ)qτεC1ulME,Vs;q,p(Rn)r

using (2.7), with C1>0 an absolute constant independent of ul for all l ≥ 1.

For the integral over Wε, as LWε< and infBRV(x)VBR>0, one sees from (2.3) and Proposition 2.1 that ME,Vs;q,pBRWs,pBRLrtt1BR with rtt1r,ps, and thus

(4.3) WεK|ul|rdx=BRWεK|ul|rdx+BRcWεK|ul|rdx(WεKtdx)1t{(BR|ul|rtt1dx)t1t+(Rn|ul|psdx)rps(L)(BRcWε)11trps}0

as R → ∞and l → ∞for a subsequence {ul : l ≥ 1} using the same notation.

So, (4.2)-(4.3) yields u l L K r R n 0 as l → ∞and thus finishes the proof.

Note the embedding ME,Vs;q,pRnLKrRn is continuous for pspsrt, and if K(x)LRn, then the integrability requirement of K(x) is fulfilled automatically.

Theorem 4.2

Assume that n ≥ 2, 1 ≤ p < ∞, 0 < s < 1 with sp < n, and 1p˜r<minps,q. Let E(x), K(x), V(x) > 0 : ℝn → ℝ be such that K(x)Lloct(Rn) for some tmaxps,qmaxpc,qr, and Kψps(β,κ)(x)Eβ(x)Vκ(x)L1Rn with ψps(β,κ):=ps+βpsp˜+κpsqpsr for some β ∈ [0,∞) and κ0,β(rp˜)+rqr. Then, the embedding ME,Vs;q,pRnLKrRn is compact.

Proof. Define w:=β(psr)ps+β(psp˜)+κ(psq),x:=κ(psr)ps+β(psp˜)+κ(psq),y:=r+β(rp˜)+κ(rq)ps+β(psp˜)+κ(psq) and z:=psrps+β(psp˜)+κ(psq)=ψps1(β,κ) with w+x+y+z=1. Then, for all uME.Vs;q,pRn and on each set Ω of ℝn, one has

(4.4) ΩK|u|rdx=ΩKEwVx(E|u)|p˜w(V|u)|qx|u|rp˜wqxdx(ΩKψps(β,κ)EβVκdx)z(ΩE|u|p˜dx)w(ΩV|u|qdx)x(Ω|u|psdx)yC1Kψps(β,κ)EβVκ1,Ωψps1(β,κ)uLEp˜(Ω)p˜wuLVq(Ω)qx[u]s,p,Rnpsy

by Hölder’s inequality and (2.7), as p˜w+qx+psy=r, provided w,x,y,z(0,1).

Note that β ≥ 0 while β = ∞furnishes a version of Theorem 4.1. As w=βzandx=κX,togetz>0 , one has 0<κ<βpsp˜+psqps, while to get y>0, one has either 0<κ<β(rp˜)+rqr or κ>βpsp˜+psqpc; so, 0<κ<β(rp˜)+rqr, When β=0=w, one simply ignores E(x) or treats E(x) as 0 with 00=1, while when κ=0=x, the same instead occurs to V(x). We may set 𝔶 = 0 to get κ=β(rp˜)+rar without having ps involved, and can simultaneously take w=x=0 corresponding to ME,Vs;q,pRn=Ds,pRn with E(x)V(x)0. So, MEVs;q,pRnLKrRn, upon replacing Ω in (4.4) by ℝn, is continuous without using K(x)LloctRn.

Finally, utilizing the same {ul : l ≥ 1} as the one in Theorem 4.1, we derive

RnKulrdx=BRKulrdx+BRcKulrdx.

For the integral on BR, as ME,Vs;q,pBRMs;q,pBRLrt1BR with rtt1r,maxps,q,

(4.5) BRKulrdxBRKtdx1tBRulrtt1dxt1t0

when l → ∞ for a subsequence {ul : l ≥ 1} by the same index l, via infBRV(χ)VBR>0, (2.2) and Proposition 2.1; for the integral on BRc, we apply (4.4) on Ω=BRc to deduce, as R →∞,

BRcKulγdxC1Kψps(β,κ)EβVκ1,BRcψps1(β,κ)ulME,Vs;q,pRnr0.

Hence, ul → 0 in LKrRn for a subsequence relabeled using the same index l.

Theorem 4.3

Suppose n ≥ 2, 1 ≤ p < ∞, 0 < s < 1 with sp < n, and 1p˜psr< q.LetE(x),K(x),V(x)> 0 : ℝn → ℝ be such that K(x)Lloct(Rn) for some tqqr, and Kψps(β,κ)(x)Eβ(x)Vκ(x)L1Rn for some β ∈ [0,∞) and κβ(rp˜)+rqr,. Then, the embedding ME.Vs;q,pRnLKrRn is compact.

Proof. The proof is essentially the same as that of Theorem 4.2. Keep in mind q> rpsp˜ when ensuring w,x,n,z(0,1). Actually, to have z>0, one sees κ>βpsp˜+psaps, while to get 𝔶 > 0, one has either 0 < κ < βpsp˜+psap or κ>β(rp˜)+rar;so,κβ(rp˜)+rar after taking y=0. Recall ME.Vs;q,pRnLKrRn is continuous with no need of K(x)LloctRn.

Several remarks are in order: first, Theorem 4.2 merged [21, Theorem 1] (the upper-triangle case rp˜) and [47, Theorem 2.3] (the lower-triangle case r < q) in one result, while β = ∞or κ = 0 yield versions of Theorem 4.1 via integrability conditions; second, Theorem 4.2 is useful particularly for Theorem 1.2, but the case β = 0 contributes to condition (f3) of Theorem 1.1; finally, Theorem 4.1 is intended for Theorem 1.1, but the case τ = 0 is used in condition (EK) of Theorem 1.2. As such, it is probably helpful to summarize them as follows.

Proposition 4.4

Assume that n2,p=p˜=2 and 0 < s < 1.

(i). Suppose further 1 ≤ r<min2s,q, and K(x), V(x) > 0 satisfy K2s+K2q2sr(x)Vκ(x)L1Rn for some κ0,rqr; then, the embedding MVs;q,2(Rn)LKr(Rn) is continuous, where MVs;q,2(Rn) is the function space defined via (4.1) without the term Eu2.

(ii). Suppose further 2r<2s, infBRE(x)EBR>0 for each R > 0, K(x) ∈ Lt(Ω) for some t[pspsr,] on each set Ω ofn with L(Ω)<, and K(x)E2sr2s2(x) vanishes at infinity; then, the embedding HEs(Rn)LKr(Rn) is continuous, where HEs(Rn) is the Hilbert function space defined through (4.1) with the term Vuq dropped.

We can take p=p˜ and V(x) 0 to haveWEs,p(Rn)LKp(Rn) or WEs,p(Rn)LK1(Rn), or take E(x) ≡ V(x) 0 to have Ds,p(Rn)LKp(Rn), for suitable E(x) and K (x), which seems to provide a complement to [14, Condition (h1)] in terms of compact embedding.

Finally, following Servadei and Valdinoci [48, Section 3] or [49], or applying Auchmuty [6] (see also [37, Section 3.1]), one observes the eigenvalue problems

(4.6) (Δ)sf+Ef=ϱKfand(Δ)sg=ξKginRn,

when n ≥ 2, admit families k > 0 : k ≥ 1} and l > 0 : l ≥ 1} of eigenvalues, and sequences {fkHEs(Rn): k ≥ 1} and {gl ∈ Ds(ℝn) : l ≥ 1} of associated eigenfunctions, respectively, in view of Theorem 4.1 (when taking V(x) 0 and p=p˜=r=2 to work in Hilbert spaces) and Theorem 4.2 (when taking E(x) ≡ V(x) 0 and p = r = 2 to work in Hilbert spaces).

ϱ1, ξ1 are simple, each ϱk,ξl are of finite multiplicities, and the sequences k : k ≥ 1} and l : l ≥ 1} of eigenvalues increase without bound.

f1, g1 are nonnegative, and the sequences {fk : k ≥ 1} and {gl : l ≥ 1} provide orthogonal bases to the spaces HEs(Rn),LK2(Rn) and Ds(Rn),LK2(Rn), respectively.

The procedure is standard, with details left for the interested reader.

5 Proof of Theorem 1.1

First, recall for a weakly convergent sequence {uk:k1}Ds(Rn) having the weak limit u, there are bounded measures μ, ν and constants μi , νi , μ, ν ≥ 0 such that

(5.1) (suk)2dxdμ(su)2dx+iNμiδxi+μδand|uk|2sdxdν=|u|2sdx+iNνiδxi+νδ

in the sense of weakly* convergence of measures, where

(sv)2=(sv(x))2:=Rn(v(x)v(y))2|xy|n+2sdyfor eachvDs(Rn),μ:=limRlim supkBRc(suk)2dxandν:=limRlim supkBRc|uk|2sdx,

δxi denotes the Dirac delta at xiRn, and Sνi2/2sμi for iN and Sν2/2sμ.

We seek a positive solution to (1.1) as the critical point of its energy functional

(5.2) F(u):=12RnRn(u(x)u(y))2|xy|n+2sdxy+12RnEu2dx+1qRnV|u|qdxRnKF+(u)dx12sRn(u+)2sdx,

where F+(u):=0uf+(v)dv0 for f+(u) := f(u) if u ≥ 0 and f+(u) := 0 otherwise through condition (f2). Then, u is a positive weak solution to equation (1.1), provided

(5.3) RnRn(u(x)u(y))(v(x)v(y))|xy|n+2sdxdy+RnEuvdx+RnV|u|q2uvdx={x:u(x)0}Kf+(u)vdx+Rn(u+)2s1vdx,vME,Vs;q,2(Rn).

To see this fact, take v = u := min{u, 0} ∈ ME,Vs;q,2Rn. Notice for each u, u = u+ + u with u+ := max{u, 0} ∈ ME,Vs;q,2Rn and u+ · u 0. Then, we get from (5.3) that

(5.4) 0=RnRn(u(x)u(y))(u(x)u(y))|xy|n+2sdxdy+RnE(u)2dx+RnV|u|qdx=RnRn(u(x))2+(u(y))22u(x)u(y)|xy|n+2sdxdy+RnE(u)2dx+RnV|u|qdx=RnRn(u(x)u(y))22u+(x)u(y)|xy|n+2sdxdy+RnE(u)2dx+RnV|u|qdxRnRn(u(x)u(y))2|xy|n+2sdxdy+RnE(u)2dx+RnV|u|qdx0,

which further implies uME,Vs;q,2(Rn)=0; so, u=u+0 follows immediately.

Now, via condition (f1), f+(u)ε|u|q1+aε|u|2s1 for each ε > 0 and a sufficiently large constant aε > 0 depending on ε; thus, we have

RnKF+(u)dxεqRnK|u|qdx+aε2sK,RnRn|u|2sdx.

From condition (EKV1) and Theorem 4.1, one accordingly derives

F(u)12[u]s,2,Rn2CKεq[u]s,2,Rnq+12uLE2(Rn)2CKεquLE2(Rn)q+1quLVq(Rn)qCKεquLVq(Rn)q12s(1+aε,K)u2s,Rn2s[u]s,2,Rn2(12CKεq[u]s,2,Rnq2C11+aε,K2s[u]s,2,Rn2s2)+uLE2(Rn)2(12CKεquLE2(Rn)q2)+1q(1εCK)uLVq(Rn)q,

so that F(u)ρ0>0 when 0<ρ2uME,Vs;q,2(Rn)ρ for sufficiently small ε, where CK > 0 depends on the embedding ME,Vs;q,2(Rn)LKq(Rn) and aε,K:=aεK,Rn>0.

F(0)=0 and F(w0)<0 for a w0ME,Vs;q,2(Rn) with w0ME,Vs;q,2(Rn)>ρ. So, the standard mountain pass structure is satisfied, and F attains a Palais-Smale sequence at level c for c=infhHmaxt[0,1]F(h(t))>0 with H:={hC([0,1];ME,Vs;q,2(Rn)):h(0)=0,h(1)=w0}.

Below, we find an upper bound for c > 0 via the mountain pass solution v0 > 0 to equation (1.3) seeing ME,Vs;q,2(Rn)LKϑ(Rn). For t ≥ 0, condition (f2) and (1.5) yield

(5.5) F(tv0)t22(RnRn(v0(x)v0(y))2|xy|n+2sdxdy+RnEv02dx)+tqqRnVv0qdxAϑtϑϑRnKv0ϑdx{t22+tqqAϑtϑϑ}RnKv0ϑdxsupt0{t2Aϑtϑϑ}RnKv0ϑdx<s2nSn2s

using a relation similar to (5.3) fulfilled by u = v = v0; thus, 0< c<s2nSn2s.

Now, take {uk : k ≥ 1} to be a Palais-Smale sequence of F at level c in ME,Vs;q,2(Rn); that is, F(uk)c and F(uk)0 in the dual space of ME,Vs;q,2(Rn) as k. Then, one has

c+o(ukME,Vs;q,2(Rn))+o(1)=F(uk)1θF(uk)(uk)(121θ)[uk]s,2,Rn2+(1q1θ)ukLVq(Rn)q+(1θ12s)uk2s,Rn2sη1θRnK1|uk|r1dxη2θRnK2|uk|r2dx+(121θ)ukLE2(Rn)2(121θ)[uk]s,2,Rn2+(1q1θ)ukLVq(Rn)q+(1θ12s)uk2s,Rn2sη1θCK1uk2s,Rnr1η2θCK2[uk]s,2,Rnr2η2θCK2ukLVq(Rn)r2

from condition (f3) using Proposition 4.4 (i) [1], with CK2 > 0 depending only on MVs;q,2(Rn)LK2r2(Rn). Thus, {uk : k ≥ 1} is bounded in ME,Vs;q,2(Rn)Ds(Rn) and L2s(Rn), and there is a subsequence, still denoted by {uk : k ≥ 1}, and a function uME,Vs;q,2(Rn) such that both the estimates in (5.1) hold, and uku in LKq(Rn) and LVq(BR) for each R > 0.

Fix an increasing function χR with χR 0 on |x|R, χR 1 on |x|R2, and 1χRCc1(Rn) (see, for instance, [28, Appenidx I]). Next, from the discussions in [14, Section 2], and noting condition (f1) yields f+(u)bε|u|q1+ε|u|2s1 for each ε > 0 and a sufficiently large constant bε > 0 depending on ε, it follows that

(5.6) 0=limkF(uk)(ukχR)lim supk{RnRn(uk(x)uk(y))2|xy|n+2sχR(x)dxdy+RnRn(uk(x)uk(y))(χR(x)χR(y))|xy|n+2suk(y)dxdy+RnEuk2χRdx+RnV|uk|qχRdxbεRnK|uk|qχRdx(1+εK),RnRn|uk|2sχRdx}.

By virtue of Lemma 3.6 in [14], one has

RnRn(uk(x)uk(y))2|xy|n+2sχR(x)dxdyμ,Rn|uk|2sχRdxν,andRnRn(uk(x)uk(y))(χR(x)χR(y))|xy|n+2suk(y)dxdy0whenR,k;

moreover, RnKukqχRdx0 when R,k as ME.Vs;q,2RnLKqRn. So, one sees from (5.6) that (1 + εK,Rnvμ+vμ for v:=limRlimsupkRnVukqχRdx0 [2]; a similar but simpler analysis shows 1+εK,Rnviμi for each xin. Thus, μi,μSn2s11+εK,Rn22s2 and vi,vSn2s11+εK,Rn2s2s2; so, μi,μ,vi,vSn2s, if they are not zero, by the arbitrariness of ε, which however would lead to a contradiction as follows.

In fact, set :=μRn[u]S,2,Rn2iNμiμ0 to observe that

c=limk{F(uk)1θF(uk)(uk)}(121θ)([u]s,2,Rn2+iNμi+μ+)η2θCK2([u]s,2,Rn2+iNμi+μ+)r22+(1θ12s)(u2s,Rn2s+iNνi+ν)η1θCK1(u2s,Rn2s+iNνi+ν)r12s+(1q1θ)(uLVq(Rn)q+υ)η2θCK2(uLVq(Rn)q+υ)r2q,

which certainly implies only finitely many of μ i , μ , v i , v S n 2 s do not vanish. To illustrate the contradiction, assume without loss of generality that μ,vSn2s. Then, we have

c=limk{F(uk)1θF(uk)(uk)}56(121θ)μ+56(1θ12s)ν+θ262θ([u]s,2,Rn2+iNμi+μ+)η2θCK2([u]s,2,Rn2+iNμi+μ+)r22+2sθ62sθ(u2s,Rn2s+iNνi+ν)η1θCK1(u2s,Rn2s+iNνi+ν)r12s+θqqθ(uLVq(Rn)q+υ)η2θCK2(uLVq(Rn)q+υ)r2q56(1212s)Sn2s3s9nSn2s=5s6nSn2ss3nSn2s=s2nSn2s,

contradicting (5.5); parallel discussions yield contradictions again on μi , νi for all xin.

So, there occurs no evanescence phenomenon and we get ukuME,Vs;q,2Rn.

6 Proof of Theorem 1.2

In this section, we combine the strategies from [7, 8] and Han [31] to find nontrivial positive solutions to (1.6) as the critical points of its energy functional Fλ(u) defined by

(6.1) Fλ(u):=12RnRn(u(x)u(y))2|xy|n+2sdxdy+12RnEu2dx+1qRnV|u|qdxλrRnK(u+)rdx.

Like the analysis in (5.4), u is a positive weak solution to equation (1.6) provided

(6.2) RnRn(u(x)u(y))(v(x)v(y))|xy|n+2sdxdy+RnEuvdx+RnV|u|q2uvdx=λRnK(u+)r1vdx,vME,Vs;q,2(Rn).

Lemma 6.1

Under the assumptions (EKV2-1) or (EKV2-2), the functional Fλ is C1 and is coercive ME,Vs;q,2Rn, so that each sequence {uk : k ≥ 1} of functions with Fλuk bounded has a weakly convergent subsequence in ME,Vs;q,2Rn Moreover, Fλ is sequentially weakly lower semi-continuous in ME,Vs;q,2Rn; that is, when uk ⇀ u ∈ ME.Vs;q,2Rn, for a subsequence relabeled using the same notation, one has Fλ(u)liminfkFλuk.

Proof. The proof of showing FλC1 is standard [3], and the claim regarding the boundedness of Fλuk implying the existence of a weakly convergent subsequence in ME,Vs;q,2Rn follows from the coercivity of Fλ and the reflexivity of ME.Vs;q,2Rn; for the latter, see [7, 8] for details, since now ME,Vs;q,2Rn is a Banach subspace of the Hilbert function space HESRn.

Next, for r1:=w1,r2:=x1,r3:=22sy1 and r4:=111r11r21r3>0 (being true under our conditions (EKV2-1) or (EKV2-2)) in (4.4) of Theorem 4.2, one has

(6.3) λrRnK(u+)rdxλrRnK|u|rdx(r14RnEu2dx)1r1(r22qRnV|u|qdx)1r2(r34RnRn(u(x)u(y))2|xy|n+2sdxdy)1r3×{(λC1r)r4(4r3)r4r3(2qr2)r4r2(4r1)r4r1(RnKψ2s(β,κ)EβVκdx)r4 ψ2s(β,κ)}1r414RnRn(u(x)u(y))2|xy|n+2sdxdy+14RnEu2dx+12qRnV|u|qdx+λr4CEKV

by Young’s inequality for an absolute constant CEKV > 0 independent of λ, u. So,

Fλ(u)C4uME,Vs;q,2Rnλr4CEKVC4

for some constants C4,C4>0 as q>2, which implies the coercivity of F.

Since Fλ is coercive, each sequence {uk : k ≥ 1} of functions in ME.Vs;q,2Rn with bounded Fλuk has a weakly convergent subsequence, written again as {uk : k ≥ 1}, such that ukuME,Vs;q,2Rn. The weakly lower semi-continuity of norms in DSRn,LE2Rn and LVqRn, along with the compact embedding ME,Vs;q,2RnLKrRn by Theorems 4.2 and 4.3, leads to the sequentially weak lower semi-continuity of Fλ, which concludes the proof.

Define

(6.4) λ˜:=infuME,Vs;q,2Rnu+LKrRn=1r2RnRn(u(x)u(y))2|Xy|n+2sdxdy+r2RnEu2dx+rqRnV|u|qdx.

Then, one has λ˜>0. Actually, if not, there would exist a sequence ul:l1ME,Vs;q,2Rn with ul+LKrRn=1 such that

r2RnRnul(x)ul(y)2|xy|n+2sdxdy+r2RnEul2dx+rqRnVulqdx0;

so, ulME.Vs;q,2Rn0, contradicting the compact embedding ME,Vs;q,2RnLKrRn.

Define λ* to be the supermum of λ such that equation (1.6) only has the trivial nonnegative solution for each ι < λ, and λ** to be the infimum of λ such that equation (1.6) has at least a nontrivial positive solution at λ. Then, 0λ=λλ˜. As a matter of fact,

λRnKvλ+rdx>r2RnRnvλ(x)vλ(y)2|xy|n+2sdxdy+r2RnEvλ2dx+rqRnVvλqdx

holds for all λ>λ˜ with some vλME,Vs;q,2Rn by homogeneity, and consequently Fλvλ<0, which along with Lemma 6.1 leads to Fλuλ=infuME,Vs;q,2RnFλ(u)Fλvλ<0 for an uλ ≥ 0 in ME,Vs;q,2Rn that is a nontrivial

positive solution to equation (1.6), since FλuλFλuλ. So, we have λλ˜. On the other hand, if λ* > λ**, we would find a λλ,λ such that problem (1.6) has at least a nontrivial positive solution at λ according to the definition of λ**, which however is against the definition of λ*; if λ* < λ**, we would find a λ (λ*, λ**] such that problem (1.6) has at least a nontrivial positive solution at some l<λ according to the definition of λ*, which however is against the definition of λ**. Thus, λ* = λ**.

Write λ1 := λ* = λ** in the sequel.

Proposition 6.2

Under our conditions (EKV2-1) or (EKV2-2), λ1 ≥ 0 and equation (1.6) has a nontrivial positive solution uλ ≥ 0 in ME,Vs;q,2Rn for all λ > λ1.

Proof. By definition, λ1 = λ*; so, if uλ is a nontrivial positive solution to (1.6) in ME,Vs;q,2Rn, then λλ1. Now, we show (1.6) has at least one nontrivial solution uλ ≥ 0 in ME,Vs;q,2Rn for all λ > λ1 combining Struwe [50, Theorem 2.4], [8, Theorem 4.2] and [31, Proposition 3.3].

By definition, λ1 = λ**; so, there is an ι ∈ [λ1, λ) such that (1.6) has a nontrivial solution uι ≥ 0 in ME,Vs;q,2Rn which of course is a subsolution to (1.6) at λ. Consider the constrained minimization problem infuMFλ(u) for M:=uME,Vs;q,2Rn:uul0. Notice M is closed and convex, so that it is weakly closed in ME,Vs;q,2Rn. Thus, Lemma 6.1 ensures the attainment of a minimizer of Fλ in M;  that is, there is an uλ(≥ uι ≥ 0) in M with Fλuλ=infuMFλ(u). Take φCc1Rn, and set φε := max{0, uιuλ + εφ} ≥ 0 and vε := φε + uλεφ(≥ uι ≥ 0) in M for all ε > 0. So, one has FλuλuλFλuλvε that further implies

(6.5) Fλuλ(φ)1εFλuλφε.

Put Ωε:=xRn:φε(x)>0=xRn:uλ(x)εφ(x)<ut(x)suppφ+. Since uι is a subsolution to (1.6) at λ and φε ≥ 0, Fλulφε0 follows and one has [4]

FλuλφεFλuλφεFλutφε=Rn×Rn(ω(χ)ω(y))φε(x)φε(y)|χy|n+2sdxdy+RnEuλulφεdx+RnVuλq1ulq1φεdxλRnKuλr1utr1φεdx=Ωεc×Ωεcc(ω(x)ω(y))φε(x)φε(y)|xy|n+2sdxdy+ΩεEuλutφεdx+ΩεVuλq1utq1φεdxλΩεKuλr1ulr1φεdxεΩεc×Ωεcc(ω(x)ω(y))(φ(x)φ(y))|xy|n+2sdxdyΩεc×Ωεcc(ω(x)ω(y))2|Xy|n+2sdxdy+ΩεEuλφεdx+ΩεEulφεdx+ΩεVuλq1φεdx+ΩεVulq1φεdxεΩε×Ωε(ω(x)ω(y))(φ(x)φ(y))|χy|n+2sdxdy+2εΩε×Ωεc(ω(x)ω(y))(φ(x)φ(y))|xy|n+2sdxdy+εΩεEuλ|φ|dx+ΩεEuι|φ|dx+ΩεVuλq1|φ|dx+ΩεVulq1|φ|dx2εΩε×Rn(ω(x)ω(y))(φ(x)φ(y))|xy|n+2sdxdy+εφLE2ΩεuλLE2Ωε+uιLE2Ωε+φLVqΩεuλLVqΩεq1+uιLVqΩεq1=2εΩε×BR(ω(x)ω(y))(φ(x)φ(y))|xy|n+2sdxdy+2εΩε×BRc(ω(x)ω(y))(φ(x)φ(y))|xy|n+2sdxdy+εφLE2ΩεuλLE2Ωε+uLE2Ωε+φLvqΩεuλLVqΩεq1+utLVqΩεq12εΩε×BR(ω(x)ω(y))(φ(x)φ(y))|xy|n+2sdxdy+2εBR×BRc(ω(x)ω(y))(φ(x)φ(y))|xy|n+2sdxdy
+εφLE2ΩεuλLE2Ωε+ulLE2Ωε+φLVqΩεuλLVqΩεq1+uLVqΩεq1

with ω := uλuι ≥ 0, seeing 0 < φεε|φ| on Ωε; that is, we have Fλuλφεo(ε) when R → ∞ and ε → 0+. This combined with (6.5) yields Fλuλ(φ)0 for all φCc1Rn; so, we also get Fλuλ(φ)0 via symmetry. By density, it follows that Fλuλ(v)=0 for each vMF.Vs;q,2Rn, and hence uλ(≥ uι ≥ 0) is a nontrivial solution to (1.6) at λ.

Proposition 6.2 obviously provides the proof for the first part of Theorem 1.2. Now, we will proceed to discuss the second part of Theorem 1.2 by first giving some estimates for solutions to equation (1.6) in general, which are presented as the result below.

Lemma 6.3

Under the assumptions (EKV2-1) or (EKV2-2), each solution uλ to equation (1.6) in ME,Vs;q,2Rn satisfies

(6.6) RnRnuλ(x)uλ(y)2|Xy|n+2sdxdy+RnEuλ2dx+RnVuλqdxλr4CEKV.

where CEKV>0 is an absolute constant independent of λ, u. Moreover, when the assumption (EK) also holds, there are absolute constants CEK,C˜EKV>0 such that λ1C˜EKV>0 and such that each nontrivial solution uλ to equation (1.6) in ME,Vs;q,2Rn satisfies

(6.7) RnKuλrdxλCEK2rr2r.

Proof. First, (6.6) follows from the fact that each solution uλ to (1.6) satisfies

(6.8) RnRnuλ(x)uλ(y)2|xy|n+2sdxdy+RnEuλ2dx+RnVuλqdx=λRnKuλrdx

and an estimate akin to (6.3), which is left as an easy exercise for the reader.

Now, when our condition (EK) also holds, from Proposition 4.4 (ii) and for uME,Vs;q,2Rn with an absolute constant CEK > 0, one has

(6.9) RnK|u|rdxCEKRnRn(u(x)u(y))2|Xy|n+2sdxdy+RnEu2dxr2.

Combining (6.8) and (6.9), one observes, for each nontrivial solution uλ to (1.6),

RnKuλrdx2rλCEK2rRnKuλrdx,

which in turn yields (6.7). Also, by (6.6), (6.7) and (6.9), we get λCEK2r22rλr4CEK2rCEKV, so that λC˜EKV>0 as 2 < r, which in particular leads to λ1C˜EKV>0.

Finally, we are ready to discuss the second twofold claim of Theorem 1.2.

Proposition 6.4

Under our conditions (EKV2-1) and (EK), we have λ1 > 0 and equation (1.6) has a nontrivial positive solution uλ ≥ 0 in ME,Vs;q,2Rn if and only if λλ1; besides, for λ2:=λ˜λ1>0 as given in (6.4), equation (1.6) has at least two distinct nontrivial positive solutions uλ,u˜λ0 in ME,Vs;q,2Rn for all λ > λ2.

Proof. Note if uλ ≥ 0 is a nontrivial positive solution to (1.6) in ME,Vs;q,2Rn, then λλ1 > 0; so, we are left to show (1.6) has a nontrivial positive solution at λ1. Let (k) > λ1 : k ≥ 1} decrease to λ1, with uλ(k)0:k1 an associated sequence of nontrivial solutions to (1.6) that is bounded in ME.Vs;q,2Rn by (6.6). Then, there exists a subsequence uλ(k)0:k1, using the same notation, such that uλ(k)w in HESRn,uλ(k)w in LVqRn,uλ(k)w in LKΥRn, and uλ(k)w a.e. on ℝn for a function w ≥ 0 in ME,Vs;q,2Rn. Thus, one has

limkRnKuλ(k)r1vdx=RnKwr1vdx,vME,Vs;q,2Rn.

Keep in mind Fλ(k)uλ(k)=0; that is, (6.2) holds for u = uλ(k) and λ = λ(k). Since Fλ(w) is a continuous linear functional on ME,Vs;q,2Rn, it follows that

0Fλ(k)uλ(k)uλ(k)w+λ(k)RnKuλ(k)r1uλ(k)wdxFλ(w)uλ(k)wλRnKwr1uλ(k)wdx=RnRn(ϖ(x)ϖ(y))2|xy|n+2sdxdy+RnEuλ(k)w2dx+RnVuλ(k)q1wq1uλ(k)wdxuλ(k)ws,2,Rn2+uλ(k)wLE2Rn2+Cquλ(k)wLVqRnq0 as k

for ϖ:=uλ(k)w and an absolute constant Cq > 0 (see Han [29, Lemma 3.2]); so, uλ(k)w in HESRn and LVqRn. Therefore, (6.2) is satisfied by w and λ for all vME,Vs;q,2Rn upon taking the limit k → ∞. Using (6.7), one sees RnKwrdxλ(1)CEK2rr2r>0 by virtue of the compact embedding MF.Vs;q,2RnLKrRn. So, w ≥ 0 is a nontrivial positive solution in MFVs;q,2Rn to equation (1.6); that is, w = uλ1 in common practice notation.

On the other hand, for each λ > λ2, there is a solution uλ ≥ 0 to (1.6) with Fλuλ<0. Furthermore, it is easily seen from (6.9) that, for some constant CEK>0,

Fλ(u)14uHEsRn2λrCEKuHEsRnruHEsRn214λrCEKuHEsRnr2,

and thus Fλ(u)ρ˜0>0 provided u H E s R n = ρ ~ < min u λ H E s R n , r 4 λ C E K 1 r 2 . So, via the mountain pass theorem of Candela and Palmieri [19, Theorem 2.5] (see also [7, Theorem A.3]), there exists a sequence {ul : l ≥ 1} in ME,Vs;q,2Rn with Fλulc>0 and Fλul0 in the dual space of ME,VS;q,2Rn when l → ∞ for c=infhHλmaxt[0,1]Fλ(h(t))>0 with Hλ:={hC([0,1]; ME,Vs;q,2Rn:h(0)=0,h(1)=uλ, Lemma 6.1 provides a subsequence {ul : l ≥ 1}, using the same notation, such that u1w˜ in HESRn,u1w˜ in LVqRn,u1w˜ in LKrRn, and ulw˜ a.e. on ℝn for a function w˜MF.Vs;q,2Rn. Similar analysis then yields ulw˜ in ME,Vs;q,2Rn; that is, u˜λ:=W˜0 is a nontrivial solution to (1.6) in ME,Vs;q,2Rn, as Fλu˜λ=0 and thus (6.2) is satisfied, which is distinct from uλ since Fλu˜λ=c>0.

A Appendix

This section provides an additional analysis for Subsection 2.1. Recall Ω denotes a bounded domain having a compact, Lipschitz boundary Ω. Note Lq(Ω) → L1(Ω). Using Minkowski’s inequality and Lemma 3.1 of Bellido and Mora-Corral [11], we have

(A.1) up,Ωuuˉp,Ω+uˉp,ΩC5[u]s,p,Ω+u1,ΩC5[u]s,p,Ω+uq,Ω,uMs;q,p(Ω) and 1q

with uˉ:=1L(Ω)Ωudx and C5, C5>0 some constants depending on n, p, q, s, Ω. Thus, (2.3) follows from (A.1) and (2.1) consequently; that is, Ms;q,p(Ω) → Ws,p(Ω).

On the other hand, seeing Ws,p(Ω) → Lq(Ω) for 1qps when sp < n, one accordingly has Ws,p(Ω) → Ms;q,p(Ω), which together with the preceding analysis yields (2.2). Moreover, noticing Ws,p(Ω) → Lq(Ω) for 1 ≤ q < ∞or1 ≤ q ≤ ∞when sp = n or sp > n, the preceding analysis then leads to (2.4) and (2.6) respectively.


Dedicated to

In loving memory of my father Jiaxing Han (June 5, 1952–April 9, 2019).


  1. Conflict of interest

    Conflict of interest statement: There is no conflict of interest.

Acknowledgement

The author is greatly indebted to the anonymous referees for helpful suggestions. The author gratefully acknowledges the partial financial support of the Research Council Grant #21870120011 plus the 2017–2021 faculty research fellowships from the College of Arts and Sciences at Texas A&M University-San Antonio.

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Received: 2020-05-06
Accepted: 2021-04-07
Published Online: 2021-09-04

© 2021 Qi Han, published by De Gruyter

This work is licensed under the Creative Commons Attribution 4.0 International License.

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